langs: 1 июня [ru] / june 1 [en] / 1. juni [de] / 1er juin [fr] / 1º giugno [it] / 1 de junio [es]
days: may 29 / may 30 / may 31 / june 1 / june 2 / june 3 / june 4
#1 1832 Mrkos
1832 Mrkos , provisional designation 1969 PC , is a carbonaceous asteroid from the outer region of the asteroid belt , approximately 30 kilometers in diameter. It was discovered on 11 August 1969 by Russian astronomer Lyudmila Chernykh at the Crimean Astrophysical Observatory in Nauchnyj, on the Cri
1858 Lobachevskij ( prov. designation : 1972 QL ) is a rare-type background asteroid from the central region of the asteroid belt , approximately 13 kilometers in diameter. It was discovered on 18 August 1972, by Soviet astronomer Lyudmila Zhuravleva at the Crimean Astrophysical Observatory in Nauch
A minor planet is " lost " when today's observers cannot find it, because its location is too uncertain to target observations. This happens if the orbital elements of a minor planet are not known accurately enough, typically because the observation arc for the object is too short, or too few observ
1822 Waterman , provisional designation 1950 OO , is a stony asteroid from the inner regions of the asteroid belt , approximately 6.5 kilometers in diameter. 1822 Waterman Discovery [1] Discovered by Indiana University ( Indiana Asteroid Program ) Discovery site Goethe Link Obs. Discovery date
1565 Lemaître , provisional designation 1948 WA , is a highly eccentric Phocaea asteroid and sizable Mars-crosser from the inner regions of the asteroid belt , approximately 8 kilometers in diameter. It was discovered on 25 November 1948, by Belgian astronomer Sylvain Arend at the Royal Observatory
#6 1167 Dubiago
1167 Dubiago , provisional designation 1930 PB , is a dark asteroid from the outer region of the asteroid belt , approximately 63 kilometers in diameter. It was discovered on 3 August 1930, by Soviet astronomer Evgenii Skvortsov at Simeiz Observatory on the Crimean peninsula, and named after astrono
#7 6500 Kodaira
6500 Kodaira , provisional designation 1993 ET , is a highly eccentric, rare-type asteroid and sizable Mars-crosser from the central regions of the asteroid belt , approximately 10 kilometers in diameter. It was discovered on 15 March 1993, by Japanese amateur astronomers Kin Endate and Kazuro Watan
1859 Kovalevskaya , provisional designation 1972 RS 2 , is a carbonaceous asteroid from the outer regions of the asteroid belt , approximately 40 kilometers in diameter. 1859 Kovalevskaya Discovery [1] Discovered by L. V. Zhuravleva Discovery site Crimean Astrophysical Obs. Discovery date 4 Se
2126 Gerasimovich , provisional designation 1970 QZ , is a stony background asteroid from the inner regions of the asteroid belt , approximately 8 kilometers in diameter. It was discovered on 30 August 1970, by Soviet astronomer Tamara Smirnova at the Crimean Astrophysical Observatory in Nauchnyj, o
#10 1708 Pólit
1708 Pólit , provisional designation 1929 XA , is a very dark asteroid from the outer region of the asteroid belt , approximately 29 kilometers in diameter. It was discovered on 30 November 1929, by Spanish astronomer of Catalan origin Josep Comas i Solà at the Fabra Observatory in Barcelona, and wa
#11 2028 Janequeo
2028 Janequeo , provisional designation 1968 OB 1 , is a stony Florian asteroid from the inner regions of the asteroid belt , approximately 3 kilometers in diameter. It was discovered on July 18th 1968, by Chilean astronomers Carlos Torres and S. Cofre at the Cerro El Roble Station of Chile's Nation
#12 152188 Morricone
152188 Morricone , provisional designation 2005 QP 51 , is a background asteroid from the central region of the asteroid belt , approximately 3 kilometers (2 miles) in diameter. It was discovered on 27 August 2005, by astronomers Franco Mallia and Alain Maury at the Campo Catino Austral Observatory
#13 1869 Philoctetes
1869 Philoctetes / f ɪ l ə k ˈ t iː t iː z / is a Jupiter trojan from the Greek camp, approximately 23 kilometers in diameter. 1869 Philoctetes Discovery [1] Discovered by C. J. van Houten I. van Houten-G. T. Gehrels Discovery site Palomar Obs. Discovery date 24 September 1960 Designations MPC
#14 2629 Rudra
2629 Rudra , provisional designation 1980 RB 1 , is a sizable Mars-crossing asteroid and slow rotator inside the asteroid belt , approximately 5.3 kilometers (3.3 miles) in diameter. It was discovered on 13 September 1980, by American astronomer Charles Kowal at the Palomar Observatory in California
#15 2325 Chernykh
