title: "1825 Klare" content: 1825 Klare 1825 Klare, provisional designation , is an asteroid from the central region of the asteroid belt, approximately 15 kilometers in diameter. It was discovered on 31 August 1954, by German astronomer Karl Reinmuth at Heidelberg Observatory in southern Germany. The asteroid was named after Heidelberg astronomer Gerhard Klare. The presumably stony asteroid orbits the Sun in the central main-belt at a distance of 2.4–3.0 AU once every 4 years and 5 months (1,600 days). Its orbit has an eccentricity of 0.11 and an inclination of 4° with respect to the ecliptic. First identified as at Uccle Observatory in


title: "1825 Klare" content: 1934, "Klare"s observation arc begins 20 years prior to its official discovery observation. "Klare" has been the subject of multiple photometric lightcurve studies, which gave a well-determined rotation period between 4.741 and 4.744 hours with a brightness variation between 0.70 and 0.90 magnitude (). Measurements have also been used as the basis for generating a three-dimensional model of its shape. The "Collaborative Asteroid Lightcurve Link" (CALL) adopts a period 4.744 hours with an amplitude of 0.70 magnitude (). According to the survey carried out by the Japanese Akari satellite, "Klare" measures 14.69 kilometers in diameter, and its surface has an


title: "1825 Klare" content: albedo of 0.167, while CALL assumes an albedo of 0.10 – a compromise value for asteroids with a semi-major axis between 2.6 and 2.7 AU, for which neither a S (0.20) nor a C (0.057) type has been determined – and calculates a diameter of 19.21 kilometers with an absolute magnitude of 11.7. "Klare" was named after Gerhard Klare (born 1932), an observing astronomer at Heidelberg Observatory since 1960, whose fields of interest include minor planets. He is also known for his numerous contributions in the yearbook series "Reviews in Modern Astronomy" of the Astronomische Gesellschaft. The official naming citation


title: "1825 Klare" content: was published by the Minor Planet Center before November 1977 (). 1825 Klare 1825 Klare, provisional designation , is an asteroid from the central region of the asteroid belt, approximately 15 kilometers in diameter. It was discovered on 31 August 1954, by German astronomer Karl Reinmuth at Heidelberg Observatory in southern Germany. The asteroid was named after Heidelberg astronomer Gerhard Klare. The presumably stony asteroid orbits the Sun in the central main-belt at a distance of 2.4–3.0 AU once every 4 years and 5 months (1,600 days). Its orbit has an eccentricity of 0.11 and an inclination of 4° with


title: "1850 Kohoutek" content: 1850 Kohoutek 1850 Kohoutek, provisional designation , is a stony Florian asteroid from the inner regions of the asteroid belt, approximately 6 kilometers in diameter. It was named after Czech astronomer Luboš Kohoutek. "Kohoutek" was discovered during World War II on 23 March 1942, by German astronomer Karl Reinmuth at Heidelberg Observatory in southwest Germany, Ten days prior to its discovery, the body was observed at Turku Observatory, Finland. However, these observations are not considered for the asteroid's orbital computation and its observation arc begins with the discovery observation at Heidelberg. Since the discovery was made in the second half


title: "1850 Kohoutek" content: of March, the letter "E" in the provisional designation is erroneous. It should have been "F", but the initially incorrect assignment has persisted. It is a member of the Flora family, one of the largest families of stony asteroids in the asteroid belt. It orbits the Sun in the inner main-belt at a distance of 2.0–2.5 AU once every 3 years and 5 months (1,233 days). Its orbit has an eccentricity of 0.13 and an inclination of 4° with respect to the ecliptic. In December 2014, a rotational lightcurve of "Kohoutek" was obtained from photometric observations in the R-band at


title: "1850 Kohoutek" content: the Palomar Transient Factory in California. Lightcurve analysis gave a rotation period of 3.68 hours with a brightness variation of 0.31 magnitude (). According to the survey carried out by NASA's Wide-field Infrared Survey Explorer with its subsequent NEOWISE mission, "Kohoutek" measures 5.91 and 7.64 kilometers in diameter, and its surface has an albedo of 0.181 and 0.383, respectively. The "Collaborative Asteroid Lightcurve Link" assumes an albedo of 0.24 – derived from 8 Flora, a S-type asteroid and the family's largest member and namesake – and calculates a diameter of 6.05 kilometers with an absolute magnitude of 13.26. This minor


title: "1850 Kohoutek" content: planet was named in honor of the Czech astronomer, Luboš Kohoutek (b. 1935), former staff member of the Hamburg-Bergedorf Observatory and prolific observer and discoverer of minor planets and comets, most notably 75D/Kohoutek, 76P/West–Kohoutek–Ikemura, and the long-period Comet Kohoutek. He has also contributed in the fields of planetary nebulae and emission-line stars. The approved naming citation was published by the Minor Planet Center before November 1977 (). 1850 Kohoutek 1850 Kohoutek, provisional designation , is a stony Florian asteroid from the inner regions of the asteroid belt, approximately 6 kilometers in diameter. It was named after Czech astronomer Luboš Kohoutek.


title: "Lost (TV series)" content: Catholic priest played by Adewale Akinnuoye-Agbaje; Ana Lucia Cortez, an airport TSA guard and former LAPD police officer played by Michelle Rodriguez; and Libby Smith, a purported clinical psychologist and formerly mentally ill woman portrayed by Cynthia Watros. Ana Lucia and Libby were written out of the series toward the end of season two after being shot by Michael, who then left the island along with his son. In season three, two actors were promoted from recurring to starring roles: Henry Ian Cusick as former Scottish soldier Desmond Hume; and Michael Emerson as the manipulative leader of the Others, Ben


title: "Kirkpatrick baronets" content: Kirkpatrick baronets The Kirkpatrick Baronetcy, of Closeburn in the County of Dumfries, is a title in the Baronetage of Nova Scotia. It was created on 26 March 1685 for Thomas Kirkpatrick, with remainder to heirs male whatsoever. The family seat of the Kirkpatrick family was Closeburn Castle, Dumfriesshire. Charles Kirkpatrick (1879–1955), grandson of Roger Kirkpatrick, second son of fourth Baronet, was a Major-General in the British Army. His son Herbert James Kirkpatrick (1910–1977) was an Air Vice-Marshal in the Royal Air Force. Sir James Kirkpatrick, 8th Baronet was a keen amateur footballer in his youth and appeared in goal for


title: "Kirkpatrick baronets" content: the Wanderers in the 1878 FA Cup Final. Kirkpatrick baronets The Kirkpatrick Baronetcy, of Closeburn in the County of Dumfries, is a title in the Baronetage of Nova Scotia. It was created on 26 March 1685 for Thomas Kirkpatrick, with remainder to heirs male whatsoever. The family seat of the Kirkpatrick family was Closeburn Castle, Dumfriesshire. Charles Kirkpatrick (1879–1955), grandson of Roger Kirkpatrick, second son of fourth Baronet, was a Major-General in the British Army. His son Herbert James Kirkpatrick (1910–1977) was an Air Vice-Marshal in the Royal Air Force. Sir James Kirkpatrick, 8th Baronet was a keen amateur footballer


title: "Bilkent Concert Hall" content: area of nearly 14.500 m2. The concert hall stage includes a stage lift which allows for the formation an orchestra pit used in operas. Two Steinway concert grand pianos are available. The interior walls of the concert hall are coated with movable acoustic panels, which make the concert hall a recording studio as well. The building hosts concerts in its concert hall for 750 seats and its foyer, performances of theatre students in its arena theatre for 200 seats and houses studios, seminar rooms, classrooms, a cafeteria and a café. Bilkent Concert Hall Bilkent Concert Hall () is a performing


title: "Fated to Love You (2008 TV series)" content: Times I Love Him" by Shorty Yuen, while the ending theme song is by Quack Wu () and Shorty Yuen entitled "心願便利貼" or "Sticky Note With Wishes". The track, "心願便利貼" (Sticky Note With Wishes) was listed at number 50 on Hit Fm Taiwan's "Hit Fm Annual Top 100 Singles Chart" (Hit-Fm年度百首單曲) for 2008. A 2014 South Korean remake of the same title starred Jang Hyuk and Jang Na-ra in the lead roles. A 2017 Thailand remake starred Esther Supreeleela and Sukrit Wisetkaew on ONE HD 31 entitled "You're My Destiny". The remake was broadcast in the Philippines by GMA network


title: "Lehigh Valley Transit Company" content: extensive rebuilding of the Allentown to Philadelphia route. Much side of road track (the line was always a single track) was replaced by track running in open country, however considerable older side-of-road trackage remained, particularly south of Quakertown. Heavy wood arch windowed interurban coaches were purchased for high speed operation. This upgrading program culminated in a high capacity interurban line running from Allentown to Norristown. It existed until 1951. Multiple car Interurbans operated from Allentown to Philadelphia's 69th Street terminal using the Philadelphia and Western Railroad south of Norristown starting in December 1912. Service on the former Inland Traction route


title: "1212 Francette" content: 1212 Francette 1212 Francette, provisional designation , is a dark Hildian asteroid from the outermost regions of the asteroid belt, approximately 82 kilometers in diameter. It was discovered on 3 December 1931, by French astronomer Louis Boyer at the Algiers Observatory in Algeria, North Africa, who named it after his wife Francette Boyer. "Francette" is a member of the small Hilda family (), an asteroid family within the dynamical Hilda group, that stays in an orbital resonance with the gas giant Jupiter. It orbits the Sun in the outermost asteroid belt at a distance of 3.2–4.7 AU once every 7


title: "1250 Galanthus" content: 1250 Galanthus 1250 Galanthus, provisional designation , is a dark background asteroid from the central regions of the asteroid belt, approximately 20 kilometers in diameter. It was discovered on 25 January 1933, by German astronomer Karl Reinmuth at the Heidelberg Observatory. The asteroid was named for the herbaceous plant "Galanthus", also known as "snowdrop". "Galanthus" is a non-family asteroid from the main belt's background population. It orbits the Sun in the central main-belt at a distance of 1.9–3.2 AU once every 4 years and 1 month (1,488 days; semi-major axis of 2.55 AU). Its orbit has an eccentricity of 0.27


title: "1250 Galanthus" content: and an inclination of 15° with respect to the ecliptic. The body's observation arc begins at Heidelberg the night after its official discovery observation. "Galanthus" is an assumed carbonaceous C-type asteroid. In the early 1980s, a rotational lightcurve of "Galanthus" was obtained during a survey conducted by Richard P. Binzel at the McDonald Observatory, Texas. Lightcurve analysis gave a well-defined rotation period of 3.92 hours with a brightness variation of 0.28 magnitude (). The period was confirmed from photometric observations by astronomers at the Palomar Transient Factory in October 2015, which gave a similar period of 3.918 hours and an


title: "1250 Galanthus" content: amplitude of 0.22 magnitude (). According to the surveys carried out by the Infrared Astronomical Satellite IRAS, the Japanese Akari satellite and the NEOWISE mission of NASA's Wide-field Infrared Survey Explorer, "Galanthus" measures between 17.18 and 21.00 kilometers in diameter and its surface has an albedo between 0.04 and 0.06. The "Collaborative Asteroid Lightcurve Link" adopts the results obtained by IRAS, that is, an albedo of 0.0500 and a diameter of 21.0 kilometers based on an absolute magnitude of 12.26. This minor planet was named after the herbaceous plant "Galanthus", also known as "snowdrop". The official naming citation was mentioned


