Stars Named After People
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Over the past few centuries, a small number of
star A star is an astronomical object comprising a luminous spheroid of plasma (physics), plasma held together by its gravity. The List of nearest stars and brown dwarfs, nearest star to Earth is the Sun. Many other stars are visible to the naked ...
s have been named after individual people. It is common in
astronomy Astronomy () is a natural science that studies astronomical object, celestial objects and phenomena. It uses mathematics, physics, and chemistry in order to explain their origin and chronology of the Universe, evolution. Objects of interest ...
for objects to be given names, in accordance with accepted
astronomical naming conventions In ancient times, only the Sun and Moon, a few stars, and the most easily visible planets had names. Over the last few hundred years, the number of identified astronomical objects has risen from hundreds to over a billion, and more are discovered ...
. Most stars have not been given
proper names A proper noun is a noun that identifies a single entity and is used to refer to that entity (''Africa'', ''Jupiter'', '' Sarah'', ''Microsoft)'' as distinguished from a common noun, which is a noun that refers to a class of entities (''continent, ...
, relying instead on alphanumeric designations in
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, ...
s. However, a few hundred had either long-standing traditional names (usually from the
Arabic Arabic (, ' ; , ' or ) is a Semitic languages, Semitic language spoken primarily across the Arab world.Semitic languages: an international handbook / edited by Stefan Weninger; in collaboration with Geoffrey Khan, Michael P. Streck, Janet C ...
) or historic names from frequent usage. In addition, many stars have catalogue designations that contain the name of their compiler or discoverer. This includes Wolf, Ross, Bradley, Piazzi, Lacaille, Struve, Groombridge, Lalande, Krueger, Mayer, Weisse, Gould, Luyten and others. For example,
Wolf 359 Wolf 359 is a red dwarf star located in the constellation Leo, near the ecliptic. At a distance of approximately 7.9 light years from Earth, it has an apparent magnitude of 13.54 and can only be seen with a large telescope. Wolf 359 i ...
was discovered and catalogued by
Max Wolf Maximilian Franz Joseph Cornelius Wolf (21 June 1863 – 3 October 1932) was a German astronomer and a pioneer in the field of astrophotography. He was the chairman of astronomy at the University of Heidelberg and director of the Heidelberg-K ...
. Various private organizations claim to name stars in honor of people in exchange for a fee, but these names are used only within their own publications, and are not recognized by the scientific community.


Names approved by the IAU

The
International Astronomical Union The International Astronomical Union (IAU; french: link=yes, Union astronomique internationale, UAI) is a nongovernmental organisation with the objective of advancing astronomy in all aspects, including promoting astronomical research, outreac ...
(IAU) is widely recognized by scientists and governments as the world authority for names of astronomical bodies, and lays down strict standards for this naming. In July 2014 the IAU launched
NameExoWorlds NameExoWorlds (also known as IAU NameExoWorlds) is the name of various projects managed by the International Astronomical Union (I.A.U.) to encourage names to be submitted for astronomical objects, which would later be considered for official ad ...
, a process for giving proper names to exoplanets and their host stars, the outcome of which was announced in December 2015. As a result, the IAU approved two star names after individuals: *Cervantes for the star
Mu Arae Mu Arae (μ Arae, abbreviated Mu Ara, μ Ara), often designated HD 160691, officially named Cervantes , is a main sequence G V star, G-type star approximately 50 light-years away from the Sun in the constellation of Ara (constellation), A ...
honoring the writer
Miguel de Cervantes Miguel de Cervantes Saavedra (; 29 September 1547 (assumed) – 22 April 1616 Old Style and New Style dates, NS) was an Early Modern Spanish writer widely regarded as the greatest writer in the Spanish language and one of the world's pre-emin ...
*Copernicus for the star 55 Cancri A honoring the astronomer
Nicolaus Copernicus Nicolaus Copernicus (; pl, Mikołaj Kopernik; gml, Niklas Koppernigk, german: Nikolaus Kopernikus; 19 February 1473 – 24 May 1543) was a Renaissance polymath, active as a mathematician, astronomer, and Catholic Church, Catholic cano ...
In 2016, the IAU organized a
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. It operates under Division C – Education ...
(WGSN) which will catalog cultural and historical names for bright stars to help preserve astronomical world heritage, and maintain a catalog of IAU-approved unique proper names for stars. The WGSN's first bulletin of July 2016 set out its terms of reference and naming guidelines. All approved names are included on the current List of IAU-approved Star Names, last updated on 1 June 2018. The WGSN rules generally discouraged the naming of stars after people, but confirmed the names Cervantes and Copernicus as well as four others: *
Barnard's Star Barnard's Star is a red dwarf about six light-years from Earth in the constellation of Ophiuchus. It is the fourth-nearest-known individual star to the Sun after the three components of the Alpha Centauri system, and the closest star in the ...