2325 Chernykh , provisional designation 1979 SP , is a dark Themistian asteroid from the outer regions of the asteroid belt , approximately 23 kilometers (14 miles) in diameter. It was discovered on 25 September 1979, by Czech astronomer Antonín Mrkos at the Klet Observatory in the Czech Republic. T
#16 1149 Volga
1149 Volga , provisional designation 1929 PF , is a dark background asteroid from the outer regions of the asteroid belt , approximately 55 kilometers in diameter. It was discovered on 1 August 1929, by Soviet astronomer Evgenij Skvorcov (a.k.a. Skvortsov) at the Simeiz Observatory on the Crimean pe
#17 (385343) 2002 LV
(385343) 2002 LV , provisional designation 2002 LV , is a stony asteroid on a highly eccentric orbit, classified as near-Earth object and potentially hazardous asteroid of the Apollo group , approximately 1.5 kilometers (0.9 miles) in diameter. It was discovered on 1 June 2002, by astronomers with t
#18 2013 LA2
2013 LA 2 is a centaur and damocloid on a cometary-like and retrograde orbit from the outer Solar System , suggesting that it is an extinct comet . It was first observed on 1 June 2013 by astronomers with the Pan-STARRS survey at Haleakala Observatory , Hawaii, in the United States. [1] The object m
#19 1692 Subbotina
1692 Subbotina , provisional designation 1936 QD , is a dark background asteroid from the central region of the asteroid belt , approximately 37 kilometers (23 miles) in diameter. The carbonaceous Cg -type asteroid has a rotation period of 9.2 hours. [12] It was discovered by Grigory Neujmin at the
#20 Haumea
Haumea ( minor-planet designation 136108 Haumea ) is a dwarf planet located beyond Neptune 's orbit. [24] It was discovered in 2004 by a team headed by Mike Brown of Caltech at the Palomar Observatory in the United States and disputably also in 2005 by a team headed by José Luis Ortiz Moreno at the
#1 Bibliography of encyclopedias: astronomy and astronomers
This is a list of encyclopedias and encyclopedic/biographical dictionaries published on the subject of astronomy and astronomers in any language. Entries are in the English language except where noted. Wikipedia bibliography This list is incomplete ; you can help by adding missing items . ( Septembe
#2 SIMBAD
SIMBAD (the S et of I dentifications, M easurements and B ibliography for A stronomical D ata) is an astronomical database of objects beyond the Solar System . It is maintained by the Centre de données astronomiques de Strasbourg (CDS), France . Astronomical database For other uses, see Simbad (disa
The Great Comet of 1882 formally designated C/1882 R1 , 1882 II , and 1882b , was a comet which became very bright in September 1882. It was a member of the Kreutz Sungrazers , a family of comets which pass within 1 R ☉ of the Sun's photosphere at perihelion . [1] [2] The comet was bright enough t
#2 C/1881 K1
C/1881 K1 (also called the Great Comet of 1881 , Comet Tebbutt , 1881 III , 1881b ) is a long-period comet discovered by John Tebbutt on 22 May 1881 [2] at Windsor, New South Wales . It is called a great comet because of its brightness at its last apparition. [3] C/1881 K1 The great comet of 1881, c
#3 85D/Boethin
Comet Boethin (officially 85D/Boethin ) was a periodic Jupiter-family comet discovered in 1975 by Leo Boethin. It appeared again in January 1986 as expected. Although the comet was next expected at perihelion in April 1997, no observations were reported, and the comet is thought to have disintegrate
Comet White–Ortiz–Bolelli (formal designations: C/1970 K1 , 1970 VI , and 1970f ) was a bright comet which appeared in 1970. It was a member of the Kreutz Sungrazers , a family of comets which resulted from the break-up of a large parent comet several centuries ago. It was already easily visible to
C/2019 Y4 (ATLAS) (or Comet ATLAS ) is a comet with a near-parabolic orbit discovered by the ATLAS survey on December 28, 2019. [3] Early predictions based on the brightening rate suggested that the comet could become as bright as magnitude 0 matching the brightness of Vega . [4] It received widespr
#6 41P/Tuttle–Giacobini–Kresák
41P/Tuttle–Giacobini–Kresák is a periodic comet in the Solar System . The comet nucleus is estimated to be 1.4 kilometers in diameter. [1] Periodic comet with 5 year orbit 41P/Tuttle–Giacobini–Kresák Comet 41P/Tuttle–Giacobini–Kresák on 2017, 3 March near the galaxy Messier 108 and Owl Nebula . Disc
#1 Messier 13
Messier 13 or M13 , also designated NGC 6205 and sometimes called the Great Globular Cluster in Hercules or the Hercules Globular Cluster , is a globular cluster of several hundred thousand stars in the constellation of Hercules . Globular cluster in the constellation Hercules Messier 13 Globular cl