title: "1250 Galanthus" content: in "The Names of the Minor Planets" by Paul Herget in 1955 (). Due to his many discoveries, Karl Reinmuth submitted a large list of 66 newly named asteroids in the early 1930s. The list covered his discoveries with numbers between and . This list also contained a sequence of 28 asteroids, starting with 1054 Forsytia, that were all named after plants, in particular flowering plants "(also see list of minor planets named after animals and plants)". 1250 Galanthus 1250 Galanthus, provisional designation , is a dark background asteroid from the central regions of the asteroid belt, approximately 20 kilometers


title: "1958 Miles" content: 1958 Miles 1958 Miles is a compilation album by American jazz musician Miles Davis, released in 1974 on CBS/Sony. Recording sessions for the album took place on May 26, 1958, at Columbia's 30th Street Studio and September 9, 1958, at the Plaza Hotel in New York City. "1958 Miles" consists of three songs featured on side two of the LP album "Jazz Track", which was released earlier in 1958, one song from the same session not appearing in the album (Love for Sale), and three recordings from Davis' live performance at the Plaza Hotel with his ensemble sextet. The recording


title: "Vehicle registration plates of Honduras" content: 12 inches. The initial letter or (two letters) identify the class of vehicle (see table), followed by a four- or five-digit serial number. Personal, commercial and trailer tags also have a one- or two-letter serial letters. The letter Ñ is included in the alphabet used for the serial letters. Light truck license plates in the PP format do not have the map of Honduras in the background. Vehicle registration plates of Honduras License plates of Honduras are issued by the Honduran Secretaría de Obras Públicas, Transporte y Vivienda (SOPTRAVI, the Ministry of Public Works, Transport and Living) and identify motor


title: "1870 Glaukos" content: 1870 Glaukos 1870 Glaukos ( ), provisional designation "", is a mid-sized Jupiter trojan from the Trojan camp, approximately in diameter. Discovered during the first Palomar–Leiden Trojan survey in 1971, it was later named for Glaucus from Greek mythology. The dark D-type asteroid has a rotation period of 6.0 hours. "Glaukos" was discovered on 24 March 1971, by Dutch astronomer couple Ingrid and Cornelis van Houten at Leiden, on photographic plates taken by astronomer Tom Gehrels at the Californian Palomar Observatory in California. The body's observation arc begins with a precovery of its first recorded observation at Palomar in November


title: "1870 Glaukos" content: 1955, or more than 15 years prior to its official discovery observation. This discovery was made in the context of a larger survey of faint Trojans. The trio of Dutch and Dutch–American astronomers also collaborated on the productive Palomar–Leiden survey in the 1960s, using the same procedure as for this (smaller) survey: Tom Gehrels used Palomar's Samuel Oschin telescope (also known as the 48-inch Schmidt Telescope), and shipped the photographic plates to Cornelis and Ingrid van Houten at Leiden Observatory where astrometry was carried out. More than 7000 Jupiter trojans have already been discovered. "Glaukos" is a dark Jovian asteroid


title: "1870 Glaukos" content: in a 1:1 orbital resonance with Jupiter. It is located in the trailering Trojan camp at the Gas Giant's Lagrangian point, 60° behind its orbit . It is also a non-family asteroid of the Jovian background population. It orbits the Sun at a distance of 5.1–5.4 AU once every 12.02 years (4,389 days; semi-major axis of 5.25 AU). Its orbit has an eccentricity of 0.03 and an inclination of 7° with respect to the ecliptic. "Glaukos" has been characterized as a dark D-type asteroid by PanSTARRS photometric survey as well as in the SDSS-based taxonomy. It is the most common


title: "1823 Gliese" content: 1823 Gliese 1823 Gliese, provisional designation , is a stony Flora asteroid from the inner regions of the asteroid belt, approximately 8 kilometers in diameter. It was discovered on 4 September 1951, by German astronomer Karl Reinmuth at Heidelberg Observatory in southern Germany. The asteroid was named after German astronomer Wilhelm Gliese. The S-type asteroid is a member of the Flora family, one of the largest groups of stony asteroids in the main-belt. It orbits the Sun in the inner main-belt at a distance of 1.9–2.5 AU once every 3 years and 4 months (1,213 days). Its orbit has an


title: "1823 Gliese" content: eccentricity of 0.14 and an inclination of 3° with respect to the ecliptic. The first unused observations date back to 1944 at Johannesburg Observatory, when it was identified as . The first used precovery was taken at the discovering Heidelberg observatory in 1950, extending the asteroid's observation arc by one year prior to its official discovery. A rotational lightcurve of this asteroid was obtained from photometric observations made by Czech astronomer Petr Pravec at the Ondřejov Observatory in August 2014. The lightcurve gave a well-defined rotation period of hours with a brightness variation of 0.27 in magnitude (). One month


title: "1823 Gliese" content: later, in September 2014, a second lightcurve by American astronomer Brian Warner at his Palmer Divide Observatory, Colorado, gave a concurring period of hours with an amplitude of 0.23 in magnitude (). According to the survey carried out by the NEOWISE mission of NASA's space-based Wide-field Infrared Survey Explorer, the asteroid measures 8.4 and 9.5 kilometers in diameter and its surface has an albedo of 0.189 and 0.135, respectively, while the "Collaborative Asteroid Lightcurve Link" assumes an albedo of 0.24 – derived from 8 Flora, the largest member and namesake of this asteroid's orbital family – and calculates a diameter


title: "1823 Gliese" content: of 8.2 kilometers with an absolute magnitude of 12.6. This minor planet was named after German astronomer Wilhelm Gliese (1915–1993) at the Astronomisches Rechen-Institut. Gliese is widely known for having compiled about 1,000 stars located within 25 parsecs of Earth into the Gliese Catalogue of Nearby Stars. The official naming citation was published by the Minor Planet Center before November 1977 (). A large number of Exoplanets derive their names form this star catalogue. 1823 Gliese 1823 Gliese, provisional designation , is a stony Flora asteroid from the inner regions of the asteroid belt, approximately 8 kilometers in diameter. It


title: "Hamish & Andy (radio show)" content: Business Brunch logo on them. The "Mug God" (a character voiced by Hamish) had the final say on who received a coveted mug. A series of "Mug Commandments" were developed by the Mug God, mostly to prevent people who expressly asked for a mug from being eligible to receive one. Some listeners attempted to trap Hamish & Andy into giving them a mug, while many were given away as a reward for games developed by Hamish & Andy. One such game resulted in a caller receiving a mug for correctly guessing that a Babysitter's Club plotline, in which two of


title: "Hamish & Andy (radio show)" content: have included: Hamish & Andy have released two ARIA Award-winning double-disc compilation albums, featuring highlights from "The Hamish & Andy Show". Hamish & Andy have won many awards throughout their decorated career. Hamish & Andy (radio show) The Hamish & Andy Show (Hamish and Andy) was an Australian radio show and currently ongoing podcast created by and starring comedic duo Hamish Blake and Andy Lee. It began on Fox FM in 2006 and, by 2007, was broadcast on the Hit Network to every state in Australia as well as the ACT for two hours in the key weekday afternoon drive


title: "1650 Heckmann" content: 1650 Heckmann 1650 Heckmann, provisional designation , is a rare-type Nysian asteroid from the inner regions of the asteroid belt, approximately 29 kilometers in diameter. It was discovered on 11 October 1937, by German astronomer Karl Reinmuth at Heidelberg Observatory in southern Germany, and later named after astronomer Otto Heckmann. "Heckmann" is a member of the Polanian subgroup of the Nysa family of asteroids and shows a rare F-type spectrum in the Tholen classification scheme. It orbits the Sun in the inner main-belt at a distance of 2.0–2.8 AU once every 3 years and 10 months (1,389 days). Its orbit


title: "1650 Heckmann" content: has an eccentricity of 0.16 and an inclination of 3° with respect to the ecliptic. "Heckmann" was first identified as at the discovering observatory in 1906. Its first used observation was taken at Heidelberg in 1909, when it was identified as , extending the body's observation arc by 28 years prior to its official discovery observation. French amateur astronomer René Roy obtained the first rotational lightcurve of "Heckmann" in September 2005. It gave a rotation period of 12.05 hours with a brightness variation of 0.06 in magnitude (). A more refined lightcurve with a period of 14.893 hours and an


title: "1650 Heckmann" content: amplitude of 0.16 magnitude was obtained by Australian amateur astronomer David Higgins at the Hunters Hill Observatory and collaborating stations in March 2008 (). In September 2013, photometric observations at the Palomar Transient Factory, California, gave a low rated lightcurve with a similar period of 14.9042 hours (). According to the surveys carried out by the Infrared Astronomical Satellite IRAS, the Japanese Akari satellite, and NASA's Wide-field Infrared Survey Explorer with its subsequent NEOWISE mission, "Heckmann" measures between 24.93 and 35.15 kilometers in diameter, and its surface has an albedo between 0.034 and 0.06. The "Collaborative Asteroid Lightcurve Link" agrees


title: "1650 Heckmann" content: with the results obtained by IRAS, that is an albedo of 0.0497 and a diameter of 29.07 kilometers with an absolute magnitude of 11.56. This minor planet was named in honor of German astronomer Otto Heckmann (1901–1983), director of the Bergedorf Observatory in Hamburg, president of the International Astronomical Union (1967–1970) and the first director of ESO, the European Southern Observatory, which foundation had been initiated by him. He was active in the fields of cosmology and several aspects of fundamental astronomy. The approved naming citation was published by the Minor Planet Center before November 1977 (). 1650 Heckmann 1650


title: "1924 Horus" content: 1924 Horus 1924 Horus, provisional designation , is a dark asteroid from the inner regions of the asteroid belt, approximately 12 kilometers in diameter. Discovered during the Palomar–Leiden survey in 1960, it was later named after Horus from Egyptian mythology. "Horus" was discovered on 24 September 1960, by Cornelis Johannes van Houten and Ingrid van Houten-Groeneveld at Leiden, on photographic plates taken by Tom Gehrels at Palomar. On the same date, the trio of astronomers also discovered 1912 Anubis, 1923 Osiris and 5011 Ptah. The survey designation "P-L" stands for "Palomar–Leiden", named after Palomar Observatory and Leiden Observatory, which collaborated


title: "1924 Horus" content: on the fruitful Palomar–Leiden survey in the 1960s. Gehrels used Palomar's Samuel Oschin telescope (also known as the 48-inch Schmidt Telescope), and shipped the photographic plates to Ingrid and Cornelis van Houten at Leiden Observatory where astrometry was carried out. The trio are credited with the discovery of . According to the survey carried out by NASA's Wide-field Infrared Survey Explorer with its subsequent NEOWISE mission, "Horus" measures 12.986 kilometers in diameter and its surface has an albedo of 0.070. The body has a rotation period of 6.183 hours. This minor planet was named after Horus, the falcon-headed king of


title: "1842 Hynek" content: 1842 Hynek 1842 Hynek, provisional designation , is a stony Florian asteroid from the inner regions of the asteroid belt, approximately 8 kilometers in diameter. The asteroid was discovered on 14 January 1972 by Czech astronomer Luboš Kohoutek at Hamburg Observatory, who named it after his father, Hynek Kohoutek. "Hynek" is member of the Flora family. It orbits the Sun in the inner main-belt at a distance of 1.9–2.7 AU once every 3 years and 5 months (1,246 days). Its orbit has an eccentricity of 0.18 and an inclination of 5° with respect to the ecliptic. First identified as at


title: "1842 Hynek" content: Heidelberg, the asteroid's observation arc begins with its first used observation taken at Lowell Observatory in 1929, when it was identified as , nearly 43 years prior to its official discovery observation at Hamburg. In the Tholen classification, "Hynek" is characterized as a common S-type asteroid. In July 2007, the so-far best rated rotational lightcurve of "Hynek" was obtained from photometric observations by French amateur astronomer Pierre Antonini. Lightcurve analysis gave a well-defined rotation period of 3.9410 hours with a brightness variation of 0.17 magnitude (). According to the surveys carried out by NASA's Wide-field Infrared Survey Explorer with its


title: "1842 Hynek" content: subsequent NEOWISE mission, "Hynek" measures between 7.996 and 9.31 kilometers in diameter, and its surface has an albedo between 0.28 of 0.300. The "Collaborative Asteroid Lightcurve Link" assumes a standard albedo for stony asteroids of 0.20 and calculates a diameter of 9.80 kilometers with an absolute magnitude of 12.41. This minor planet was named after Hynek Kohoutek, the father of the discoverer, celebrating his 70th birthday. The official naming citation was published by the Minor Planet Center before November 1977 (). 1842 Hynek 1842 Hynek, provisional designation , is a stony Florian asteroid from the inner regions of the asteroid


title: "Hyundai i40" content: Hyundai i40 The Hyundai i40 is a large family car (D) designed for the European market by the South Korean manufacturer Hyundai. Sharing its platform with the United States marketed Hyundai Sonata, the i40 sedan was unveiled at the 2011 Barcelona Motor Show. In some markets, the Sonata remains on sale as a separate model, such as the United States, where the i40 is not available. The estate/wagon variant of the i40 was released in Europe and South Korea in September 2011, followed by the sedan variant in January 2012, and it is also available in Australia and New Zealand.