, the fourth-closest star to the solar system, named after the American astronomer E. E. Barnard who discovered it has the highest known
proper motion Proper motion is the astrometric measure of the observed changes in the apparent places of stars or other celestial objects in the sky, as seen from the center of mass of the Solar System, compared to the abstract background of the more dista ...
of any star. *
Cor Caroli Cor Caroli is a binary star designated Alpha Canum Venaticorum or α Canum Venaticorum. The International Astronomical Union uses the name "Cor Caroli" specifically for the brighter star of the binary. Alpha Canum Venaticorum is the brig ...
(
Latin Latin (, or , ) is a classical language belonging to the Italic branch of the Indo-European languages. Latin was originally a dialect spoken in the lower Tiber area (then known as Latium) around present-day Rome, but through the power of the ...
for 'heart of Charles') for the star Alpha Canum Venaticorum, so named in honour of
King Charles I of England Charles I (19 November 1600 – 30 January 1649) was King of England, Scotland, and Ireland from 27 March 1625 until his execution in 1649. He was born into the House of Stuart as the second son of King James VI of Scotland, but after hi ...
by Sir
Charles Scarborough Sir Charles Scarborough or Scarburgh Member of Parliament, MP Fellow of the Royal Society, FRS Fellow of the Royal College of Physicians, FRCP (29 December 1615 – 26 February 1694) was an English physician and mathematician.Robert L. Martensen, ...
, his physician. * Sualocin and Rotanev for components of
Alpha Alpha (uppercase , lowercase ; grc, ἄλφα, ''álpha'', or ell, άλφα, álfa) is the first letter of the Greek alphabet. In the system of Greek numerals, it has a value of one. Alpha is derived from the Phoenician letter aleph , whic ...
and
Beta Delphini Beta Delphini (β Delphini, abbreviated Beta Del, β Del) is a binary star in the constellation of Delphinus. It is the brightest star in Delphinus. The two components of the system are designated Beta Delphini A ...
, two stars which appeared in the Palermo star catalogue of 1814. They were eventually identified as the reversed spelling of ''Nicolaus Venator'', a Latinised version of Nicolò Cacciatore, assistant to the astronomer
Giuseppe Piazzi Giuseppe Piazzi ( , ; 16 July 1746 – 22 July 1826) was an Italian Catholic priest of the Theatine order, mathematician, and astronomer. He established an observatory at Palermo, now the '' Osservatorio Astronomico di Palermo – Giuseppe ...
. It is not clear whether Piazzi intended to name the stars after his assistant, or if Cacciatore made the names up himself. In 2019, the IAU held a second NameExoWorlds campaign to celebrate the 100th anniversary of the IAU's founding. *
Azerbaijan Azerbaijan (, ; az, Azərbaycan ), officially the Republic of Azerbaijan, , also sometimes officially called the Azerbaijan Republic is a transcontinental country located at the boundary of Eastern Europe and Western Asia. It is a part of th ...
named the star HD 152581 (16h 53m 44s / +11° 58′ 25″, in
Ophiuchus Ophiuchus () is a large constellation straddling the celestial equator. Its name comes from the Ancient Greek (), meaning "serpent-bearer", and it is commonly represented as a man grasping a snake. The serpent is represented by the constella ...
) as Mahsati (
Mahsati Mahsati ( fa, مهستی, Māhsatī) was a medieval Persian female poet who was reportedly one of the first poets to compose '' ruba'iyat'' (quatrains) in her native language. Name Various interpretations of her name have been suggested based ...
). *
Cuba Cuba ( , ), officially the Republic of Cuba ( es, República de Cuba, links=no ), is an island country comprising the island of Cuba, as well as Isla de la Juventud and several minor archipelagos. Cuba is located where the northern Caribbea ...
named the star BD−17 63 as Felixvarela (
Félix Varela Félix Varela y Morales (November 20, 1788 – February 18, 1853) was a Cuban Catholic priest and independence leader who is regarded as a notable figure in the Catholic Church in both his native Cuba and the United States, where he also served. ...
). *
India India, officially the Republic of India (Hindi: ), is a country in South Asia. It is the seventh-largest country by area, the second-most populous country, and the most populous democracy in the world. Bounded by the Indian Ocean on the so ...
named the star HD 86081 as Bibha (
Bibha Chowdhuri Bibha Chowdhuri (3 July 1913 – 2 June 1991) was an Indian physicist. She worked on particle physics and cosmic rays. The IAU has re-christened the star HD 86081 as Bibha (a yellow-white dwarf star in the constellation Sextans south of the cele ...
). *
Spain , image_flag = Bandera de España.svg , image_coat = Escudo de España (mazonado).svg , national_motto = ''Plus ultra'' (Latin)(English: "Further Beyond") , national_anthem = (English: "Royal March") , i ...
named the star HD 149143 as Rosalíadecastro (
Rosalía de Castro María Rosalía Rita de Castro (; 23 February 1837 – 15 July 1885), was a Galician poet and novelist, considered one of the most important figures of the 19th-century Spanish literature and modern lyricism. Widely regarded as the greatest Galic ...
).


