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langs: 13 июня [ru] / june 13 [en] / 13. juni [de] / 13 juin [fr] / 13 giugno [it] / 13 de junio [es]

days: june 10 / june 11 / june 12 / june 13 / june 14 / june 15 / june 16

Asteroid / Asteroid


#1 2111 Tselina

2111 Tselina ( prov. designation : 1969 LG ) is a stony Eos asteroid from the outer regions of the asteroid belt . It was discovered on 13 June 1969, by Soviet astronomer Tamara Smirnova at Crimean Astrophysical Observatory in Nauchnij, on the Crimean peninsula. [12] The S-type asteroid has a rotati

#2 198 Ampella

Ampella ( minor planet designation : 198 Ampella ) is a Main belt asteroid that was discovered by Alphonse Borrelly on June 13, 1879. The name seems to be the feminine form of Ampelos , a satyr and good friend of Dionysus in Greek mythology . It could also derive from the Ampelose (plural of Ampelos

#3 10251 Mulisch

10251 Mulisch , provisional designation 3089 T-1 , is a bright background asteroid from the inner regions of the asteroid belt , approximately 2.4 kilometers (1.5 miles) in diameter. It was discovered during the Palomar–Leiden Trojan survey on 26 March 1971, by Ingrid and Cornelis van Houten at Leid

#4 132524 APL

132524 APL , provisional designation 2002 JF 56 , is a small background asteroid in the intermediate asteroid belt . It was discovered by Lincoln Near-Earth Asteroid Research in May 2002, [1] and imaged by the New Horizons space probe on its flyby in June 2006, when it was passing through the astero

#5 4337 Arecibo

4337 Arecibo ( prov. designation : 1985 GB ) is a binary Themistian asteroid from the outer regions of the asteroid belt , approximately 24 kilometers (15 miles) in diameter. It was discovered on 14 April 1985, by American astronomer Edward Bowell at the Anderson Mesa Station near Flagstaff, Arizona

#6 1566 Icarus

1566 Icarus ( / ˈ ɪ k ər ə s / IK -ə-rəs ; provisional designation : 1949 MA ) is a large near-Earth object of the Apollo group and the lowest numbered potentially hazardous asteroid . [20] It has is an extremely eccentric orbit (0.83) and measures approximately 1.4   km (0.87   mi) in diameter. In

#7 30000 Camenzind

30000 Camenzind , provisional designation 2000 AB 138 , is a very bright background asteroid from the inner region of the asteroid belt , approximately 2.6 kilometers (1.6 miles) in diameter. It was discovered on 4 January 2000, by astronomers of the Lincoln Near-Earth Asteroid Research program cond

#8 3361 Orpheus

3361 Orpheus (1982 HR) is an Apollo asteroid that was discovered on 24 April 1982 by Carlos Torres at Cerro El Roble Astronomical Station . Its eccentric orbit crosses that of Mars and Earth , and approaches Venus as well. From 1900 to 2100 it passes closer than 30   Gm to Venus 11, Earth 33, and Ma

#9 4672 Takuboku

4672 Takuboku , provisional designation 1988 HB , is a background asteroid from the outer regions of the asteroid belt , approximately 35 kilometers (22 miles) in diameter. It was discovered on 17 April 1988, by Japanese astronomers Seiji Ueda and Hiroshi Kaneda at the Kushiro Observatory on Hokkaid

#10 25143 Itokawa

25143 Itokawa (provisional designation 1998 SF 36 ) is a sub-kilometer near-Earth object of the Apollo group and a potentially hazardous asteroid . It was discovered by the LINEAR program in 1998 and later named after Japanese rocket engineer Hideo Itokawa . [1] The peanut-shaped S-type asteroid has

#11 1806 Derice

1806 Derice , provisional designation 1971 LC , is a stony Flora asteroid from the inner regions of the asteroid belt , approximately 10 kilometers in diameter. Discovered on 13 June 1971, at the Bickley site of the Perth Observatory in Western Australia, it was the first discovery of a minor planet