title: "Hyundai i40" content: For Malaysia, Hyundai launched the i40 at the 2013 Kuala Lumpur International Motor Show, in both sedan and tourer specifications. It is placed above the Hyundai Sonata. The engine is the two litre GDI motor which is linked to a paddle shifted six speed automatic gearbox. The car was designed at Hyundai's European R&D facilities in Russelsheim, Germany. It is manufactured at the Ulsan plant in South Korea. The i40 is described as featuring Hyundai's 'fluidic sculpture' design language, and was launched in Europe initially as an estate/wagon (marketed as the i40 Tourer) with a saloon was due in 2011.


title: "Hyundai i40" content: The boot space is 553 litres, increasing to 1,719 litres with the rear seats folded down. Depending on market, up to three engines are available from a total of four, a 1.7 L diesel in two states of tune (114 bhp and 134 bhp) and three petrol units 1.6 L (133 bhp) and 2.0 L (175 bhp) "GDI" (or a 2.0L (164 bhp) MPi petrol units. A 'BlueDrive' option includes Intelligent Stop & Go (ISG) start-stop system and 16 inch rolling resistance tyres, resulting in a reduced CO2 of 113g/km for the diesel. Euro NCAP test results for a LHD,


title: "Hyundai i40" content: five door hatchback variant on a registration from 2011: Hyundai Motor supplied the i40 estate for use in the 2011 FIFA Beach Soccer World Cup. The Hyundai i40 won the 2011 Eurocarbody Golden Award. Hyundai i40 The Hyundai i40 is a large family car (D) designed for the European market by the South Korean manufacturer Hyundai. Sharing its platform with the United States marketed Hyundai Sonata, the i40 sedan was unveiled at the 2011 Barcelona Motor Show. In some markets, the Sonata remains on sale as a separate model, such as the United States, where the i40 is not available.


title: "Craftsman Farms" content: Craftsman Farms Craftsman Farms was founded in 1908 in Parsippany-Troy Hills, Morris County, New Jersey, United States, by noted early 20th century designer Gustav Stickley as a farm and school for the Arts and Crafts movement. It remained in use until 1915 when it was sold to a family and became a private house. When threatened by development in 1989, the home was purchased by the Township of Parsippany-Troy Hills through eminent domain. The property is operated as a museum, also known as the Stickley Museum at Craftsman Farms, and is operated by the Craftsman Farms Foundation. Craftsman Farms is


title: "Konstantinos Iosifidis" content: Konstantinos Iosifidis Konstantinos Iosifidis (; born 14 January 1952) is a retired Greek footballer. Iosifidis spent his entire career from 1971 to 1985 in PAOK FC, playing as a left back. He is the only player in PAOK FC history that has won 4 titles, being part of the squad that won 2 cups in 1972 and 1974 and the 1976 and 1985 Greek league, being also captain in the latter. He also made 51 caps and scored 2 goals for the Greece national football team, and participated in UEFA Euro 1980. After retiring, he managed several teams in Greece,


title: "Konstantinos Iosifidis" content: such as Polykastro FC, Anagennisi Karditsas, PAONE, Anagennisi Kolindrou (Division C), Apollon Kalamarias, Naoussa, Ialysos Rodou, Kalamata FC (Division B) and Kavala FC (Division A). Since 2005, he is the general manager of PAOK. 1976, 1985 1972, 1974 Konstantinos Iosifidis Konstantinos Iosifidis (; born 14 January 1952) is a retired Greek footballer. Iosifidis spent his entire career from 1971 to 1985 in PAOK FC, playing as a left back. He is the only player in PAOK FC history that has won 4 titles, being part of the squad that won 2 cups in 1972 and 1974 and the 1976 and


title: "Virginia Avenue Tunnel" content: partnership as part of its National Gateway initiative. In 2011, CSX announced that it would fund the tunnel project itself.<ref name="CSX 5/18/11">CSX (2011-05-18). "CSX Commits Additional $160 Million to National Gateway." Press release.</ref> In 2012, CSX and government agencies considered four design alternatives for a new tunnel, conducting public outreach meetings, and preparing an environmental impact assessment for each of the alternatives. A final decision on the selected alternative was expected in spring 2013. CSX released its Draft Environmental Impact Statement (DEIS) in July 2013. During the comment period, many Capitol Hill and Navy Yard residents raised objections to the


title: "Electoral history of George H. W. Bush" content: Presidential tally): United States presidential election, 1980 1984 Republican National Convention (Vice Presidential tally): United States presidential election, 1984 1988 Republican presidential primaries: 1988 Republican National Convention (Presidential tally): United States presidential election, 1988 1992 Republican presidential primaries: 1992 Republican National Convention (Presidential tally): 1992 New York State Right to Life Party Convention: United States presidential election, 1992 Electoral history of George H. W. Bush George Herbert Walker Bush, 41st President of the United States (1989–1993), 43rd Vice President of the United States (1981–1989); Director of the CIA (1976–1977) and United States Representative from Texas (1967–1971). Texas United States Senate


title: "1873 Agenor" content: 1873 Agenor 1873 Agenor ( ), provisional designation "", is a dark Jupiter trojan from the Trojan camp, approximately in diameter. It was discovered during the Palomar–Leiden Trojan survey in 1971, and later named after Agenor from Greek mythology. The dark Jovian asteroid belongs to the 100 largest Jupiter trojans and has a rotation period of 20.60 hours. "Agenor" was discovered on 25 March 1971, by Dutch astronomer couple Ingrid and Cornelis van Houten at Leiden, on photographic plates taken by Dutch–American astronomer Tom Gehrels at Palomar Observatory in the Palomar Mountain Range, southeast of Los Angeles. The discovery was


title: "1873 Agenor" content: made in a survey of faint Trojans, one night after the discovery of 1870 Glaukos. The trio of Dutch and Dutch–American astronomers also collaborated on the productive Palomar–Leiden survey in the 1960s, using the same procedure as for this (smaller) survey: Tom Gehrels used Palomar's Samuel Oschin telescope (also known as the 48-inch Schmidt Telescope), and shipped the photographic plates to Cornelis and Ingrid van Houten at Leiden Observatory where astrometry was carried out. "Agenor" is a dark Jovian asteroid in a 1:1 orbital resonance with Jupiter. It is located in the trailering Trojan camp at the Gas Giant's Lagrangian


title: "1873 Agenor" content: point, 60° behind its orbit . It is also a non-family asteroid of the Jovian background population. It orbits the Sun at a distance of 4.7–5.7 AU once every 11 years and 12 months (4,370 days; semi-major axis of 5.23 AU). Its orbit has an eccentricity of 0.09 and an inclination of 22° with respect to the ecliptic. The body's observation arc begins with its official discovery observation at Palomar in March 1971. "Agenor" is an assumed, carbonaceous C-type asteroid. In February 1994, photometric observations with the ESO 1-metre telescope by astronomer Stefano Mottola and Anders Erikson at La Silla


title: "1873 Agenor" content: Observatory in Chile, were used to build a rotational lightcurve showing a rotation period of hours with a brightness variation of in magnitude (). According to the surveys carried out by the Japanese Akari satellite and the NEOWISE mission of NASA's Wide-field Infrared Survey Explorer, "Agenor" measures between 50.80 and 54.38 kilometers in diameter and its surface has an albedo between 0.038 and 0.062. The "Collaborative Asteroid Lightcurve Link" derives an albedo of 0.0506 and a diameter of 53.89 kilometers based on an absolute magnitude of 10.2. This minor planet was named for Agenor, who was able to inflict a


title: "1873 Agenor" content: wound on the Greek warrior Achilles. The Olympian deity Apollo assumed Agenor's form to distract Achilles while the Trojans forces were retreating. The minor planets 588 Achilles and 1862 Apollo are named after these two figures from Greek mythology. The body's name was suggested by Brian G. Marsden, the then director of the MPC. The official naming citation was published by the Minor Planet Center before November 1977 (). 1873 Agenor 1873 Agenor ( ), provisional designation "", is a dark Jupiter trojan from the Trojan camp, approximately in diameter. It was discovered during the Palomar–Leiden Trojan survey in 1971,


title: "2500 Alascattalo" content: 2500 Alascattalo 2500 Alascattalo, provisional designation , is a stony Flora asteroid from the inner regions of the asteroid belt, approximately 8 kilometers in diameter. The asteroid was discovered on 2 April 1926, by German astronomer Karl Reinmuth at Heidelberg Observatory in southern Germany. It was later named for the fictional moose–walrus Alascattalo creature. "Alascattalo" is a member of the Flora family, one of the largest groups of stony asteroids in the main-belt. It orbits the Sun in the inner main-belt at a distance of 2.0–2.5 AU once every 3 years and 4 months (1,225 days). Its orbit has an


title: "2500 Alascattalo" content: eccentricity of 0.10 and an inclination of 7° with respect to the ecliptic. No precoveries were obtained prior to its discovery. "Alascattalo" has been characterized as a common, stony S-type asteroid. A rotational lightcurve of this asteroid was obtained from photometric observations made by Junda Liu at the Lvye Observatory (), China, and at the iTelescope Observatory (), at the Siding Spring Observatory site, Australia, in December 2015. The lightcurve gave a well-defined rotation period of hours with a brightness variation of 0.19 in magnitude (). A previous lightcurve with a concurring period of hours and a similar amplitude of


title: "2500 Alascattalo" content: 0.15 was already obtained by French amateur astronomer Pierre Antonini in March 2013 (). According to the survey carried out by the NEOWISE mission of NASA's space-based Wide-field Infrared Survey Explorer, "Alascattalo" measures 7.5 and 7.9 kilometers in diameter and its surface has an albedo of 0.21 and 0.27, respectively, while the "Collaborative Asteroid Lightcurve Link" assumes an albedo of 0.24 – which derives from 8 Flora, the largest member and namesake of this orbital family – and calculates a diameter of 8.2 kilometers with an absolute magnitude of 12.6. This minor planet was named after the mythological creature "Alascattalo",