Names not approved by the IAU

Apart from the few formally approved by the IAU, and leaving aside commercial attempts, stars named after individuals fall broadly into two groups. The first group are those named openly for an individual connected with them in some way. The second, somewhat more obscurely, are those named after an individual but without explicitly making this clear.


Openly named stars

There is a growing number of stars whose common names honour individuals. Many of these were highly significant in some way when discovered, usually through having some unusual characteristic. The best source to get these names is Sky Catalogue 2000.0, Volume 2 (Double Stars, Variable Stars, and Nonstellar Objects), in the chapter Glossary Of Selected Astronomical Names. *Abt's Star is SV Crateris (ADS 8115/ HD 98088/ β 600) in
Crater Crater may refer to: Landforms *Impact crater, a depression caused by two celestial bodies impacting each other, such as a meteorite hitting a planet *Explosion crater, a hole formed in the ground produced by an explosion near or below the surfac ...
. Named after
Helmut Abt Helmut Arthur Abt (born 26 May 1925) is a German-born American astrophysicist, having worked at the National Optical Astronomy Observatory and an Elected Fellow of the American Association for the Advancement of Science. He is astronomer emeri ...
. *Andrews' Star is a suspected variable star in
Auriga AURIGA (''Antenna Ultracriogenica Risonante per l'Indagine Gravitazionale Astronomica'') is an ultracryogenic resonant bar gravitational wave detector in Italy. It is at the Laboratori Nazionali di Legnaro of the Istituto Nazionale di Fisica Nuclea ...
( HD 37519 / SAO 58319 / HR 1938). Named after A. David Andrews. *Anthelm's Nova/Star is Nova 1670 Vulpeculae, observed by Anthelme Voituret (aka père Anthelme / don Anthelme). *Argelander's Star is
Groombridge 1830 Groombridge 1830 (also known as 1830 Groombridge or Argelander's Star)Peters, C. A. F.; "On the Parallax of Argelander's Star", Monthly Notices of the Royal Astronomical Society, December 1853, v.50, p.302, is a star in the constellatio ...
, a high proper motion star. Named for
Friedrich Wilhelm Argelander Friedrich Wilhelm August Argelander (22 March 1799 – 17 February 1875) was a German astronomer. He is known for his determinations of stellar brightnesses, positions, and distances. Life and work Argelander was born in Memel in the Kingd ...
, who discovered its high proper motion in 1842. *Argelander's second star is
Lalande 21185 Lalande 21185 (also known as BD+36 2147, Gliese 411, and HD 95735) is a star in the south of Ursa Major. It is the apparent brightest red dwarf in the northern hemisphere.Only AX Microscopii and Lacaille 9352, in the southern hemisphere ...
, a nearby
red dwarf ''Red Dwarf'' is a British science fiction comedy franchise created by Rob Grant and Doug Naylor, which primarily consists of a television sitcom that aired on BBC Two between 1988 and 1999, and on Dave since 2009, gaining a cult following. T ...
star. Named also for Argelander, who discovered its high
proper motion Proper motion is the astrometric measure of the observed changes in the apparent places of stars or other celestial objects in the sky, as seen from the center of mass of the Solar System, compared to the abstract background of the more dista ...
in 1857. *Baade's Star is the pulsar in the
Crab Nebula The Crab Nebula (catalogue designations Messier object, M1, New General Catalogue, NGC 1952, Taurus (constellation), Taurus A) is a supernova remnant and pulsar wind nebula in the constellation of Taurus (constellation), Taurus. The common name ...
(Messier 1,
Taurus Taurus is Latin for 'bull' and may refer to: * Taurus (astrology), the astrological sign * Taurus (constellation), one of the constellations of the zodiac * Taurus (mythology), one of two Greek mythological characters named Taurus * ''Bos taurus ...
). Also known as the
Crab Pulsar The Crab Pulsar (PSR B0531+21) is a relatively young neutron star. The star is the central star in the Crab Nebula, a remnant of the supernova SN 1054, which was widely observed on Earth in the year 1054.Walter Baade Wilhelm Heinrich Walter Baade (March 24, 1893 – June 25, 1960) was a German astronomer who worked in the United States from 1931 to 1959. Biography The son of a teacher, Baade finished school in 1912. He then studied maths, physics and astro ...
. *Babcock's Magnetic Star is HD 215441 in
Lacerta Lacerta is one of the 88 modern constellations defined by the International Astronomical Union. Its name is Latin for lizard Lizards are a widespread group of squamate reptiles, with over 7,000 species, ranging across all continents except ...
. Named after
Horace W. Babcock Horace Welcome Babcock (September 13, 1912 – August 29, 2003) was an American astronomer. He was the son of Harold D. Babcock. Career Babcock invented and built a number of astronomical instruments, and in 1953 was the first to propose th ...
. *Becklin's Star is IRC -10093 in Messier 42, Orion. Named after
Eric Becklin Eric E. Becklin (born 6 April 1940) is an American astrophysicist. The primary focus of Becklin's research is infrared imaging and spectroscopy, including the search for brown dwarfs, the detection of circumstellar dust rings, the dynamics a ...