#12 List of minor planets discovered using the WISE spacecraft

The following is a list of numbered minor planets discovered, co-discovered and re-discovered by the Wide-field Infrared Survey Explorer (WISE), a NASA infrared spaceborne observatory. As of July 2018, the list contains 4093 entries, accredited by the Minor Planet Center as discovered by "WISE". Not

#13 132 Aethra

Aethra ( minor planet designation : 132 Aethra ) is a metallic asteroid and Mars-crosser on an eccentric orbit from the asteroid belt . It measures approximately 40 kilometers in diameter. 132 Aethra Lightcurve -based 3D-model of Aethra Discovery Discovered   by James C. Watson Discovery   date 13 J

#14 1349 Bechuana

1349 Bechuana , provisional designation 1934 LJ , is a background asteroid from the outer regions of the asteroid belt , approximately 26 kilometers in diameter. It was discovered on 13 June 1934, by South-African astronomer Cyril Jackson at the Union Observatory in Johannesburg. [13] The asteroid w


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Book / Book


#1 Star catalogue

A star catalogue is an astronomical catalogue that lists stars . In astronomy , many stars are referred to simply by catalogue numbers. There are a great many different star catalogues which have been produced for different purposes over the years, and this article covers only some of the more frequ

#2 Gaia catalogues

The Gaia catalogues are star catalogues created using the results obtained by Gaia space telescope. Catalogues consisting of data from the Gaia misson. The catalogues are released in stages that will contain increasing amounts of information; the early releases also miss some stars, especially faint


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Comet / Comet


#1 Comet ISON

Comet ISON , formally known as C/2012 S1 , was a sungrazing comet from the Oort cloud which was discovered on 21 September 2012 by Vitaly Nevsky (Виталий Невский, Vitebsk , Belarus ) and Artyom Novichonok (Артём Новичонок, Kondopoga , Russia ). [4] Oort cloud comet C/2012 S1 (ISON) Comet ISON as cap

#2 C/2008 T2 (Cardinal)

C/2008 T2 (Cardinal) , is a non-periodic comet . It was discovered by Rob. D. Cardinal from the University of Calgary . [1] [4] [5] It was visible as a telescopic and binocular object during 2009. [5] [6] It passed near the Perseus star clusters NGC 1528 on March 15 and NGC 1545 on March 17, 2009. [

#3 100P/Hartley

100P/Hartley , also known as Hartley 1 , is a periodic, Jupiter family comet in the Solar System . [1] This article is about 100P/Hartley. For other comets, see Comet Hartley . Periodic comet with 6 year orbit 100P/Hartley Discovery Discovered by Malcolm Hartley Discovery date June 13, 1985 Alternat

#4 P/2019 LD2 (ATLAS)

P/2019 LD 2 (ATLAS) is a Jupiter-family comet discovered by the Asteroid Terrestrial-impact Last Alert System on 10 June 2019. [6] [7] It was initially reported as the first known Jupiter trojan asteroid to display cometary activity, [8] but its classification as a Jupiter trojan was retracted after

#5 C/2007 K5 (Lovejoy)

C/2007 K5 (Lovejoy) [1] is a periodic comet , discovered on 26 May 2007 by amateur astronomer Terry Lovejoy . [2] Periodic comet For other comets discovered by Terry Lovejoy, see Comet Lovejoy . C/2007 K5 (Lovejoy) Discovery Discovered by Terry Lovejoy Discovery date 26 May 2007 Orbital characterist

#6 128P/Shoemaker–Holt

128P/Shoemaker–Holt , also known as Shoemaker-Holt 1 , is a periodic comet in the Solar System . The comet passed close to Jupiter in 1982 and was discovered in 1987. The comet was last observed in March 2018. [4] Periodic comet with 9 year orbit 128P/Shoemaker-Holt Discovery Discovered by Carolyn S