title: "2500 Alascattalo" content: a fictional chimera between a moose and a walrus. According to legend, it was genetically bred by miners during the Klondike Gold Rush in the late 19th century. The alascattalo also stands for the local people's unique sense of humor, dealing with tourists who ask naive questions, and is the mascot of the four-minute long, annual parade on "Alascattalo Day" held in November. The official naming citation was published by the Minor Planet Center on 21 November 1991 (). 2500 Alascattalo 2500 Alascattalo, provisional designation , is a stony Flora asteroid from the inner regions of the asteroid belt, approximately


title: "1846 Bengt" content: 1846 Bengt 1846 Bengt, provisional designation , is a dark asteroid from the inner regions of the asteroid belt, approximately 11 kilometers in diameter. Discovered by the Palomar–Leiden survey in 1960, it was named for Danish astronomer Bengt Strömgren. "Bengt" was discovered on 24 September 1960, by Dutch astronomer couple Ingrid and Cornelis van Houten in collaboration with Tom Gehrels, who took the photographic plates at Palomar Observatory in California. The survey designation "P-L" stands for "Palomar–Leiden", named after Palomar Observatory and Leiden Observatory, which collaborated on the fruitful Palomar–Leiden survey in the 1960s. Gehrels used Palomar's Samuel Oschin telescope


title: "1846 Bengt" content: (also known as the 48-inch Schmidt Telescope), and shipped the photographic plates to Ingrid and Cornelis van Houten at Leiden Observatory where astrometry was carried out. The trio are credited with . The asteroid was first identified as at McDonald Observatory in 1951. The observation arc starts 3 years prior to its official discovery observation, with its first used identification made at Goethe Link Observatory in 1957. "Bengt" orbits the Sun in the inner main-belt at a distance of 2.0–2.7 AU once every 3 years and 7 months (1,306 days). Its orbit has an eccentricity of 0.14 and an inclination


title: "1846 Bengt" content: of 3° with respect to the ecliptic. Based on preliminary results by NASA's Wide-field Infrared Survey Explorer with its subsequent NEOWISE mission, "Bengt" measures 10.998 kilometers in diameter and its surface has an albedo of 0.047, which is typical for carbonaceous C-type asteroids. As of 2017, no rotational lightcurve has been obtained. This minor planet was named after renowned Danish astronomer Bengt Strömgren (1908–1987), on the occasion of his 70th birthday. He was an authority in the field of stellar structure and stellar evolution, director of the Yerkes Observatory from 1951 to 1957, and president of the International Astronomical Union


title: "1846 Bengt" content: (1970–1973). The official naming citation was published by the Minor Planet Center before November 1977 (). 1846 Bengt 1846 Bengt, provisional designation , is a dark asteroid from the inner regions of the asteroid belt, approximately 11 kilometers in diameter. Discovered by the Palomar–Leiden survey in 1960, it was named for Danish astronomer Bengt Strömgren. "Bengt" was discovered on 24 September 1960, by Dutch astronomer couple Ingrid and Cornelis van Houten in collaboration with Tom Gehrels, who took the photographic plates at Palomar Observatory in California. The survey designation "P-L" stands for "Palomar–Leiden", named after Palomar Observatory and Leiden Observatory,


title: "Winter salami" content: Winter salami Winter salami () is a type of Hungarian salami produced according to a centuries-old tradition. Made from Mangalitsa pork and spices (white pepper, allspice, and others), winter salami is cured in cold air and smoked slowly. During the dry ripening process, a special noble-mold is formed on the casing surface. "Szegedi téliszalámi" (winter salami of Szeged) gained European Union PDO status in 2007, followed by "Budapesti téliszalámi", which gained PGI status in 2009. The Hungarian Ministry of Agriculture and Rural Development places many specific regulations on what can be called Szeged winter salami. Pick Szeged is one of


title: "Winter salami" content: the most successful producers of this style of salami. Winter salami Winter salami () is a type of Hungarian salami produced according to a centuries-old tradition. Made from Mangalitsa pork and spices (white pepper, allspice, and others), winter salami is cured in cold air and smoked slowly. During the dry ripening process, a special noble-mold is formed on the casing surface. "Szegedi téliszalámi" (winter salami of Szeged) gained European Union PDO status in 2007, followed by "Budapesti téliszalámi", which gained PGI status in 2009. The Hungarian Ministry of Agriculture and Rural Development places many specific regulations on what can be


title: "The Shape of Things to Come (Lost)" content: holds them at gunpoint, successfully demanding that Hurley goes with him (as he has found Jacob's cabin before). Flashforwards show Ben on three continents in autumn 2005. Ben is startled when he wakes up in the Sahara Desert wearing a winter jacket and with a large cut on his upper arm; challenged by two armed locals, he kills one of them (Nick Hermz) and knocks the other (Sammy Sheik) unconscious and travels on horseback to Tozeur, Tunisia on October 24, 2005. Ben journeys to Tikrit, Iraq, where the funeral of Sayid's wife Nadia Jazeem (Andrea Gabriel) is taking place. Ben


title: "1851 Lacroute" content: 1851 Lacroute 1851 Lacroute, provisional designation , is an asteroid from the outer region of the asteroid belt, approximately 17 kilometers in diameter. It was discovered on 9 November 1950, by French astronomer Louis Boyer at the Algiers Observatory in the capital of Algeria, Northern Africa, and named after French astronomer Pierre Lacroute. "Lacroute" orbits the Sun in the outer main-belt at a distance of 2.5–3.7 AU once every 5 years and 6 months (1,996 days). Its orbit has an eccentricity of 0.19 and an inclination of 2° with respect to the ecliptic. As no precoveries were taken, and no


title: "1851 Lacroute" content: prior identifications were made, the body's observation arc begins with its official discovery observation in 1950. According to the surveys carried out by the Infrared Astronomical Satellite (IRAS) and NASA's Wide-field Infrared Survey Explorer with its subsequent NEOWISE mission, "Lacroute" measures 16.9 and 18.2 kilometers in diameter, and its surface has an albedo of 0.049 and 0.074, respectively. As of 2016, the body's spectral type, as well as its rotation period and shape remain unknown. This minor planet was named in honor of French astronomer Pierre Lacroute (1906–1993), a known astrometrist, president of IAU's Commission 24 in the 1970s, and


title: "1851 Lacroute" content: director of the Observatory of Strasbourg, instrumental in the establishment of the Stellar Data Center "(also see SIMBAD)". Lacroute also made an independent reduction of the astrometric star catalogue AGK3, using a technique involving overlapping photographic plates. The official naming citation was published by the Minor Planet Center before November 1977 (). 1851 Lacroute 1851 Lacroute, provisional designation , is an asteroid from the outer region of the asteroid belt, approximately 17 kilometers in diameter. It was discovered on 9 November 1950, by French astronomer Louis Boyer at the Algiers Observatory in the capital of Algeria, Northern Africa, and named


title: "1938 Lausanna" content: 1938 Lausanna 1938 Lausanna, provisional designation , is a stony Florian asteroid from the inner regions of the asteroid belt, approximately 8 kilometers in diameter. It was discovered on 19 April 1974, by Swiss astronomer Paul Wild at Zimmerwald Observatory near Bern, Switzerland. It is named for the city of Lausanne. "Lausanna" is a S-type asteroid and member of the Flora family, one of the largest collisional populations of stony asteroids in the main-belt. It orbits the Sun in the inner main-belt at a distance of 1.9–2.6 AU once every 3 years and 4 months (1,222 days). Its orbit has


title: "1930 Lucifer" content: 1930 Lucifer 1930 Lucifer, provisional designation , is a carbonaceous asteroid from the outer regions of the asteroid belt, approximately 34 kilometers in diameter. It was discovered on 29 October 1964, by American astronomer Elizabeth Roemer at the Flagstaff station (NOFS) of the United States Naval Observatory (USNO). It is named after Lucifer, the "shining one" or "light-bearer" form the Hebrew Bible. "Lucifer" orbits the Sun in the outer main-belt at a distance of 2.5–3.3 AU once every 4 years and 11 months (1,802 days). Its orbit has an eccentricity of 0.14 and an inclination of 14° with respect to


title: "1930 Lucifer" content: the ecliptic. It was first identified as at Goethe Link Observatory in 1954, extending the body's observation arc by 10 years prior to its official discovery observation at NOFS. In the SMASS taxonomy, "Lucifer" is a Cgh-type that belongs to the carbonaceous C-group of asteroids. According to the surveys carried out by the Infrared Astronomical Satellite IRAS, the Japanese Akari satellite, and NASA's Wide-field Infrared Survey Explorer with its subsequent NEOWISE mission, "Lucifer" measures between 27.00 and 39.61 kilometers in diameter, and its surface has an albedo between 0.05 and 0.1058. The "Collaborative Asteroid Lightcurve Link" derives an albedo of


title: "1930 Lucifer" content: 0.0886 and calculates a diameter of 26.90 kilometers based on an absolute magnitude of 11.1. In October 2003, a rotational lightcurve of "Lucifer" was obtained from photometric observations by American astronomer Brian Warner at his Palmer Divide Observatory in Colorado. Lightcurve analysis gave a well-defined rotation period of 13.056 hours with a brightness amplitude of 0.44 magnitude (). In January 2005, observations by astronomer Horacio Correia gave a concurring period of 13.054 hours and an amplitude of 0.22 magnitude (). In 2013, another lightcurve was obtained at the Palomar Transient Factory (), and a modeled lightcurve from various data sources,


title: "1930 Lucifer" content: including the AstDyS database, gave another concurring period of 13.0536 hours and found a pole of (32.0°,17.0°). Lutz D. Schmadel's "Dictionary of Minor Planet Names" reads "Named for the proud, rebellious archangel, identified with Satan, who was expelled from heaven". The official naming citation was published by the Minor Planet Center before November 1977 (). 1930 Lucifer 1930 Lucifer, provisional designation , is a carbonaceous asteroid from the outer regions of the asteroid belt, approximately 34 kilometers in diameter. It was discovered on 29 October 1964, by American astronomer Elizabeth Roemer at the Flagstaff station (NOFS) of the United States


title: "1936 Lugano" content: 1936 Lugano 1936 Lugano, provisional designation , is a carbonaceous Adeonian asteroid from the middle region of the asteroid belt, approximately 26 kilometers in diameter. It was discovered on 24 November 1973, by Swiss astronomer Paul Wild at Zimmerwald Observatory near Bern, Switzerland. It was later named for the Swiss city of Lugano. "Lugano" is a member of the Adeona family (), a large family of carbonaceous asteroids. It orbits the Sun in the central main-belt at a distance of 2.3–3.0 AU once every 4 years and 5 months (1,599 days). Its orbit has an eccentricity of 0.14 and an


title: "1936 Lugano" content: inclination of 10° with respect to the ecliptic. It was first identified as at Johannesburg Observatory in 1936. The body's observation arc begins 22 years prior to its official discovery observation at Zimmerwald, when it was identified as at McDonald Observatory in 1951. In the SMASS classification, "Lugano" is a Ch-subtype, a hydrated C-type asteroid, while the Wide-field Infrared Survey Explorer (WISE) rates it as a very dark and featureless reddish P-type asteroid. According to the space-based surveys carried out by the Infrared Astronomical Satellite IRAS, the Japanese Akari satellite and the NEOWISE mission of NASA's WISE telescope, "Lugano" measures