#2 NGC 6054
NGC 6054 is a barred [2] lenticular galaxy located about 460 million light-years away [3] in the constellation Hercules . [4] It was discovered by astronomer Lewis Swift on June 27, 1886. [5] [6] It was then rediscovered by astronomer Guillaume Bigourdan on June 1, 1888. PGC 57073 is often misidenti
The Florence and George Wise Observatory (IAU code 097) is an astronomical observatory owned and operated by Tel Aviv University . It is located 5 kilometers (3.1 miles) west of the town of Mitzpe Ramon in the Negev desert near the edge of the Ramon Crater , and it is the only professional astronomi
Meudon Castle , also known as the Royal Castle of Meudon or Imperial Palace of Meudon, is a French castle located in Meudon in the Hauts-de-Seine department . At the edge of a wooded plateau, the castle offers views of Paris and the Seine , as well as of the Chalais valley. Located between Paris and
#3 Ondokuz Mayıs University Observatory
The Ondokuz Mayıs University Observatory ( Turkish : Ondokuz Mayıs Üniversitesi Gözlemevi ) is a ground-based astronomical observatory operated by the Astronomy and Space Sciences Department at Ondokuz Mayıs University 's Faculty of Science. Established on June 1, 2006, it is located within the univ
The Archenhold Observatory ( German : Archenhold-Sternwarte ) was named in honour of Friedrich Simon Archenhold , is an observatory in Berlin-Treptow . It houses the Großer Refraktor (Great Refractor), which is the longest pointable telescope in the world. It is also called the Himmelskanone (Celest
Morrison Observatory is an astronomical observatory owned and operated by Central Methodist University located in Fayette , Missouri (USA). It was named after Bernice Morrison who, in 1874, pledged $100,000 to C. W. Pritchett for the construction of the observatory. Half of that amount would go the
#6 List of solar eclipses visible from Russia
This list of solar eclipses visible from Russia enumerates the solar eclipses that have been seen and will be seen in Russia . Lists of solar eclipses Geometry of a total solar eclipse (not to scale) Solar eclipses in antiquity Solar eclipses in the Middle Ages Modern history 16th 17th 18th 19th 20t
The Orange County Astronomers (OCA) is a 501(c)(3) non-profit , civilian-led astronomy organization in Orange County , southern California. [1] [2] It was formed in 1967 and currently operates with around 800 concurrent members; they offer beginner courses in astronomy, and have meetings on the seco
The William Herschel Telescope ( WHT ) is a 4.20-metre (165 in) optical / near-infrared reflecting telescope located at the Roque de los Muchachos Observatory on the island of La Palma in the Canary Islands , Spain. The telescope, which is named after William Herschel , the discoverer of the plane
#9 Association of Universities for Research in Astronomy
The Association of Universities for Research in Astronomy ( AURA ) is a consortium of universities and other institutions that operates astronomical observatories and telescopes . Operating consortium for observatories and telescopes The Association of Universities for Research in Astronomy at the U
#10 LIGO
The Laser Interferometer Gravitational-Wave Observatory ( LIGO ) is a large-scale physics experiment and observatory designed to detect cosmic gravitational waves and to develop gravitational-wave observations as an astronomical tool. [1] Two large observatories were built in the United States with
#11 List of solar eclipses visible from Ukraine
This list of solar eclipses seen from Ukraine enumerates the solar eclipses that were seen and will be seen in Ukraine . Lists of solar eclipses Geometry of a total solar eclipse (not to scale) Solar eclipses in antiquity Solar eclipses in the Middle Ages Modern history 16th 17th 18th 19th 20th 21st
The Manuel Foster Observatory , originally known as the D. O. Mills Observatory after the philanthropist Darius Ogden Mills , is an astronomical observatory constructed on Cerro San Cristóbal near Santiago, Chile in 1903. It was originally built as an offshoot of the Lick observatory to observe star
The Črni Vrh Observatory ( Slovene : Observatorij Črni Vrh , IAU code : 106 ) is an astronomical observatory located in western Slovenia , close to the settlement of Črni Vrh , near the town of Idrija . The current observatory was built in 1985 and stands at an elevation of 730 metres (2,400 ft) .