. *The
Becklin–Neugebauer Object The Becklin–Neugebauer Object (BN) is an object visible only in the infrared in the Orion molecular cloud 1 (OMC1). It was discovered in 1967 by Eric Becklin and Gerry Neugebauer during their near-infrared survey of the Orion Nebula. ...
is an infrared source, possibly a
protostar A protostar is a very young star that is still gathering mass from its parent molecular cloud. The protostellar phase is the earliest one in the process of stellar evolution. For a low-mass star (i.e. that of the Sun or lower), it lasts about 5 ...
, in the
Orion molecular cloud complex The Orion molecular cloud complex (or, simply, the Orion complex) is a star-forming region with stellar ages ranging up to 12 Myr. Two giant molecular clouds are a part of it, Orion A and Orion B. The stars currently forming within the complex a ...
. Named after
Eric Becklin Eric E. Becklin (born 6 April 1940) is an American astrophysicist. The primary focus of Becklin's research is infrared imaging and spectroscopy, including the search for brown dwarfs, the detection of circumstellar dust rings, the dynamics a ...
and
Gerry Neugebauer Gerhart "Gerry" Neugebauer (3 September 1932 – 26 September 2014) was an American astronomer known for his pioneering work in infrared astronomy. Neugebauer was born in Göttingen, Germany and was the son of Otto Neugebauer, an Austrian-Ameri ...
. *Bessel's Star is
61 Cygni 61 Cygni is a binary star system in the constellation Cygnus, consisting of a pair of K-type dwarf stars that orbit each other in a period of about 659 years. Of apparent magnitude 5.20 and 6.05, respectively, they can be seen ...
, for a short time the nearest star whose distance was accurately known (measured by
Friedrich Bessel Friedrich Wilhelm Bessel (; 22 July 1784 – 17 March 1846) was a German astronomer, mathematician, physicist, and geodesist. He was the first astronomer who determined reliable values for the distance from the sun to another star by the method ...
in 1838). Also called Piazzi's Flying Star, since
Giuseppe Piazzi Giuseppe Piazzi ( , ; 16 July 1746 – 22 July 1826) was an Italian Catholic priest of the Theatine order, mathematician, and astronomer. He established an observatory at Palermo, now the '' Osservatorio Astronomico di Palermo – Giuseppe ...
nominated it as a good candidate for distance measurements ( parallaxes). *Bidelman's helium variable star is V761 Centauri (
HD 125823 HD 125823, also known as V761 Centauri or a Centauri, is a variable star in the constellation Centaurus. It is a blue-white star that is visible to the naked eye with a mean apparent visual magnitude of +4.41. The distance to this star ...
). Named after
William P. Bidelman William Pendry Bidelman ( ; September 25, 1918 – May 3, 2011)PV Telescopii variable PV Telescopii variable is a type of variable star that is established in the ''General Catalogue of Variable Stars'' with the acronym PVTEL. This class of variables are defined as "helium supergiant Bp stars with weak hydrogen lines and enhanced l ...
. *Bidelman's high-latitude Be star is HD 127617 in Bootes. *Bond's Flare Star is V3885 in Sagittarius (Sky Catalogue 2000.0 shows wrong coordinates, 23:31 / -2°45' in Pisces). *Borrelly's Star is probably S Ceti (0h 23.8m / -9° 28'). Named after
Alphonse Borrelly Alphonse Louis Nicolas Borrelly (December 8, 1842 – February 28, 1926) was a French astronomer. He joined the Marseille Observatory in 1864. In the course of his career, he discovered a number of asteroids and comets, including the periodic c ...
. *Boyajian's Star (or Tabby's Star) is
KIC 8462852 Tabby's Star (also known as Boyajian's Star and WTF Star, and designated KIC 8462852 in the Kepler Input Catalog) is an F-type main-sequence star in the constellation Cygnus approximately from Earth. Unusual light fluctuations of the s ...
, an F-type main-sequence star with a highly unusual
light curve In astronomy, a light curve is a graph of light intensity of a celestial object or region as a function of time, typically with the magnitude of light received on the y axis and with time on the x axis. The light is usually in a particular frequ ...
in the
constellation A constellation is an area on the celestial sphere in which a group of visible stars forms Asterism (astronomy), a perceived pattern or outline, typically representing an animal, mythological subject, or inanimate object. The origins of the e ...
of Cygnus, named after
Tabetha S. Boyajian Tabetha "Tabby" Suzanne Boyajian is an American astronomer of Armenian descent and astrophysicist on faculty at Louisiana State University. She was a post-doctoral fellow 2012–16 at Yale University, working with Debra Fischer. Boyajian is acti ...
; its peculiar characteristics engendered speculation that a
Dyson sphere A Dyson sphere is a hypothetical megastructure that completely encompasses a star and captures a large percentage of its solar power output. The concept is a thought experiment that attempts to explain how a spacefaring civilization would meet ...
of an extraterrestrial civilization had been discovered. *Branchett's Object (Star) is a possible
nova A nova (plural novae or novas) is a transient astronomical event that causes the sudden appearance of a bright, apparently "new" star (hence the name "nova", which is Latin for "new") that slowly fades over weeks or months. Causes of the dramati ...
in
Scutum The ''scutum'' (; plural ''scuta'') was a type of shield used among Italic peoples in antiquity, most notably by the army of ancient Rome starting about the fourth century BC. The Romans adopted it when they switched from the military formati ...