#7 Comet Holmes

Comet Holmes / ˈ h oʊ m z / (official designation: 17P/Holmes ) is a periodic comet in the Solar System , discovered by the British amateur astronomer Edwin Holmes on November 6, 1892. Although normally a very faint object, Holmes became notable during its October 2007 return when it temporarily bri

#8 Great Comet of 1901

The Great Comet of 1901 , sometimes known as Comet Viscara , formally designated C/1901 G1 (and in the older nomenclature as 1901 I and 1901a ), was a comet which became bright in the spring of 1901. Visible exclusively (or almost exclusively) [2] from the southern hemisphere , it was discovered on

#9 C/2009 R1 (McNaught)

C/2009 R1 (McNaught) , one of more than fifty comets known as Comet McNaught , [4] is a non-periodic comet discovered by British-Australian astronomer Robert H. McNaught on September 9, 2009, using the Uppsala Southern Schmidt Telescope at Siding Spring Observatory in New South Wales , Australia . [


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Galaxy / Galaxy


#1 Sagittarius Dwarf Irregular Galaxy

The Sagittarius Dwarf Irregular Galaxy ( SagDIG ) is a dwarf galaxy in the constellation of Sagittarius . (SagD I G should not be confused with the Sagittarius Dwarf Spheroidal Galaxy , SagD E G, a satellite galaxy of the Milky Way discovered decades later in the same constellation.) It lies about 3

#2 NGC 6373

NGC 6373 is a barred spiral galaxy located in the constellation Draco . It is designated as SBc in the galaxy morphological classification scheme and was discovered by the American astronomer Lewis A. Swift on 13 June 1885. There are two recorded supernovae in this galaxy designated SN 2001ad and SN


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Institution / Institution


#1 Galileo Galilei Planetarium

The Galileo Galilei planetarium , commonly known as Planetario , is located in Parque Tres de Febrero in the Palermo district of Buenos Aires , Argentina . Planetarium in Buenos Aires (Argentina) This article does not cite any sources . ( July 2021 ) This article may be expanded with text translated

#2 Stamford Museum & Nature Center

The Stamford Museum & Nature Center , located in Stamford, Connecticut , is an art, history, nature, and agricultural sciences museum . The property covers 118 acres (ca. 48 hectares) beginning about half a mile north of the Merritt Parkway . It was originally a private estate. Stamford Museum & Nat

#3 Union Observatory

Union Observatory also known as Johannesburg Observatory ( 078 ) is a defunct astronomical observatory in Johannesburg , South Africa that was operated between 1903 and 1971. It is located on Observatory Ridge , the city's highest point at 1,808 metres altitude in the suburb Observatory . [1] [2] De

#4 Arecibo Telescope

The Arecibo Telescope was a 305   m (1,000   ft) spherical reflector radio telescope built into a natural sinkhole at the Arecibo Observatory located near Arecibo, Puerto Rico . A cable-mount steerable receiver and several radar transmitters for emitting signals were mounted 150   m (492   ft) above

#5 Campo Imperatore Near-Earth Object Survey

The CINEOS program ( Campo Imperatore Near-Earth Object Survey ), started in 2001, is dedicated to the discovery and follow-up of near-Earth objects (NEOs), namely asteroids and comets which periodically approach or intersect the Earth's orbit . In particular CINEOS is addressed to the discovery of


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Meteorite / Meteorite


#1 Gliese 876 d

Gliese 876 d is an exoplanet approximately 15 light-years away in the constellation of Aquarius . The planet was the third planet discovered orbiting the red dwarf Gliese 876 . It was the lowest- mass extrasolar planet apart from the pulsar planets orbiting PSR B1257+12 at the time of its discovery.