#14 IAU Working Group on Star Names
The International Astronomical Union (IAU) established a Working Group on Star Names ( WGSN ) in May 2016 to catalog and standardize proper names for stars for the international astronomical community. [1] It operates under Division C – Education, Outreach and Heritage. [2] IAU group to catalog an
#1 WASP-79b
WASP-79b is an extrasolar planet orbiting the star CD-30 1812. This planet is in the constellation Eridanus , and is about 810 light-years from Earth. Exoplanet WASP-79b Discovery Discovered by Smalley et al. [1] Discovery date June 1 2012 [1] Detection method Transit method [1] Orbital characte
#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
Timothy B. Hunter , better known as Tim Hunter , is an American radiologist and amateur astronomer , who was the president of the International Dark-Sky Association . [1] American radiologist and amateur astronomer
#2 Colin Ronan
Colin Alistair Ronan FRAS (4 June 1920, in London – 1 June 1995) was a British author and specialist in the history and philosophy of science . [1] [2] British author (1920–1995) Colin Alistair Ronan Born ( 1920-06-04 ) 4 June 1920 London Died 1 June 1995 (1995-06-01) (aged 74)
#3 Kip Thorne
Kip Stephen Thorne (born June 1, 1940) is an American theoretical physicist known for his contributions in gravitational physics and astrophysics . A longtime friend and colleague of Stephen Hawking and Carl Sagan , he was the Richard P. Feynman Professor of Theoretical Physics at the California I
Charles Scott Venable (March 19, 1827 – August 11, 1900) was a mathematician , astronomer , and military officer . In mathematics, he is noted for authoring a series of publications as a University of Virginia professor. Charles Scott Venable Born ( 1827-03-19 ) March 19, 1827 Prince Edward County,
Snježana Kordić ( pronounced [sɲěʒana kôːrditɕ] ( listen ) ; born 29 October 1964) [1] is a Croatian linguist . [3] In addition to her work in syntax , she has written on sociolinguistics . [2] Kordić is known among non-specialists for numerous articles against the puristic and prescriptive langua
Geminiano Montanari (1 June 1633 – 13 October 1687) was an Italian astronomer , lens -maker, and proponent of the experimental approach to science. He was a member of various learned academies, notably the Accademia dei Gelati . Montanari's famous students were Domenico Guglielmini , Francesco Bianc
Sylvain Julien Victor Arend (6 August 1902 – 18 February 1992) was a Belgian astronomer born in Robelmont , Luxembourg province, Belgium . His main interest was astrometry . [2] Belgian astronomer Minor planets discovered: 51 [1] see § List of discovered minor planets Together with Georges Rolan
#8 Okuro Oikawa
Okuro Oikawa ( 及川 奥郎 , Oikawa Okurō , 1896–1970) [2] was a Japanese astronomer and discoverer of minor planets . [3] Japanese astronomer Minor planets discovered: 8 [1] 1088 Mitaka 17 November 1927 MPC 1089 Tama 17 November 1927 MPC 1090 Sumida 20 February 1928 MPC 1098 Hakone 5 September 1928 MPC
#9 Arthur Hoag
Arthur Allen Hoag (January 28, 1921 - July 17, 1999) was an American astronomer most famous for his discovery of Hoag's Object , a type of ring galaxy , in 1950. American astronomer Arthur Hoag Born ( 1921-01-28 ) 28 January 1921 Ann Arbor , Michigan , United States Died 17 July 1999 (1999-07-17) (a
#10 Phil Diamond
Philip John Diamond HonFInstP is a Professor in the School of Physics and Astronomy at the University of Manchester . He was the director of the Jodrell Bank Centre for Astrophysics from 1 October 2006 until 2010. He was the Chief of CSIRO 's Astronomy and Space Sciences Division from 1 June 2010 [2
#11 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
#12 Anil Bhardwaj
Anil Bhardwaj (born 1 June 1967) is an Indian astrophysicist. He is the Director of the Physical Research Laboratory, [1] which is a Unit of the Department of Space of Government of India in Ahmedabad, India. Indian astrophysicist (born 1967) For the Indian cricketer, see Anil Bhardwaj (cricketer) .