title: "1904 Massevitch" content: 1904 Massevitch 1904 Massevitch, provisionally designated , is a rare-type asteroid from the middle region of the asteroid belt, approximately 16 kilometers in diameter. It was discovered on 9 May 1972, by the Russian astronomer Tamara Smirnova at the Crimean Astrophysical Observatory in Nauchnyj, on the Crimean peninsula. It was later named after Russian astrophysicist Alla Massevitch. "Massevitch" orbits the Sun in the central main-belt at a distance of 2.5–2.9 AU once every 4 years and 7 months (1,662 days). Its orbit has an eccentricity of 0.07 and an inclination of 13° with respect to the ecliptic. It was first


title: "1904 Massevitch" content: identified as at Goethe Link Observatory in 1949, extending the body's observation arc by 23 years prior to its discovery observation. The moderately bright R-type asteroid has a surface that strongly absorbs in the olivine and pyroxene spectral region, which give it its very reddish color. According to the surveys carried out by NASA's Wide-field Infrared Survey Explorer with its subsequent NEOWISE mission and the Infrared Astronomical Satellite IRAS, "Massevitch" measures 13.50 and 18.19 kilometers in diameter, and its surface has an albedo of 0.161 and 0.581, respectively, while the "Collaborative Asteroid Lightcurve Link" derives an albedo of 0.176 and


title: "1904 Massevitch" content: a diameter of 18.25 kilometers with an absolute magnitude of 11.2. In September 2014, a rotational lightcurve of "Massevitch" was obtained from photometric observations taken at the Oakley Southern Sky Observatory () in Coonabarabran, Australia. It gave a rotation period of hours with a brightness varitaion of 0.30 magnitude () This minor planet was named after Russian astrophysicist and astronomer Alla Genrichovna Massevitch (born 1918), vice-president of the Astronomical Council of the former USSR Academy of Sciences (now Russian Academy of Sciences). In the former USSR, Massevitch organized the optical tracking of artificial satellites in Earth's orbit. The approved naming


title: "1904 Massevitch" content: citation was published by the Minor Planet Center before November 1977 (). 1904 Massevitch 1904 Massevitch, provisionally designated , is a rare-type asteroid from the middle region of the asteroid belt, approximately 16 kilometers in diameter. It was discovered on 9 May 1972, by the Russian astronomer Tamara Smirnova at the Crimean Astrophysical Observatory in Nauchnyj, on the Crimean peninsula. It was later named after Russian astrophysicist Alla Massevitch. "Massevitch" orbits the Sun in the central main-belt at a distance of 2.5–2.9 AU once every 4 years and 7 months (1,662 days). Its orbit has an eccentricity of 0.07 and


title: "Blossom Kite Festival" content: Blossom Kite Festival The Blossom Kite Festival, formerly the Smithsonian Kite Festival, is an annual kite event usually held on the National Mall in Washington, D.C. in late March during the National Cherry Blossom Festival. The 2018 kite festival took place on the Washington Monument grounds on Saturday, March 31. The festival was founded in 1967 by aviation pioneer Paul E. Garber, the first curator of the National Air and Space Museum (NASM). Until 2010, the Smithsonian Associates, the cultural, educational, and membership division of the Smithsonian Institution organized and sponsored the festival. The National Cherry Blossom Festival, Inc. began


title: "Blossom Kite Festival" content: producing the festival in 2011 and renamed the event to the "Blossom Kite Festival". Sponsored by the Smithsonian National Associate Program (see S. Dillon Ripley Center) and the NASM, the first annual Smithsonian Kite Carnival (later referred to as the Kite Festival) took place on the National Mall on March 25, 1967. Individuals could compete in contests with homemade kites as well as ready-made ones. The festival also included kite-making workshops led by Paul Garber, a lecture series, and a special display of kites made by Garber and his wife. However, an 1892 law that was still in effect barred


title: "Blossom Kite Festival" content: the flying of kites, balloons and parachutes within the city limits of Washington, D.C. In 1970, the Smithsonian Institution was therefore denied a permit to hold its annual kite flying carnival on the National Mall. On April 18, 1970, police arrested 11 people who were protesting the law by flying kites near the Washington Monument. As kite enthusiasts were not allowed to have the kite carnival that year in D.C., they moved the event to Fort Washington in Prince George's County, Maryland. The law was subsequently changed, permitting the kite carnival/festival to again be held on the National Mall. The


title: "Blossom Kite Festival" content: 2008 Smithsonian Kite Festival was held on Saturday, March 29 on the National Mall. The festival, which was tied to the 2008 Summer Olympics to be held in Beijing, China, from August 8 to August 24, 2008, highlighted the art and history of Chinese kites. The Smithsonian stated that the Chinese introduced the first kites more than 2,000 years ago. According to the Smithsonian, the Chinese first used kites in military affairs for estimating distances and carrying propaganda leaflets, but the kites' influence gradually spread to Western countries to become what the Smithsonian called a “familiar artistic and cultural icon.”


title: "Blossom Kite Festival" content: The Smithsonian stated that kites continue to play an important role in China. The 2009 Smithsonian Kite Festival was held on Saturday, March 28, on the Washington Monument grounds. The theme of the festival was "Going Green". Participants were encouraged to create environmentally and thematically “green” kites from renewable resources such as bamboo and recyclable goods such as paper and cloth. Organizers expected to distribute 1,000 free kites to children on a first come, first served basis. The 2010 Smithsonian Kite Festival, which the Smithsonian Associates and the NASM presented, took place on Saturday, March 27. The theme was "CRAFTed


title: "Blossom Kite Festival" content: for Flight". Events included the competitive Rokkaku Battle, Hot Tricks Showdown and Ground Display. The festival also featured a kitemaking competition that was open to any hand-made kite. Adult competitors and a team of judges ranging from kitemaking experts to local celebrities to museum staff chose the winners of awards in each category. Kitemakers were grouped according to experience and age: kitemaker, master kitemaker, age 11 and under, age 12–15. The event also encouraged non-competitors to make and fly kites on the Washington Monument grounds. The first Blossom Kite Festival took place on the Washington Monument grounds on Sunday, April


title: "Blossom Kite Festival" content: 10, 2011, following a postponent from March 27 because of forecasted inclement weather. The 2012 Blossom Kite festival took place on the Washington Monument grounds on Saturday, March 31. The 2013 Blossom Kite Festival took place on the Washington Monument grounds on Saturday, March 30. The 2014 Blossom Kite Festival was originally scheduled to take place on the Washington Monument grounds on Saturday, March 29. However, the event's organizers first postponed the event to Sunday, March 30, because of rain and then cancelled the Sunday event because inclement weather had saturated the Monument grounds. The 2015 Blossom Kite Festival took


title: "Blossom Kite Festival" content: place on the Washington Monument grounds on Saturday, March 28. The 2016 kite festival took place on the Washington Monument grounds on Saturday, April 2. The organizer's announcement for the festival stated: "Please note: drones are prohibited at this event." The 2017 kite festival took place on the Washington Monument grounds on Saturday, April 1. Blossom Kite Festival The Blossom Kite Festival, formerly the Smithsonian Kite Festival, is an annual kite event usually held on the National Mall in Washington, D.C. in late March during the National Cherry Blossom Festival. The 2018 kite festival took place on the Washington Monument


title: "Talento de Barrio (soundtrack)" content: troubled surroundings. The soundtrack became a major debuting success on the "Billboard" 200, peaking at number 13 with 26,000 sold in its first week. It dropped to number 23 the week after, and eventually to number 35. Its final charting position was at number 191, as of December 13, 2008. It also became entered in the Top 5 of the "Billboard" Top Soundtracks chart peaking at number 3, becoming Daddy Yankee's first Top 5 soundtrack on the Top Soundtracks chart. The soundtrack is also Yankee's fourth consecutive number-one album on the "Billboard" Top Latin Albums chart. Credits adapted from the


title: "Hickory Hill Park" content: Hickory Hill Park Hickory Hill Park is a large natural area in northeast Iowa City, Iowa consisting of of forest, abandoned fields, reconstructed prairie, wetlands, and parkland centered on Ralston Creek and its tributary drainages. It is owned and administered by the city, with help from Friends of Hickory Hill Park. The park is popular with day hikers, dog walkers, cross-country skiers, sledders, and picnickers. Iowa City’s Hickory Hill Park should not be confused with Hickory Hills Park near Waterloo, or Hickory Hills Park in Tama County. Hickory Hill Park traces its origins to 1927 with a parcel of wood


title: "Franklin Township, Franklin County, Kansas" content: members of the Franklin Township Board of Trustees and one member appointed by the City of Wellsville. Interstate 35 runs from the northeast to the southeast through Franklin Township. Kansas State Highway 33 runs north/south through Franklin Township. Franklin Township contains one airport or landing strip, Qualls-Hart Airport. A main line of the BNSF Railway runs through the middle of Franklin Township. Franklin Township, Franklin County, Kansas Franklin Township is a township in Franklin County, Kansas, USA. As of the 2000 census, its population was 2,552. It is the most populated township in Franklin County. Franklin Township covers an area


title: "Katarina Dalayman" content: Provence (2008) and at the Metropolitan Opera (2009) and at the Osterfestspiele Salzburg (2009–10); Judith (Bluebeard's Castle) in the Gran Teatre del Liceu, Barcelona (2008); Isolde at the New York Met (2008); Brünnhilde; Kundry at the New York Met (2013). After training to a mezzosoprano, she returned and sang Fricka and Waltraute in the 2017 brief revival of Valdemar-Holm's Wagner Ring Cycle in Stockholm. In the beginning of 2018 she created a well reviewed Klytaemnestra in the revival of Valdemar Holm's Elektra (the same production she sang the main role Elektra in 2009), also in Stockholm. Dalayman's recordings include: Berg


title: "Hyman Goldin" content: 360 acres of land in the Adirondack Mountains and established children's summer camps and the Blue Sky Lodge Hotel, which become a meeting ground for modern Orthodox thinkers. Jewish chaplain to Comstock Prison from 1932 to 1947, Goldin collaborated with two prisoners to write a "Dictionary of American Underworld Lingo" (1950). His "The Case of the Nazarene Reopened" (1948), written in the form of a court transcript, acquitted the Jews of the charge of killing Jesus Christ. Goldin translated the "Kitzur Shulchan Aruch," an abridged version of the Shulchan Aruch (The standard code of Jewish law), publishing his translation in


title: Nutraloaf content: from vegetables, fruit, meat, and bread or other grains. The ingredients are blended and baked into a solid loaf. In one version, it is made from a mixture of ingredients that include ground beef, vegetables, beans, and bread crumbs. Other versions include mechanically separated poultry and "dairy blend". Although nutraloaf can be found in many United States prisons, its use is controversial. It was mentioned by the U.S. Supreme Court in 1978 in "Hutto v. Finney" while ruling that conditions in the Arkansas penal system constituted cruel and unusual punishment. Prisoners were fed "", described as "a substance created by


title: "Tony LeMans" content: also produced a song with David Gamson for Donny Osmond's comeback album. (Sure Looking Good). Tony's true name was "Tony MansFortier" Tony chose the name "Lemans", because his father loved the vehicle. Therefore, Tony merged his father's love of the car and the name together. Shayne Soentpiet, Tony LeMans band member Tony LeMans Tony LeMans was a singer and songwriter associated with Prince and signed to Prince's Paisley Park Records. Tony LeMans grew up in Hollywood and ran around with the Gordy kids and other musical stars. Lenny Kravitz and Tony started a band called Romeo Blue but had a