(1981). *The Brendan Downs Supernova is SN 1997de, in Pavo (in galaxy NGC 6769). *Brewer's Star is HD 50169 (a magnetic star) in
Monoceros Monoceros (Greek: Μονόκερως, "unicorn") is a faint constellation on the celestial equator. Its definition is attributed to the 17th-century Dutch cartographer Petrus Plancius. It is bordered by Orion to the west, Gemini to the north, ...
. Named after K. R. W. Brewer. *Butler's Star is BT Tucanae / HD 6090 (a
flare star A flare star is a variable star that can undergo unpredictable dramatic increases in brightness for a few minutes. It is believed that the flares on flare stars are analogous to solar flares in that they are due to the magnetic energy stored in th ...
at 1:00:18 / -72°44'35" in the
Small Magellanic Cloud The Small Magellanic Cloud (SMC), or Nubecula Minor, is a dwarf galaxy near the Milky Way. Classified as a dwarf irregular galaxy, the SMC has a D25 isophotal diameter of about , and contains several hundred million stars. It has a total mass of ...
). Named after C. J. Butler. * Caffau's Star is an ultra-metal-poor
halo Halo, halos or haloes usually refer to: * Halo (optical phenomenon) * Halo (religious iconography), a ring of light around the image of a head HALO, halo, halos or haloes may also refer to: Arts and entertainment Video games * ''Halo'' (franch ...
star named after the astronomer Elisabetta Caffau. *Campbell's Star is HD 184738, which is the nucleus of
planetary nebula A planetary nebula (PN, plural PNe) is a type of emission nebula consisting of an expanding, glowing shell of ionized gas ejected from red giant stars late in their lives. The term "planetary nebula" is a misnomer because they are unrelated to ...
PK 64 + 5.1, in Cygnus. Named after
William Wallace Campbell William Wallace Campbell (April 11, 1862 – June 14, 1938) was an American astronomer, and director of Lick Observatory from 1901 to 1930. He specialized in spectroscopy. He was the tenth president of the University of California from 1923 to 1 ...
. *
Cayrel's Star BPS CS31082-0001, named Cayrel's Star , is an old Population II star located in a distance of 2.1 kpc in the galactic halo. It belongs to the class of ultra-metal-poor stars (metallicity Fe/Hydrogen.html"_;"title="Iron.html"_;"title="/ ...
is an ultra-metal-poor halo star named after the French astronomer Roger Cayrel. *Chanal's variable star is a suspected variable star in Orion (NSV 2229). *Chavira's Supernova is SN 1965h in NGC 4666 (in
Virgo Virgo may refer to: *Virgo (astrology), the sixth astrological sign of the zodiac *Virgo (constellation), a constellation *Virgo Cluster, a cluster of galaxies in the constellation Virgo *Virgo Stellar Stream, remains of a dwarf galaxy *Virgo Supe ...
). Named after E. Chavira. *Chevremont's Star is a variable star in
globular cluster A globular cluster is a spheroidal conglomeration of stars. Globular clusters are bound together by gravity, with a higher concentration of stars towards their centers. They can contain anywhere from tens of thousands to many millions of membe ...
Messier 2 Messier 2 or M2 (also designated NGC 7089) is a globular cluster in the constellation Aquarius, five degrees north of the star Beta Aquarii. It was discovered by Jean-Dominique Maraldi in 1746, and is one of the largest known globular clusters. ...
, in
Aquarius Aquarius may refer to: Astrology * Aquarius (astrology), an astrological sign * Age of Aquarius, a time period in the cycle of astrological ages Astronomy * Aquarius (constellation) * Aquarius in Chinese astronomy Arts and entertainment ...
. *Chuadze's Supernova is SN 1967c in NGC 3389 (in Leo). Named after A. D. Chuadze. *Chu's Object (Star?) in
Perseus In Greek mythology, Perseus (Help:IPA/English, /ˈpɜːrsiəs, -sjuːs/; Greek language, Greek: Περσεύς, Romanization of Greek, translit. Perseús) is the legendary founder of Mycenae and of the Perseid dynasty. He was, alongside Cadmus ...
, named after You-Hua Chu. *The Cohen–Schwartz Star is a
T Tauri star T Tauri stars (TTS) are a class of variable stars that are less than about ten million years old. This class is named after the prototype, T Tauri, a young star in the Taurus star-forming region. They are found near molecular clouds and iden ...
and infrared source in Orion. Named after M. Cohen and R. D. Schwartz. *Eggen's Nearby Star is CoD -31°622 in
Sculptor Sculpture is the branch of the visual arts that operates in three dimensions. Sculpture is the three-dimensional art work which is physically presented in the dimensions of height, width and depth. It is one of the plastic arts. Durable sc ...