#2 HD 49674 b

HD 49674 b is an extrasolar planet [1] located approximately 134 light-years away in the constellation of Auriga , orbiting the star HD 49674 . This planet was discovered orbiting the star in 2002. The planet is a gas giant and orbits extremely close to its star, which takes only 4.95 days to revolv

#3 Mu Arae e

Mu Arae e , also known as HD 160691 e , later named Sancho / ˈ s æ n tʃ oʊ / , [2] is one of the four extrasolar planets orbiting the star Mu Arae of the constellation Ara . Extrasolar planet in the constellation Ara Mu Arae e Mu Arae e rendered by Celestia Discovery Discovered   by Butler , Marcy D

#4 HD 37124 c

HD 37124 c is an extrasolar planet approximately 103 light-years away in the constellation of Taurus . The planet was discovered in 2002 orbiting the star HD 37124 . [1] The planet is most likely to be a gas giant (based on its mass). Extrasolar planet HD 37124 c Discovery Discovered   by Marcy et a

#5 Kesen meteorite

The Kesen Meteorite is a meteorite that fell on June 13, 1850, landing in a swamp in the outskirts of the City of Rikuzentakata , Kesen District in Iwate Prefecture , Japan . Kesen meteorite Kesen meteorite, main mass Type Chondrite Class Ordinary chondrite Group H4 Country Japan Region Rikuzentakat

#6 HD 196050 b

HD 196050 b is a 1378-day extrasolar planet with a minimum mass of 2.90 Jupiter mass . The average orbital distance is 2.54 astronomical units or 380 gigameters or 12.3 microparsecs . The orbital eccentricity is 22.8%. The periastron (closest) distance is 1.96 AU and the apastron (farthest) distance

#7 Kepler-1647b

Kepler-1647b (sometimes named Kepler-1647(AB)-b to distinguish it from the secondary component) is a circumbinary exoplanet that orbits the binary star system Kepler-1647, 3,700 light-years (1,100   pc) from Earth in the constellation Cygnus . [2] It was announced on June 13, 2016, in San Diego at a

#8 HD 72659 b

HD 72659 b is a superjovian exoplanet massing at least 3.3 M J orbiting at 4.77 AU from the star taking 3630 days to orbit. The orbital distance range from 3.49 AU to 6.05 AU with orbital eccentricity of 0.269. [2] In 2022, the inclination and true mass of HD 72659 b were measured via astrometry . [

#9 55 Cancri c

55 Cancri c (abbreviated 55 Cnc c ), formally named Brahe (pronounced / ˈ b r ɑː h iː / or / ˈ b r ɑː / ), is an extrasolar planet in an eccentric orbit around the Sun -like star 55 Cancri A , making one revolution every 44.34 days . It is the third known planet in order of distance from its star. 5

#10 55 Cancri d

55 Cancri d (abbreviated 55 Cnc d ), formally named Lipperhey / ˈ l ɪ p ər h iː / , is an extrasolar planet in a long-period orbit around the Sun -like star 55 Cancri A . Located at a similar distance from its star as Jupiter is from our Sun, it is the fifth and outermost known planet in its planeta

#11 HD 40979 b

HD 40979 b is an extrasolar planet orbiting the star HD 40979 , was detected from the Lick and Keck observatories and photometric observations at Fairborn Observatory reveal low-amplitude brightness variations in HD 40979. It is thought to be a large gas giant planet. It was discovered in 2002 by De

#12 HD 30177 b

HD 30177 b is an extrasolar planet located approximately 181.6 light-years away in the constellation of Dorado , orbiting the star HD 30177 . Extrasolar planet in the constellation Dorado HD 30177 b Discovery Discovered   by Tinney , Butler , Marcy et al. Discovery   site Anglo-Australian Planet Sea


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Planet / Planet


#1 Anglo-Australian Planet Search

The Anglo Australian Planet Search or ( AAPS ) is a long-term astronomical survey started in 1998 and continuing to the present. It is being carried out on the 3.9-metre Anglo-Australian Telescope (AAT) of the Anglo-Australian Observatory in Australia . The purpose of this survey is to catalog plane


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Researcher / Researcher


#1 James Craig Watson

James Craig Watson (January 28, 1838 – November 22, 1880) was a Canadian - American astronomer , discoverer of comets and minor planets , director of the University of Michigan's Detroit Observatory in Ann Arbor, and awarded with the Lalande Prize in 1869. [1] [2] Canadian-American astronomer For ot