title: "Thermal conductivity measurement" content: using selected sensors, respectively. Two basic forms are now available: the linear source freestanding sensor and the planar source freestanding sensor. The range of thermophysical properties can be covered by different forms of the technique, with the exception that the recommended thermal conductivity range where the highest precision can be attained is 0.01 to 150 W/m•K for the linear source freestanding sensor and 500 to 8000 J/m2•K•s0.5 for the planar source freestanding sensor. Time-domain thermoreflectance is a method by which the thermal properties of a material can be measured, most importantly thermal conductivity. This method can be applied most notably


title: "Colm Coyle" content: Colm Coyle Colm Coyle (born 26 February 1963), is a former Gaelic footballer and former manager from County Meath, Ireland. He was the manager of the Meath senior football team from September 2006 to July 2008. Coyle won a Leinster Minor Football Championship medal with Meath in 1980. He made his senior debut for Meath in the 1981/82 National League. He enjoyed much success play inter-county football in the eighty's & ninety's on the Meath teams managed by Sean Boylan. He was part of the Meath team which won the Leinster Championship in 1986, Meath's first since 1970. Coyle then


title: "Colm Coyle" content: board. Colm Coyle Colm Coyle (born 26 February 1963), is a former Gaelic footballer and former manager from County Meath, Ireland. He was the manager of the Meath senior football team from September 2006 to July 2008. Coyle won a Leinster Minor Football Championship medal with Meath in 1980. He made his senior debut for Meath in the 1981/82 National League. He enjoyed much success play inter-county football in the eighty's & ninety's on the Meath teams managed by Sean Boylan. He was part of the Meath team which won the Leinster Championship in 1986, Meath's first since 1970. Coyle


title: "Walter Meeuws" content: player, he won 4 championships, 2 with Standard in Belgium, 1 with Bruges in Belgium and 1 with Ajax in the Netherlands. He also won 2 cups and played the final of the European Championship with Belgium in Italy in 1980. As a manager, he won 3 cups with Lierse, Antwerp and Far Rabat ( 2009 ), 1 Supercup with Lierse and was runner up in the African Champions League Final with Raja Casablanca and also runner up with Antwerp in the final of the European Cup II in 1993 at Wembley. He is the last manager ever that reached


title: "Toque Toque Grande and Toque Toque Pequeno" content: Toque Toque Grande and Toque Toque Pequeno Toque-Toque Grande and Toque-Toque Pequeno are two beaches at the Atlantic Ocean in the city of São Sebastião, SP, Brasil. They are separated by another beach called "das Calhetas", being 2,4km away from each other. Despite its name ("Grande" means "big" in Portuguese), the beach is only some 800m long, and is smaller than Toque-toque Pequeno Beach. Several mid-class houses surround the beach, while a couple of kiosks offer food and beverage for visitors. Most of them work only during summer, when the beach is visited by more people. At one and a


title: "Toque Toque Grande and Toque Toque Pequeno" content: half a kilometer far from the left (Southeast) edge of the beach, there's the Toque-Toque Grande Island (larger than the Toque-Toque Pequeno Island), unhabitated and with no beaches, but frequently visited for scuba diving. The top of the hill at the left of the beach can be achieved by walking. Toque-Toque Pequeno is the second beach after Toque Toque Grande, heading Northwest. It is longer than Toque-Toque Grande, and its landscape is much the same: mid-class houses between the beach and the highway, weak or moderate waves and restaurants. Just as Toque Toque Grande, it also has its own island,


title: "Toque Toque Grande and Toque Toque Pequeno" content: which is much smaller than the other's. The island resembles a turtle when seen from the continent. Toque Toque Grande and Toque Toque Pequeno Toque-Toque Grande and Toque-Toque Pequeno are two beaches at the Atlantic Ocean in the city of São Sebastião, SP, Brasil. They are separated by another beach called "das Calhetas", being 2,4km away from each other. Despite its name ("Grande" means "big" in Portuguese), the beach is only some 800m long, and is smaller than Toque-toque Pequeno Beach. Several mid-class houses surround the beach, while a couple of kiosks offer food and beverage for visitors. Most of


title: "April 2005 lunar eclipse" content: Total Lunar Eclipse: 2167 Aug 01 First Central Lunar Eclipse: 2221 Sep 02 Greatest Eclipse of the Lunar Saros 141: 2293 Oct 16 Last Central Lunar Eclipse: 2546 Mar 18 Last Total Lunar Eclipse: 2618 May 01 Last Partial Lunar Eclipse: 2744 Jul 16 Last Penumbral Lunar Eclipse: 2888 Oct 11 1901-2100 March 1915 lunar eclipse March 1933 lunar eclipse March 1951 lunar eclipse April 1969 lunar eclipse April 1987 lunar eclipse April 2005 lunar eclipse May 2023 lunar eclipse May 2041 lunar eclipse May 2059 lunar eclipse June 2077 lunar eclipse June 2095 lunar eclipse This eclipse is the


title: "1921 Pala" content: 1921 Pala 1921 Pala, provisional designation is an unstable asteroid from the background population of the outer asteroid belt, approximately 8.2 kilometers in diameter. It is one of very few bodies located in the 2 : 1 mean motion resonance with Jupiter. It was discovered by Dutch–American astronomer Tom Gehrels at Palomar Observatory on 20 September 1973. "Pala" is a non-family background asteroid from the main belt's background population. It orbits the Sun in the outer asteroid belt at a distance of 2.0–4.6 AU once every 5 years and 12 months (2,187 days; semi-major axis of 3.30 AU). Its orbit


title: "1921 Pala" content: has an eccentricity of 0.39 and an inclination of 19° with respect to the ecliptic. The body's observation arc begins at Palomar with its official discovery observation. It has a strongly unstable orbit near the 2:1 orbital resonance with Jupiter. The asteroid's orbit is expected to persist for another 18 million years though. "Pala" measures approximately 8.2 kilometers in diameter, while the albedo of its surface has not been estimated. As of 2017, the body's spectral type as well as its rotation period and shape remain unknown. This minor planet is named after the Indian reservation, Pala, located at the


title: "1921 Pala" content: base of Palomar Mountain, believed to apply to an Indian tribe whose members have lived in the area for many centuries. The official naming citation was published by the Minor Planet Center before November 1977 (). 1921 Pala 1921 Pala, provisional designation is an unstable asteroid from the background population of the outer asteroid belt, approximately 8.2 kilometers in diameter. It is one of very few bodies located in the 2 : 1 mean motion resonance with Jupiter. It was discovered by Dutch–American astronomer Tom Gehrels at Palomar Observatory on 20 September 1973. "Pala" is a non-family background asteroid from


title: "1830 Pogson" content: 1830 Pogson 1830 Pogson, provisional designation , is a stony Florian asteroid and an asynchronous binary system from the inner regions of the asteroid belt, approximately in diameter. It was discovered on 17 April 1968, by Swiss astronomer Paul Wild at the Zimmerwald Observatory near Bern, Switzerland. The S-type asteroid has a rotation period 2.6 of hours. It was named for English astronomer Norman Pogson. The discovery of its 2.5-kilometer sized companion was announced in May 2007. According to a HCM-analysis by David Nesvorný, "Pogson" is a member of the Flora family (), a giant asteroid clan and the largest


title: "1830 Pogson" content: family of stony asteroids in the asteroid belt. It has also been grouped into the Augusta family () by Zappalà, while for Milani and Knežević, who don't recognize the Florian clan as a family, "Pogson" is a non-family asteroid from the main belt's background population. It orbits the Sun in the inner asteroid belt at a distance of 2.1–2.3 AU once every 3 years and 3 months (1,182 days; semi-major axis of 2.19 AU). Its orbit has an eccentricity of 0.06 and an inclination of 4° with respect to the ecliptic. The asteroid was first observed as at Simeiz Observatory


title: "1830 Pogson" content: in April 1926. The body's observation arc begins with its observation as at Heidelberg Observatory in March 1929, or 39 years prior to its official discovery observation at Zimmerwald. This minor planet was named after English astronomer Norman Pogson (1829–1891), inventor of the modern astronomical magnitude scale. At the Radcliffe and Madras observatories, he discovered eight asteroids, including 42 Isis and 67 Asia. The lunar crater "Pogson" was also named in his honor. The official was published by the Minor Planet Center before November 1977 (). In the Tholen and SMASS classification, "Pogson" is a common, stony S-type asteroid. In


title: "1830 Pogson" content: April 2007, a rotational lightcurve of "Pogson" was obtained from photometric observations by an international collaboration of Australian, European and American astronomers, namely, David Higgins, Petr Pravec, Peter Kušnirák, Julian Oey and Donald Pray. Lightcurve analysis gave a rotation period of hours with a brightness variation of 0.12 magnitude (). In the following month, a more refined period of hours with the same amplitude was measured by Petr Pravec (). Additional period determinations were made by Melissa Dykhuis and collaborators (2.5698 h) at the Calvin College Observatory during 2008 (), and by Pierre Antonini (2.5699 h) and Julian Oey (2.604


title: "1830 Pogson" content: h) in March 2013 (). During the photometric observation in 2007, it was also revealed, that "Pogson" is an asynchronous binary system with a minor-planet moon in its orbit. The mutual eclipse and occultation events showed that the companion, provisionally designated , orbits its primary every 24.24 hours. Based on a secondary-to-primary diameter ratio of 0.32 or larger, Johnston's archive estimates a diameter of 2.52 kilometers for the satellite, separated by 8 kilometers from its primary. According to the survey carried out by the NEOWISE mission of NASA's Wide-field Infrared Survey Explorer, "Pogson" measures between 7.7 and 8.35 kilometers in


title: "1830 Pogson" content: diameter and its surface has an albedo between 0.2188 and 0.274. The "Collaborative Asteroid Lightcurve Link" adopts the result from Petr Pravec's revised WISE-data, that is, an albedo of 0.2188 and a diameter of 8.35 kilometers based on an absolute magnitude of 12.659. 1830 Pogson 1830 Pogson, provisional designation , is a stony Florian asteroid and an asynchronous binary system from the inner regions of the asteroid belt, approximately in diameter. It was discovered on 17 April 1968, by Swiss astronomer Paul Wild at the Zimmerwald Observatory near Bern, Switzerland. The S-type asteroid has a rotation period 2.6 of hours.