. Briefly thought to be near the solar system but later found not to be. Named after Olin J. Eggen. *Fehrenbach's Star is HD 116745 in globular cluster
Omega Centauri Omega Centauri (ω Cen, NGC 5139, or Caldwell 80) is a globular cluster in the constellation of Centaurus that was first identified as a non-stellar object by Edmond Halley in 1677. Located at a distance of , it is the largest-known globular clust ...
. Named after Charles Fehrenbach. *Herschel's Garnet Star is
Mu Cephei Mu Cephei ( Latinized from μ Cephei, abbreviated Mu Cep or μ Cep), also known as Herschel's Garnet Star, Erakis, or HD 206936, is a red supergiant or hypergiant star in the constellation Cepheus. It appears garnet red and is located at ...
, a
red supergiant Red supergiants (RSGs) are stars with a supergiant luminosity class ( Yerkes class I) of spectral type K or M. They are the largest stars in the universe in terms of volume, although they are not the most massive or luminous. Betelgeuse and Anta ...
particularly remarkable for its deep red color, first described by
William Herschel Frederick William Herschel (; german: Friedrich Wilhelm Herschel; 15 November 1738 – 25 August 1822) was a German-born British astronomer and composer. He frequently collaborated with his younger sister and fellow astronomer Caroline H ...
. *Herschel's Wonder Star is
Beta Monocerotis Beta Monocerotis (Beta Mon, β Monocerotis, β Mon) is a triple star system in the constellation of Monoceros. To the naked eye, it appears as a single star with an apparent visual magnitude of approximately 3.74 ...
. *Hind's Crimson Star is
R Leporis R Leporis (R Lep), sometimes called Hind's Crimson Star, is a well-known variable star in the constellation Lepus, near its border with Eridanus. It is designated "R" in the chart to the right. It is a carbon star which app ...
, a long-period
variable star A variable star is a star whose brightness as seen from Earth (its apparent magnitude) changes with time. This variation may be caused by a change in emitted light or by something partly blocking the light, so variable stars are classified as ...
, named after the discoverer
John Russell Hind John Russell Hind FRS FRSE LLD (12 May 1823 – 23 December 1895) was an English astronomer. Life and work John Russell Hind was born in 1823 in Nottingham, the son of lace manufacturer John Hind and Elizabeth Russell, and was educated at ...
. It is one of the reddest stars visible (a typical Cool Carbon Star, CCS). *Hind's New Star is
V841 Ophiuchi V841 Ophiuchi (Nova Ophiuchi 1848) was a bright nova discovered by John Russell Hind on 27 April 1848. It was the first object of its type discovered since 1670. At the time of its discovery, it had an apparent magnitude of 5.6, but m ...
, or Nova Ophiuchi 1848. *Hoffmeister's Star is V442 Cassiopeiae (aka Sonneberg 9484). Named after
Cuno Hoffmeister Cuno Hoffmeister (2 February 1892 – 2 January 1968) was a German astronomer, observer and discoverer of variable stars, comets and minor planets, and founder of Sonneberg Observatory. Born in Sonneberg in 1892 to Carl and Marie Hoffmeister, Cu ...
. *Honda's Variable Star is a
long-period variable star The descriptive term long-period variable star refers to various groups of cool luminous pulsating variable stars. It is frequently abbreviated to LPV. Types of variation The General Catalogue of Variable Stars does not define a long-period vari ...
(not a nova) in Cygnus *The
Hulse–Taylor binary The Hulse–Taylor binary is a binary star system composed of a neutron star and a pulsar (known as PSR B1913+16, PSR J1915+1606 or PSR 1913+16) which orbit around their common center of mass. It is the first binary pulsar ever discovere ...
is PSR B1913+16 (a binary pulsar) in Aquila. Named after
Russell Alan Hulse Russell Alan Hulse (born November 28, 1950) is an American physicist and winner of the Nobel Prize in Physics, shared with his thesis advisor Joseph Hooton Taylor Jr., "''for the discovery of a new type of pulsar, a discovery that has opened up n ...
and
Joseph Hooton Taylor Jr. Joseph Hooton Taylor Jr. (born March 29, 1941) is an American astrophysicist and Nobel Prize laureate in Physics for his discovery with Russell Alan Hulse of a "new type of pulsar, a discovery that has opened up new possibilities for the study ...
This discovery won them the
Nobel Prize in Physics ) , image = Nobel Prize.png , alt = A golden medallion with an embossed image of a bearded man facing left in profile. To the left of the man is the text "ALFR•" then "NOBEL", and on the right, the text (smaller) "NAT•" then " ...
in 1993. *Huruhata's Object is an
eclipsing binary A binary star is a system of two stars that are gravitationally bound to and in orbit around each other. Binary stars in the night sky that are seen as a single object to the naked eye are often resolved using a telescope as separate stars, in wh ...
in
Canis Minor Canis Minor is a small constellation in the northern celestial hemisphere. In the second century, it was included as an asterism, or pattern, of two stars in Ptolemy's 48 constellations, and it is counted among the 88 modern constellation ...