#2 Paul G. Comba

Paul G. Comba (1926 – April 5, 2017) was an Italian-American computer scientist , an amateur astronomer and a prolific discoverer of minor planets . [2] Paul G. Comba Born 1926   ( 1926 ) Tunisia Died April 4, 2017 (2017-04-04) (aged   90–91) Education Ph.D. Alma   mater University of Turin , Blufft

#3 George K. Miley

George Kildare Miley (born 15 March 1942) is an Irish-Dutch astronomer . He holds a professorship at Leiden University , where he served as director of Leiden Observatory from 1996 to 2003. [1] Irish-Dutch astronomer George K. Miley Born ( 1942-03-15 ) 15 March 1942 (age   80) Dublin , Ireland Alma

#4 Fritz Cohn

Fritz Cohn , RAS Associate [1] (12 May 1866 – 14 December 1922) was a German astronomer and professor of astronomy at the University of Berlin . Throughout his career he worked at numerous observatories and was director of the Astronomical Calculation Institute . His main work was in astrometry and

#5 Mary Rosse

The Rt Hon. Mary Parsons, Countess of Rosse ( née Mary Field) (14 April 1813 – 1885), was a British Irish amateur astronomer , architect, furniture designer, and pioneering photographer. Often known simply as Mary Rosse , she was one of the early practitioners of making photographs from waxed-paper

#6 Bindon Blood Stoney

Bindon Blood Stoney FRS (13 June 1828, Oakley Park, County Offaly – 5 May 1909, Dublin ) was an Irish engineer who also made some significant contributions to astronomy. [1] Bindon Blood Stoney Plaque to Stoney at the Dublin Port Centre Born 13 June 1828   ( 1828-06-13 ) Oakley Park, County Offaly D

#7 Giovanni Antonio Magini

Giovanni Antonio Magini (in Latin , Maginus ) (13 June 1555 – 11 February 1617) was an Italian astronomer , astrologer , cartographer , and mathematician . Italian mathematician and astronomer For the crater, see Maginus (crater) . For the saint, see Saint Maginus . Giovanni Antonio Magini, Italian

#8 James Westphal

James Adolph Westphal (June 13, 1930 – September 8, 2004) was an American academic , scientist , engineer , inventor and astronomer and Director of Caltech's Palomar Observatory from 1994 through 1997. [1] This article is about the astronomer. For the business professor, see James D. Westphal . His

#9 William Bayly (astronomer)

William Bayly (1737–1810) was an English astronomer. English astronomer

#10 Michel Lefrançois de Lalande

Michel Lefrançois de Lalande (21 April 1766 – 8 April 1839) was a French astronomer. French astronomer (1766–1839) Michel Lefrançois de Lalande Portrait at physionotrace of Michel Lefrançois de Lalande.

#11 Prem Saran Satsangi

Prem Saran Satsangi is the eighth and current Sant Satguru [1] of Radhasoami Faith , Dayalbagh . [2] He holds the Emeritus Chair from the East of the Integrated East-West Forum at The Science of Consciousness Conferences since 2012. [3] He is the chairman of Advisory Committee on Education, Dayalbag

#12 Robert H. McNaught

Robert H. McNaught (born in Scotland in 1956) is a Scottish-Australian astronomer at the Research School of Astronomy and Astrophysics of the Australian National University (ANU). He has collaborated with David J. Asher of the Armagh Observatory . Scottish-Australian astronomer (born 1956) Minor pla

#13 Stephen P. Laurie

Stephen P. Laurie is a British amateur astronomer . He is a prolific discoverer of asteroids and comets , [1] although his profession is that of an actuary . [2] He has also worked on searches for dwarf stars [3] and discovered a supernova (SN 1997bq in NGC 3147) in 1997. [2] [4] British astronomer

#14 Anders Spole

Anders Spole (13 June 1630 – 1 August 1699) was a Swedish mathematician and astronomer. He was born at a farm in Målen   [ sv ] , the son of blacksmith Per Andersson and his wife Gunilla Persdotter. [1] At the age of twelve he started studying at Jönköpings skola and was sent to the University of Gr