title: "1484 Postrema" content: 1484 Postrema 1484 Postrema, provisional designation , is a carbonaceous Postremian asteroid and namesake of the Postrema family from the central regions of the asteroid belt, approximately 41 kilometers in diameter. It was discovered on 29 April 1938, by Soviet astronomer Grigory Neujmin at the Simeiz Observatory on the Crimean peninsula. The name "Postrema" celebrates the astronomer's last minor planet discovery. "Postrema" is the parent body and namesake of the Postrema family (), a mid-sized central asteroid family of little more than 100 members. It orbits the Sun in the central main-belt at a distance of 2.2–3.3 AU once every


title: "1484 Postrema" content: 4 years and 6 months (1,656 days). Its orbit has an eccentricity of 0.20 and an inclination of 17° with respect to the ecliptic. The asteroid was first identified as at Johannesburg Observatory in May 1911. The body's observation arc begins with its identification as at Lowell Observatory in February 1933, more than 5 years prior to its official discovery observation at Simeiz. In the SMASS classification, "Postrema" is a bright carbonaceous B-type asteroid, while the overall spectral type of the Postrema family has been described as that of C- and X-type. In May 2006, two rotational lightcurves of "Postrema"


title: "1484 Postrema" content: were independently obtained from photometric observations. Lightcurve analysis gave a rotation period of 12.19 and 12.1923 hours with a brightness amplitude of 0.23 and 0.22 magnitude, respectively (). The asteroids lightcurve has also been modeled, using photometric data from the Lowell Photometric Database and other sources. Modelling gave a concurring period of 12.18978 hours, as well as two spin axis of (19.0°, 44°) and (250.0°, 64°) in ecliptic coordinates (λ, β). According to the surveys carried out by the Infrared Astronomical Satellite IRAS, the Japanese Akari satellite and the NEOWISE mission of NASA's Wide-field Infrared Survey Explorer, "Postrema" measures between


title: "1484 Postrema" content: 34.696 and 47.00 kilometers in diameter and its surface has a notably low albedo between 0.0137 and 0.05. The "Collaborative Asteroid Lightcurve Link" derives an albedo of 0.0409 and a diameter of 43.42 kilometers based on an absolute magnitude of 10.9. This minor planet was named "Postrema", which means "the last of a group". It celebrates Grigory Neujmin's last numbered minor planet discovery. The official naming citation was published by the Minor Planet Center on June 1955 (). The citation only holds true at the time of publication. In retrospect, "Postrema" is not Neujmin's last discovery, neither by number nor


title: "1484 Postrema" content: by its discovery date. These would be the asteroids 4420 Alandreev (highest numbered) and 2536 Kozyrev, officially discovered on 15 August 1939, more than a year after "Postrema". 1484 Postrema 1484 Postrema, provisional designation , is a carbonaceous Postremian asteroid and namesake of the Postrema family from the central regions of the asteroid belt, approximately 41 kilometers in diameter. It was discovered on 29 April 1938, by Soviet astronomer Grigory Neujmin at the Simeiz Observatory on the Crimean peninsula. The name "Postrema" celebrates the astronomer's last minor planet discovery. "Postrema" is the parent body and namesake of the Postrema family


title: "Subi Reef" content: but were allowed to continue their mission undeterred. In April 2016 a new lighthouse 55 metres high commenced operations. A civilian test flight to the new airport was conducted by a passenger jet of Hainan Airlines on July 13, 2016. Subi Reef Subi Reef, also known as Zhubi Reef (; ; ) is a reef in the Spratly Islands of the South China Sea located southwest of Philippine-occupied Thitu Island. It is occupied by China, and claimed by Taiwan, Vietnam, and the Philippines. It currently falls under the "de facto" jurisdiction of Nansha islands, Sansha city, Hainan province, China. The


title: "Future of the Royal Air Force" content: is increased substantially as well. The cargo box is 17.71 m long excluding ramp, 4.00 m wide, and 3.85 m high. The height is 4.00 m aft of the wing and the ramp is 5.40 m long. The Airbus A400M will operate in many configurations including cargo transport, troop transport, Medical evacuation, and electronic surveillance. The aircraft is intended for use on short, soft landing strips and for long-range, cargo transport flights. Current & Future Units Strategic Defence and Security Review 2015 included a reprieve for some of the Hercules fleet, with the Government announcing "We will upgrade and extend


title: "Acanthopagrus australis" content: be variable: fish caught in freshwater may be bronze- or brown-coloured, while those caught in estuarine or marine habitats are more silvery. A specimen measuring long and weighing 7 pounds 3 ounces was caught in the Georges River and reported in 1928, while another even longer specimen from the Clarence River was and 7 pounds 2 ounces. Yellowfin bream are found along the east coast of Australia from around 19 S to 38 S—roughly from Townsville in northern Queensland to Mallacoota and the Gippsland Lakes region in eastern Victoria. Bream inhabit estuaries in salt- or brackish water up to the


title: "Cricket Namibia" content: Women's Cricket Teams Zebra WHS Pro-Ed Blue Waters Sparta Defence Force Ground Trans Namib Ground United Ground, Windhoek Wanderers Cricket Ground Windhoek High School WAP Cricket Ground Sparta Cricket Ground Doc Jubber Cricket Field Walvis Bay Cricket Oval Swakopmund Vineta Cricket Field Cricket Namibia The Namibia Cricket Board, known commercially as Cricket Namibia, is the official governing body of the sport of cricket in Namibia. Its current headquarters is in Windhoek, Namibia. Cricket Namibia is Namibia's representative at the International Cricket Council and has been an associate member of that body since 1992. It is also a member of the


title: "Cook Islands Cricket Association" content: Cricket. The Cook Islands is one of three International Cricket Council member countries that do not issue their own passports, instead Cook Islanders have New Zealand passports, this presents significant challenges for Cook Islands Cricket in eligibility of its overseas based and even returning Cook Islands resident players. Cook Islands Cricket Association Cook Islands Cricket Association is the official governing body of the sport of cricket in Cook Islands. Its current headquarters is in Rarotonga, Cook Islands. Cook Islands Cricket Association is Cook Islands's representative at the International Cricket Council and is an affiliate member and has been a member


title: "Sweat Band" content: Sweat Band Sweat Band is the 1980 debut album by the P-Funk spin off act the Sweat Band. The album was the first official release on the Uncle Jam Records label, formed by George Clinton and his business manager Archie Ivy, and distributed by CBS Records. The band was formed by P-Funk bassist Bootsy Collins after losing the rights to the name Rubber Band to a folk music group of the same name. The album features many of the same musicians and singers from Bootsy's Rubber Band. The album was released during the same week as "Ultra Wave", Collins' fifth


title: "Sweat Band" content: album for Warner Bros. Records. The album was produced by Bootsy Collins, while George Clinton serves as executive producer. The album was reissued on CD by CBS/Sony Records in Japan on May 21, 1994, but quickly went out of print soon after. Art Direction/Photography: Diem Jones Sweat Band Sweat Band is the 1980 debut album by the P-Funk spin off act the Sweat Band. The album was the first official release on the Uncle Jam Records label, formed by George Clinton and his business manager Archie Ivy, and distributed by CBS Records. The band was formed by P-Funk bassist Bootsy


title: "Blue Valley Songbird" content: mother before entering the studio to cut her first record. The film ends with Leana singing "Blue Valley Songbird" in concert with Hank watching from the back of the room before leaving. There was no official soundtrack released, but some songs are available on other Dolly releases as noted below. "Blue Valley Songbird" - Written and Performed by Dolly Parton "I Hope You're Never Happy" - Written by Dolly Parton Performed by Dolly Parton featuring Billy Dean "Wildflowers" - Written and Performed by Dolly Parton "We Might Be In Love" - Written by Dolly Parton Performed by Dolly Parton and


title: "Grandmother Jia" content: Grandmother Jia Grandmother Jia (), née Shi, so often also called Dowager Shi () or simply the Dowager, is a major character in the Chinese novel "Dream of the Red Chamber". She is the daughter of Marquis Shi of Jinling. She is also Baoyu and Daiyu's grandmother and the oldest and most respected authority of the Jia Clan. A doting figure, it was she who arranged for Daiyu, her only "outside" (i.e., maternal) grandchild, to come to the Rongguo Mansion. It was with her help that Baoyu and Daiyu became extremely close as childhood playmates, and eventually, kindred spirits and


title: "Grandmother Jia" content: lovers. Grandmother Jia is at heart a fun-loving elder who greatly enjoys conversation and the company of her many grandchildren. A Chinese opera fan, despite her great wealth and prestige she is mindful of the rustic poor like Granny Liu, and is pious and generous in almsgiving. The Dowager's descendants and close relatives include: Grandmother Jia Grandmother Jia (), née Shi, so often also called Dowager Shi () or simply the Dowager, is a major character in the Chinese novel "Dream of the Red Chamber". She is the daughter of Marquis Shi of Jinling. She is also Baoyu and Daiyu's


title: Termopsidae content: Termopsidae Dampwood termites constitute a small and rather primitive family Termopsidae ("Latin") of termites (Isoptera). They contain four or five extant genera with 13–20 living species, but can be divided into several subfamilies. They may be a nuisance, but compared to the drywood termites (Kalotermitidae), usually do not cause extensive damage to buildings or other man-made structures. As their name implies, they eat wood that is not dried out, perhaps even rotting, and consequently of little use to humans. The termites as a group were traditionally placed in the Exopterygota, but such an indiscriminate treatment makes that group a paraphyletic


title: "1879 Broederstroom" content: 1879 Broederstroom 1879 Broederstroom, provisional designation , is a stony Florian asteroid from the inner regions of the asteroid belt, approximately 7 kilometers in diameter. It was discovered on 16 October 1935, by Dutch astronomer Hendrik van Gent at the Leiden Southern Station (), annex to the Johannesburg Observatory in South Africa. The asteroid was named after the South African village of Broederstroom. "Broederstroom" is a member of the Flora family. It orbits the Sun in the inner main-belt at a distance of 1.9–2.6 AU once every 3 years and 4 months (1,229 days). Its orbit has an eccentricity of


title: "1879 Broederstroom" content: 0.15 and an inclination of 2° with respect to the ecliptic. No precoveries were taken, and no prior identifications were made. The body's observation arc begins with its official discovery observation at Johannesburg in 1935. "Broederstroom" has been characterized as a common stony S-type asteroid. In January 2007, a rotational lightcurve obtained by Italian amateur astronomer Antonio Vagnozzi gave a well-defined rotation period of 3.01555 hours with a brightness variation of 0.11 magnitude (). In Spring 2014, photometry at the Palomar Transient Factory in California gave two lightcurves with a period of 3.016 and 3.02 hours and an amplitude of


title: "1879 Broederstroom" content: 0.12 magnitude (). According to the surveys carried out by the Japanese Akari satellite and NASA's Wide-field Infrared Survey Explorer with its subsequent NEOWISE mission, "Broederstroom" measures 7.444 and 7.66 kilometers in diameter and its surface has an albedo of 0.242 and 0.319, respectively. The "Collaborative Asteroid Lightcurve Link", assumes an albedo of 0.24 – derived from the asteroid 8 Flora, the family's principal body and namesake – and calculates a diameter of 7.14 kilometers with an absolute magnitude of 13.42. This minor planet was named after the village Broederstroom located in the North West province of South Africa. The


title: "1879 Broederstroom" content: Leiden Southern Observatory was later located near this town for 25 years until 1982. The official naming citation was published by the Minor Planet Center on 8 April 1982 (). 1879 Broederstroom 1879 Broederstroom, provisional designation , is a stony Florian asteroid from the inner regions of the asteroid belt, approximately 7 kilometers in diameter. It was discovered on 16 October 1935, by Dutch astronomer Hendrik van Gent at the Leiden Southern Station (), annex to the Johannesburg Observatory in South Africa. The asteroid was named after the South African village of Broederstroom. "Broederstroom" is a member of the Flora


title: "1848 Delvaux" content: 1848 Delvaux 1848 Delvaux, provisional designation , is a stony Koronian asteroid from the outer region of the asteroid belt, approximately 17 kilometers in diameter. It was discovered on 18 August 1933, by Belgian astronomer Eugène Delporte at the Royal Observatory of Belgium in Uccle, Belgium. It was later named after astronomer Georges Roland's sister-in-law. "Delvaux" is a stony asteroid and a member of the Koronis family, a collisional group consisting of a few hundred known bodies with nearly ecliptical orbits. It orbits the Sun in the outer main-belt at a distance of 2.7–3.0 AU once every 4 years and


title: "1848 Delvaux" content: 10 months (1,777 days). Its orbit has an eccentricity of 0.05 and an inclination of 1° with respect to the ecliptic. First identified as at Simeiz Observatory in 1912, the body's observation arc begins 3 day after its official discovery, as non of the previous observations were used. In the SMASS taxonomy "Delvaux" is a common S-type asteroid. It has a well-determined rotation period of 3.63 to 3.65 hours with a brightness variation of 0.57–0.69 magnitude (). The "Collaborative Asteroid Lightcurve Link" (CALL) adopts a period of 3.637 hours. According to the surveys carried out by the Japanese Akari satellite