. Named after . *Huruhata's Variable is the WZ Sagittae type
dwarf nova A U Geminorum-type variable star, or dwarf nova (pl. novae) is one of several types of cataclysmic variable star, consisting of a close binary star system in which one of the components is a white dwarf that accretes matter from its companion. Dw ...
EG Cancri. * Innes' star, better known as LHS 40, is a high proper-motion star named after
Robert T. A. Innes Robert Thorburn Ayton Innes FRSE FRAS (10 November 1861 – 13 March 1933) was a Scottish astronomer best known for discovering Proxima Centauri in 1915, and numerous binary stars. He was also the first astronomer to have seen the Great January ...
, the discoverer of
Proxima Centauri Proxima Centauri is a small, low-mass star located away from the Sun in the southern constellation of Centaurus. Its Latin name means the 'nearest tarof Centaurus'. It was discovered in 1915 by Robert Innes and is the nearest-kno ...
. In 1930 Luyten listed this as the fifth-closest star system, but his belief was mistaken as it turned out to be 41
light-year A light-year, alternatively spelled light year, is a large unit of length used to express astronomical distances and is equivalent to about 9.46 trillion kilometers (), or 5.88 trillion miles ().One trillion here is taken to be 1012 ...
s away. *
Kapteyn's Star Kapteyn's Star is a class M1 red subdwarf about 12.83 light-years from Earth in the southern constellation Pictor; it is the closest halo star to the Solar System. With a magnitude of nearly 9 it is visible through binoculars or a teles ...
, a
subdwarf A subdwarf, sometimes denoted by "sd", is a star with luminosity class VI under the Yerkes spectral classification system. They are defined as stars with luminosity 1.5 to 2 magnitudes lower than that of main-sequence stars of the same spectral ...
, was discovered in 1897 by
Jacobus Kapteyn Prof Jacobus Cornelius Kapteyn FRS FRSE LLD (19 January 1851 – 18 June 1922) was a Dutch astronomer. He carried out extensive studies of the Milky Way and was the discoverer of evidence for galactic rotation. Kapteyn was also among the fi ...
, the star with the highest known
proper motion Proper motion is the astrometric measure of the observed changes in the apparent places of stars or other celestial objects in the sky, as seen from the center of mass of the Solar System, compared to the abstract background of the more dista ...
at the time of its discovery and is a halo star. *
Kepler's Star SN 1604, also known as Kepler's Supernova, Kepler's Nova or Kepler's Star, was a Type Ia supernova that occurred in the Milky Way, in the constellation Ophiuchus. Appearing in 1604, it is the most recent supernova in the Milky Way galaxy to have ...
, name given to the
supernova A supernova is a powerful and luminous explosion of a star. It has the plural form supernovae or supernovas, and is abbreviated SN or SNe. This transient astronomical event occurs during the last evolutionary stages of a massive star or when ...
later designated
SN 1604 SN 1604, also known as Kepler's Supernova, Kepler's Nova or Kepler's Star, was a Type Ia supernova that occurred in the Milky Way, in the constellation Ophiuchus. Appearing in 1604, it is the most recent supernova in the Milky Way galaxy to hav ...
when first observed, after
Johannes Kepler Johannes Kepler (; ; 27 December 1571 – 15 November 1630) was a German astronomer, mathematician, astrologer, natural philosopher and writer on music. He is a key figure in the 17th-century Scientific Revolution, best known for his laws ...
, who studied it extensively though he did not have priority of discovery. *Klemola's Star is BD +10°2179 (SAO 99230) in Leo. * Koiki, a star within the
Southern Cross Crux () is a constellation of the southern sky that is centred on four bright stars in a cross-shaped asterism commonly known as the Southern Cross. It lies on the southern end of the Milky Way's visible band. The name ''Crux'' is Latin for c ...
constellation, named after
Indigenous Australian land rights Indigenous land rights in Australia, also known as Aboriginal land rights in Australia, relate to the rights and interests in land of Aboriginal Australians, Aboriginal and Torres Strait Islander people in Australia, and the term may also includ ...
campaigner Eddie Koiki Mabo on 3 June 2015, the 23rd anniversary of the
Mabo decision ''Mabo v Queensland (No 2)'' (commonly known as ''Mabo'') is a decision of the High Court of Australia, decided on 3 June 1992.. It is a landmark case, brought by Eddie Mabo against the State of Queensland. The case is notable for first reco ...
, which overturned the notion of
terra nullius ''Terra nullius'' (, plural ''terrae nullius'') is a Latin expression meaning " nobody's land". It was a principle sometimes used in international law to justify claims that territory may be acquired by a state's occupation of it. : : ...
in Australia. It was named by
Museum of Applied Arts and Sciences The Powerhouse Museum is the major branch of the Museum of Applied Arts & Sciences (MAAS) in Sydney, the others being the historic Sydney Observatory at Observatory Hill, and the newer Museums Discovery Centre at Castle Hill. Although often des ...
in
Sydney Sydney ( ) is the capital city of the state of New South Wales, and the most populous city in both Australia and Oceania. Located on Australia's east coast, the metropolis surrounds Sydney Harbour and extends about towards the Blue Mountain ...