#15 Cyril Jackson (astronomer)

Cyril V. Jackson (5 December 1903 – February 1988) was a South African astronomer , known for discovering 72 asteroids and a number of comets. South African astronomer Asteroids discovered: 72 1116 Catriona 5 April 1929 1186 Turnera 1 August 1929 1193 Africa 24 April 1931 1194 Aletta 13 May 1931 119

#16 Carl K. Seyfert

Carl Keenan Seyfert (February 11, 1911 – June 13, 1960) was an American astronomer . He is best known for his 1943 research paper on high-excitation line emission from the centers of some spiral galaxies, which are named Seyfert galaxies after him. Seyfert's Sextet , a group of galaxies, is also nam

#17 Henry E. Holt

Henry E. Holt (27 September 1929 - 5 May 2019) [2] was an American astronomer and prolific discoverer of minor planets and comets , who has worked as a planetary geologist at the United States Geological Survey and Northern Arizona University . [3] American astronomer (1929–2019) For other people na

#18 Gerald J. Wasserburg

Gerald J. Wasserburg (March 25, 1927 – June 13, 2016) was an American geologist. At the time of his death, he was the John D. MacArthur Professor of Geology and Geophysics, Emeritus, at the California Institute of Technology . He was known for his work in the fields of isotope geochemistry , cosmoch

#19 Willebrord Snellius

Willebrord Snellius [1] [2] (born Willebrord Snel van Royen ) [3] (13 June 1580 [4]   – 30 October 1626) was a Dutch astronomer and mathematician , AKA Snell . His name is usually associated with the law of refraction of light known as Snell's law . [5] Dutch astronomer This article may be expanded

#20 Alphonse Borrelly

Alphonse Louis Nicolas Borrelly (December 8, 1842 – February 28, 1926) was a French astronomer . French astronomer This article needs additional citations for verification . ( July 2015 ) Asteroids discovered: 18 99 Dike May 28, 1868 110 Lydia April 19, 1870 117 Lomia September 12, 1871 120 Lachesis


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Star / Star


#1 HD 30177

HD 30177 is an 8th magnitude star located approximately 182 light-years (56 parsecs ) away in the constellation Dorado . The star is a yellow dwarf , a type of yellow star that fuses hydrogen in its core. Since if this star is a late G-type, it is cooler and less massive than the Sun , but larger in

#2 SN 2003gd

SN 2003gd was a Type II-P supernova explosion in the spiral galaxy Messier 74 , located in the constellation Pisces . SN 2003gd was discovered on 12 June 2003 by Robert Evans , using a 0.31m reflector , and its discovery was confirmed on 13 June 2003 by R. H. McNaught using the 1.0m telescope at the

#3 Gliese 876

Gliese 876 is a red dwarf approximately 15 light-years away from Earth in the constellation of Aquarius . It is one of the closest known stars to the Sun confirmed to possess a planetary system with more than two planets, after Gliese 1061 , YZ Ceti , Tau Ceti , and Luyten's Star ; as of 2018, four

#4 Polaris

Polaris is a star in the northern circumpolar constellation of Ursa Minor . It is designated α Ursae Minoris ( Latinized to Alpha Ursae Minoris ) and is commonly called the North Star or Pole Star . With an apparent magnitude that fluctuates around 1.98, [3] it is the brightest star in the constella

#5 HD 73526

HD 73526 is a star in the southern constellation of Vela . With an apparent visual magnitude of +8.99, [2] it is much too faint to be viewed with the naked eye. The star is located at a distance of approximately 318   light years from the Sun based on parallax , [1] and is drifting further away with

#6 Circumbinary planet

A circumbinary planet is a planet that orbits two stars instead of one. The two stars orbit each other in a binary star system, while the planet typically orbits farther from the center of the system than either of the two stars, although planets in stable orbits around one of the two stars in a bin


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