title: "1848 Delvaux" content: and NASA's Wide-field Infrared Survey Explorer with its subsequent NEOWISE mission, "Delvaux" measures between 16.66 and 17.51 kilometers in diameter, and its surface has an albedo of 0.233 to 0.461. CALL assumes a standard albedo for members of the Koronis family of 0.24, and calculates a diameter of 17.12 kilometers with an absolute magnitude of 11.0. This minor planet was named after the sister-in-law of Georges Roland, astronomer at the observatory in Uccle and known as the co-discoverer of the comet Arend–Roland. The approved naming citation was published by the Minor Planet Center on 8 April 1982 (). 1848 Delvaux


title: "Pakistan Day" content: Pakistan Day Pakistan Day (, lit. "Yaum-e-Pakistan") or Pakistan Resolution Day, also Republic Day, is a national holiday in Pakistan commemorating the Lahore Resolution passed on 23 March 1940 and the adoption of the first constitution of Pakistan during the transition of the Dominion of Pakistan to the Islamic Republic of Pakistan on 23 March 1956 making Pakistan the world's first Islamic republic. A Republic Day parade by the armed forces is often part of the celebrations. The day celebrates the adoption of the Pakistan resolution by the Muslim League at the "Minar-e-Pakistan" (lit. Pakistan Tower) that called for establishing


title: "NYC Condom" content: NYC Condom The NYC Condom, funded by New York City's Department of Health, is a program run by the New York City Department of Health and Mental Hygiene to distribute free condoms. The NYC Condom is the first municipally branded condom in the United States. The NYC Condom was launched on Valentine's Day, 2007 with a highly successful citywide media campaign including bilingual subway ads, radio spots, club launch parties, and street teams distributing the NYC Condom at high pedestrian traffic spots throughout the city. Six months after the unveiling of the NYC Condom, the city's average monthly condom distribution


title: "Reach for the Rainbow" content: worked with a variety of overnight camps since its establishment. These include: Cairn-Glen Mhor (1988), John Island Camp (1989), Pearce Williams Christian Centre (1992), Canterbury Hills Overnight Camp (1993), Camp Kitchikewana (1993), Camp Pine Crest (1993), Camp Wanakita (1994), Ryerson Camp (1997), Silver Lake Camp (1997), Cave Springs Camp (1999), Lambton Centre (2000), Camp Presqu'ile (2001), Camp Ko-Mo-Kee (2003), Forest Cliff Camps (2005), Hidden Bay Leadership Camp (2005), RKY Camp (2005), Camp Maple Leaf (2017), Hockey Opportunity Camp (2017), and Camp Menesetung (2017). "REACH" is supported by the following companies and foundations: Air Canada Foundation, Alice & Murray Maitland Foundation,


title: "Benjamin Moore & Co." content: Benjamin Moore & Co. Benjamin Moore & Co., also known as Benjamin Moore Paints or simply Benjamin Moore, is an American company that produces paint. It is owned by Berkshire Hathaway. Founded in 1883, Benjamin Moore is based in Montvale, New Jersey. The Moore Brothers founded the company in Brooklyn, New York, with one product, "Moore's Prepared Calsom Finish", and sold their paints only through independent retailers. In July 2015, the Asthma and Allergy Foundation of America and Allergy Standards Limited announced that Benjamin Moore's most environmentally friendly paint, Natura®, has been Certified Asthma and Allergy Friendly. “This is the


title: "Benjamin Moore & Co." content: latest step in our long history and commitment to manufacturing green paints that are safer for your family and the environment,” said Chris Connelly, Director of Brand Management, Benjamin Moore. “With zero emissions and no harsh fumes, Natura® truly is an eco-friendly paint that delivers on performance and color integrity.” Benjamin Moore & Co. Benjamin Moore & Co., also known as Benjamin Moore Paints or simply Benjamin Moore, is an American company that produces paint. It is owned by Berkshire Hathaway. Founded in 1883, Benjamin Moore is based in Montvale, New Jersey. The Moore Brothers founded the company in Brooklyn,


title: "Protein–protein interaction screening" content: Protein–protein interaction screening Protein–protein interaction screening refers to the identification of Protein–protein interaction with high-throughput screening methods such as computer- and/or robot-assisted plate reading, flow cytometry analyzing. The interactions between proteins are central to virtually every process in a living cell. Information about these interactions improves understanding of diseases and can provide the basis for new therapeutic approaches. Though there are many methods to detect protein–protein interactions, the majority of these methods—such as co-immunoprecipitation, fluorescence resonance energy transfer (FRET) and dual polarisation interferometry—are not screening approaches. Methods that screen protein–protein interactions in the living cells. Bimolecular fluorescence complementation (BiFC) is


title: "Joe Pack" content: Joe Pack Joe Pack (born April 10, 1978) is an American freestyle skier and Olympic medalist. He received a silver medal at the 2002 Winter Olympics in Salt Lake City, in aerials. Pack is a Latter-day Saint. He was born in Eugene, Oregon. Joe was inducted into the US Ski and Snowboard Hall of Fame in 2001. Pack currently lives in Hawaii as the Head Golf Professional at Turtle Bay Resort. He is married to jewelry designer Vanessa Pack (nee Gardiner). They got married at the historic Maidstone Club in 2008. They have one daughter Gabriella, and a german shepard


title: "Private Jet Expeditions" content: Private Jet Expeditions Private Jet Expeditions was a charter airline that was part of the Oasis Group from Spain. Private Jet Expeditions was founded in 1989 by Wichita, Kansas entrepreneur Jack P. DeBoer and began operations with a former TWA Boeing 727 aircraft to tourist destinations around the world operating under FAR Pt 121. After Deboer sold the company its headquarters was moved to Atlanta, GA and was later owned by Apple Vacations and then by the Spanish consortium OASIS. When Oasis took over, the McDonnell Douglas MD-83 was put into service and service was expanded, including scheduled flights. In


title: "Private Jet Expeditions" content: 1993 it had a scheduled route from Chicago to Atlanta and on to Miami. According to the September 15, 1994 edition of the Official Airline Guide (OAG), the air carrier was operating McDonnell Douglas DC-9-50 and MD-80 jetliners as National Airlines with the same "5J" airline code. According to the OAG, routes at this time included Miami-Atlanta-Dallas/Fort Worth-Las Vegas, New York LaGuardia-Atlanta-Dallas/Fort Worth, Miami-Atlanta-New York LaGuardia, and Chicago Midway-Atlanta-St. Thomas-St.Croix. At one point, an MD-80 was leased by French carrier Air Liberte and used to briefly operate a scheduled Chicago Midway-San Francisco route while retaining the full livery of the


title: "Private Jet Expeditions" content: French carrier. Because of poor load factors these routes were abandoned in 1994 and shortly thereafter Chapter 11 bankruptcy protection was sought. The charter operations did not go well and by March 1995 operations were permanently suspended. Private Jet Expeditions Private Jet Expeditions was a charter airline that was part of the Oasis Group from Spain. Private Jet Expeditions was founded in 1989 by Wichita, Kansas entrepreneur Jack P. DeBoer and began operations with a former TWA Boeing 727 aircraft to tourist destinations around the world operating under FAR Pt 121. After Deboer sold the company its headquarters was moved


title: "Multi-junction solar cell" content: shaded area under the red line represents the maximum work done by ideal infinite multi-junction solar cells. Hence, the limiting efficiency of ideal infinite multi-junction solar cells is evaluated to be 68.8% by comparing the shaded area defined by the red line with the total photon-flux area determined by the black line. (This is why this method is called "graphical" QE analysis.) Although this limiting efficiency value is consistent with the values published by Parrott and Vos in 1979: 64% and 68.2% respectively, there is a small gap between the estimated value in this report and literature values. This minor


title: "Boeing 737 rudder issues" content: Boeing 737 rudder issues During the 1990s, a series of rudder issues on Boeing 737 aircraft resulted in multiple incidents. In two separate accidents, pilots lost control of their Boeing 737 aircraft due to a sudden and unexpected movement of the rudder, and the resulting crashes killed everyone aboard. A total of 157 people aboard the two aircraft were killed. Similar rudder issues led to a temporary loss of control on at least one other Boeing 737 flight before the problem was ultimately identified. The National Transportation Safety Board ultimately determined that the accidents and incidents were the result of


title: "Georgie Welcome" content: Georgie Welcome Georgie Wilson Welcome Collins (born 9 March 1985) is a Honduran Striker. Welcome is the only player to debut with the national side playing in the second level of Honduras. Welcome started his career Arsenal FC (Roatan) and was snapped up by Honduran giants F.C. Motagua in 2008. On 1 August 2010, Welcome travelled to Glasgow to begin a week-long unsuccessful trial with Scottish champions Rangers. In January 2011, Welcome was sent to AS Monaco on loan from Motagua. After an unsuccessful stint in Monaco, Welcome was signed by Mexican league club Atlas to a one-year contract. The


title: "Grand Hallway" content: Grand Hallway Grand Hallway is an American rock band from Seattle, Washington, led by singer and multi-instrumentalist Tomo Nakayama. Their sound is described variously as chamber pop, indie folk, and art rock. Grand Hallway began as a recording project between singer/songwriter Tomo Nakayama and producer Jeramy Koepping. After the dissolution of his first band, Asahi, Nakayama sought a different direction from that band's guitar-based indie rock sound. Using the piano as his main instrument, Nakayama began to write songs inspired by artists such as Nina Simone, Neil Young, and John Lennon. After playing a handful of solo shows, Nakayama recruited


title: "Grand Hallway" content: bassist Erik Neumann and drummer Bob Roberts, and along with Koepping on guitar, began playing out in earnest as Grand Hallway. Strong word of mouth based on a four song demo and live shows opening for the likes of Damien Jurado led to The Stranger declaring them one of the "10 Emerging Bands of 2007." The basic tracks for Grand Hallway's debut album, "Yes is the Answer", were recorded in 3 days at Jack Straw Productions through a grant received from their Artist Support Program. Engineering was performed by Moe Provencher, and overdubs and mixing were completed over the following


title: "Grand Hallway" content: summer by Jeramy Koepping. What began as a minimalist collection of piano/bass/drums songs grew into a fuller, chamber-pop sound with the addition of a string quartet. The cover art was hand drawn by Japanese artist Heisuke Kitazawa, after a chance meeting with Nakayama at an art show in Seattle. "Yes is the Answer" was released in Japan on Sideout Records (Bright Eyes, Nada Surf, The Velvet Teen), and self-released by the band in the U.S. The album was received warmly in both countries. The Stranger praised it, saying it "glows brightly with warm, delicate orchestration and thoughtful song structures." In


title: "Grand Hallway" content: September 2007, joined by new members Alina To and Jaclyn Shumate on violins, Grand Hallway toured Japan with fellow Seattle band Arthur & Yu and Japanese singer/songwriter Shugo Tokumaru. Shortly after touring in Japan and recording the EP "We Flew Ephemera", Bob Roberts left the band to pursue his career as a video game designer, and was replaced by Joel Harmon. Grand Hallway spent 2008 touring the west coast and performing in that year's Sasquatch! Music Festival. During this time, Erik Neumann left the band, and bassist Kevin Large and multi-instrumentalist Chris Zasche joined as full-time members. That fall, the