#13 Marc Buie
Marc William Buie ( / ˈ b uː i / ; born 1958) is an American astronomer and prolific discoverer of minor planets who works at the Southwest Research Institute in Boulder, Colorado in the Space Science Department. [1] Formerly he worked at the Lowell Observatory in Flagstaff, Arizona, and was the Sen
#14 Agnes Giberne
Agnes Giberne (19 November 1845 in Belgaum , India – 20 August 1939 in Eastbourne , England ) was a prolific British novelist and scientific writer. [1] Her fiction was typical of Victorian evangelical fiction with moral or religious themes for children. She also wrote books on science for young peo
Carmen Adelina Gutiérrez Alonso (aka Adelina Gutiérrez , May 27, 1925 – April 11, 2015) was a Chilean scientist , academic and professor of astrophysics . [1] She was the first Chilean to obtain a doctoral degree in astrophysics and the first woman to become a member of the Chilean Academy of Scienc
Dr. Walter F. Huebner (born February 22, 1928 in New York City; died June 1, 2021 in Norman, Oklahoma) was an astrophysicist who wrote several books on comets including close-orbit and asteroids that may collide with the Earth, and how to prevent catastrophic collisions. American astrophysicist (192
#17 Michel Ory
Michel Ory (born 18 April 1966) is a Swiss amateur astronomer and a prolific discoverer of minor planets and comets , [1] who was one of five winners of the 2009 Edgar Wilson Award for his discovery of 304P/Ory (P/2008 Q2 Ory), a periodic comet of the Jupiter family on 27 August 2008, [2] using a 24
#18 George O. Abell
George Ogden Abell (March 1, 1927 – October 7, 1983) was an American educator. Teaching at UCLA , priorly he worked as a research astronomer , administrator, as a popularizer of science and of education, and as a skeptic . He earned his B.S. in 1951, his M.S. in 1952 and his Ph.D. in 1957, all from
#19 Eduard Mahler
Eduard Mahler ( Hungarian : Mahler Ede , September 28, 1857, Cífer , Austro-Hungarian Empire – June 29, 1945, Újpest ) was a Hungarian - Austrian astronomer , Orientalist , and natural scientist . Austro-Hungarian scientist He graduated from a Vienna public school in 1876 and then studied mathematic
Sir Charles Todd KCMG FRS FRAS FRMS FIEE [1] (7 July 1826 – 29 January 1910) worked at the Royal Greenwich Observatory 1841–1847 and the Cambridge University observatory from 1847 to 1854. He then worked on telegraphy and undersea cables until engaged by the government of South Australia as astronom
#1 Beta Corvi
Beta Corvi or β Corvi , officially named Kraz ( / ˈ k r æ z / ), [11] is the second-brightest star in the southern constellation of Corvus with an apparent visual magnitude of 2.647. [2] Based on parallax measurements obtained during the Hipparcos mission, it is about 146 light-years (45 parsecs
#2 Beta Cancri
Beta Cancri ( β Cancri , abbreviated Beta Cnc , β Cnc ), also named Tarf / ˈ t ɑːr f / , [9] is the brightest star in the zodiacal constellation of Cancer . It has an apparent visual magnitude of +3.5 [2] and an absolute magnitude of −1.2. [6] Based on parallax measurements obtained during the Hippa
#3 GW170104
GW170104 was a gravitational wave signal detected by the LIGO observatory on 4 January 2017. On 1 June 2017, the LIGO and Virgo collaborations announced that they had reliably verified the signal, making it the third such signal announced , after GW150914 and GW151226 , and fourth overall. [1] [2] G
#4 Alruba
Alruba , [9] a name derived from Arabic for "the foal", is a suspected astrometric binary [10] star system in the northern circumpolar constellation of Draco . It is just barely visible to the naked eye as a dim point of light with an apparent visual magnitude of 5.76. [2] Based on parallax measurem
#5 Eta Piscium
Eta Piscium ( η Piscium , abbreviated Eta Psc , η Psc ) is a binary star and the brightest point of light in the constellation of Pisces with an apparent visual magnitude of +3.6. [2] Based upon a measured annual parallax shift of 9.33 mas as seen from Earth, [1] it is located roughly 350 light-
#6 Xi Aquarii
Xi Aquarii ( ξ Aquarii , abbreviated Xi Aqr , ξ Aqr ) is a binary star system in the equatorial constellation of Aquarius . It is visible to the naked eye with an apparent visual magnitude of 4.7. [2] Based upon parallax measurements made during the Hipparcos mission, this system lies at a distance
#7 Zeta Aquilae
Zeta Aquilae , or ζ Aquilae , is a binary star [10] system in the equatorial constellation of Aquila . It is readily visible with the naked eye, being of the third magnitude. [2] Based on parallax measurements obtained during the Hipparcos mission, it is approximately 83 light-years (25 parsecs ) di
#8 Algol
Algol / ˈ æ l ɡ ɒ l / , [9] designated Beta Persei ( β Persei , abbreviated Beta Per , β Per ), known colloquially as the Demon Star , is a bright multiple star in the constellation of Perseus and one of the first non- nova variable stars to be discovered. Eclipsing variable star in the conste
Theta Columbae , also named Elkurud / ˈ ɛ l k ə r ʌ d / , [10] is a solitary [11] star in the southern constellation of Columba . It is faintly visible to the naked eye, having an apparent visual magnitude of 5.02. [2] Based upon parallax measurements taken during the Hipparcos mission, it is roughl
#10 List of proper names of stars
These names of stars that have either been approved by the International Astronomical Union or which have been in somewhat recent use. IAU approval comes mostly from its Working Group on Star Names , which has been publishing a "List of IAU-approved Star Names" since 2016. As of August 2018, the lis
#11 Xi Puppis
Xi Puppis ( ξ Puppis , abbreviated Xi Pup , ξ Pup ) is a multiple star system in the southern constellation of Puppis . With an apparent visual magnitude of 3.35, [2] it is one of the brighter members of this constellation. Based on parallax measurements made during the Hipparcos mission, it
Over the past few centuries, a small number of stars have been named after individual people. It is common in astronomy for objects to be given names, in accordance with accepted astronomical naming conventions . Most stars have not been given proper names , relying instead on alphanumeric designati
#13 Iota Hydrae
Iota Hydrae ( ι Hydrae , abbreviated Iota Hya , ι Hya ), formally named Ukdah / ˈ ʌ k d ə / , [7] is a star in the constellation of Hydra , about 8° to the north-northwest of Alphard (Alpha Hydrae) [8] and just to the south of the celestial equator . [9] Visible to the naked eye, it is a suspected v
#14 Supernova
A supernova is a powerful and luminous explosion of a star . It has the plural form supernovae /- v iː / or supernovas , and is abbreviated SN or SNe . This transient astronomical event occurs during the last evolutionary stages of a massive star or when a white dwarf is triggered into runaway nucle
#15 Epsilon Hydrae
Epsilon Hydrae ( ε Hydrae , abbreviated Epsilon Hya , ε Hya ) is a multiple star system of a combined third magnitude in the constellation of Hydra . Based upon parallax measurements obtained during the Hipparcos mission, it is located roughly 129 light-years (40 parsecs ) distant from the Sun . [1]
#16 Zeta Virginis
Zeta Virginis ( ζ Virginis , abbreviated Zeta Vir , ζ Vir ) is a binary star in the zodiac constellation of Virgo . It is visible to the naked eye with an apparent visual magnitude of +3.376 and is located about a half degree south of the celestial equator . Based on parallax measurements obtained d
#17 Xi Cancri
Xi Cancri ( ξ Cancri , abbreviated Xi Cnc , ξ Cnc ) is a spectroscopic binary star system in the zodiac constellation of Cancer . It is visible to the naked eye with an apparent visual magnitude of +5.15. [2] Based upon parallax measurements obtained during the Hipparcos mission, [1] it is roughly 3
#18 Beta Piscium
Beta Piscium or β Piscium , formally named Fumalsamakah / ˌ f ʌ m əl ˈ s æ m ə k ə / , [10] is a blue-white hued star in the zodiac constellation of Pisces . Its apparent magnitude is 4.40, [2] meaning it can be faintly seen with the naked eye. Based on parallax measurements taken during the Hippa
#19 HD 85951
HD 85951 ( HR 3923 ), formally named Felis / ˈ f iː l ɪ s / , [13] is a solitary [14] orange hued star in the constellation Hydra . It has an apparent magnitude of 4.94, [2] making faintly visible to the naked eye under ideal conditions. Based on parallax measurements, the object is about 570 light-
#20 Delta Cygni
Delta Cygni ( δ Cygni , abbreviated Delta Cyg , δ Cyg ) is a binary star of a combined third-magnitude in the constellation of Cygnus . It is also part of the Northern Cross asterism whose brightest star is Deneb . Based upon parallax measurements obtained during the Hipparcos mission, Delta Cygni i