. The star also falls within the larger
Torres Strait Islanders Torres Strait Islanders () are the Indigenous Melanesian people of the Torres Strait Islands, which are part of the state of Queensland, Australia. Ethnically distinct from the Aboriginal people of the rest of Australia, they are often grouped ...
' constellation known as Tagai, which is very culturally significant and used for
nautical navigation Navigation is a field of study that focuses on the process of monitoring and controlling the movement of a craft or vehicle from one place to another.Bowditch, 2003:799. The field of navigation includes four general categories: land navigation, ...
. * Krzeminski's Star is a blue
supergiant Supergiants are among the most massive and most luminous stars. Supergiant stars occupy the top region of the Hertzsprung–Russell diagram with absolute visual magnitudes between about −3 and −8. The temperature range of supergiant stars spa ...
, part of the
pulsar A pulsar (from ''pulsating radio source'') is a highly magnetized rotating neutron star that emits beams of electromagnetic radiation out of its magnetic poles. This radiation can be observed only when a beam of emission is pointing toward Ea ...
Centaurus X-3 Centaurus X-3 (4U 1118-60) is an X-ray pulsar with a period of 4.84 seconds. It was the first X-ray pulsar to be discovered, and the third X-ray source to be discovered in the constellation Centaurus. The system consists of a neutron star ...
, discovered by the Polish astronomer Wojciech Krzemiński in 1974. *Kurtz's Light Variable Star is HD 188136 in
Octans Octans () is a faint constellation located in the deep Southern Sky. Its name is Latin for the eighth part of a circle, but it is named after the octant, a navigational instrument. Devised by French astronomer Nicolas Louis de Lacaille in 1752, ...
. *Kuwano's Object/Star has been used to refer to the nova-like object PU Vulpeculae. The names "Kuwano's Object" and "Kuwano's Star" have also been used to refer to V1407 Aquilae and V4021 Sagittarii, respectively. These are all named after . *Lamont's Star is a peculiar star near the nucleus of the
Andromeda Galaxy The Andromeda Galaxy (IPA: ), also known as Messier 31, M31, or NGC 224 and originally the Andromeda Nebula, is a barred spiral galaxy with the diameter of about approximately from Earth and the nearest large galaxy to the Milky Way. The gala ...
(Messier 31). *Latham's planet is the small red dwarf star or massive brown dwarf
HD 114762 b HD 114762 b is a small red dwarf star, in the HD 114762 system, formerly thought to be a gas giant, massive gaseous exoplanet, extrasolar planet, approximately away in the constellation of Coma Berenices. This optically undetected compani ...
in
Coma Berenices Coma Berenices is an ancient asterism in the northern sky, which has been defined as one of the 88 modern constellations. It is in the direction of the fourth galactic quadrant, between Leo and Boötes, and it is visible in both hemisphere ...
, unofficially named ''Latham's planet'' after its discoverer David Latham (1989). *Liller's Star is a star near
Centaurus X-3 Centaurus X-3 (4U 1118-60) is an X-ray pulsar with a period of 4.84 seconds. It was the first X-ray pulsar to be discovered, and the third X-ray source to be discovered in the constellation Centaurus. The system consists of a neutron star ...
. Named after
William Liller William Liller (April 1, 1927, Philadelphia – February 28, 2021) was an American astronomer, known for his research on "planetary nebulae, comets, asteroids, magnetic activity in cool stars, the optical identification of X-ray sources, and astr ...
. *Lovas's Supernova is SN 1964e in MCG 9-20-51 (in
Ursa Major Ursa Major (; also known as the Great Bear) is a constellation in the northern sky, whose associated mythology likely dates back into prehistory. Its Latin name means "greater (or larger) bear," referring to and contrasting it with nearby Ursa ...
). Named after
Miklós Lovas This is a list of minor-planet discoverers credited by the Minor Planet Center with the discovery of one or several minor planets (such as near-Earth and main-belt asteroids, Jupiter trojans and distant objects). , the discovery of 612,011 nu ...
. *
Luyten's Star Luyten's Star (GJ 273) is a red dwarf in the constellation Canis Minor located at a distance of approximately from the Sun. It has a visual magnitude of 9.9, making it too faint to be viewed with the unaided eye. It is named after ...
, another red dwarf, is named after
Willem Jacob Luyten Willem Jacob Luyten (March 7, 1899 – November 21, 1994) was a Dutch-American astronomer. "Willem Jacob Luyten", ''Marquis Who's Who'', 2006. Life Jacob Luyten was born in Semarang, Java, at the time part of the Dutch East Indies. His ...
, its discoverer. *Luyten's Flare Star is a nearby UV Ceti variable (L 726-8). *Merrill's Star is the high-velocity
Wolf–Rayet star Wolf–Rayet stars, often abbreviated as WR stars, are a rare heterogeneous set of stars with unusual spectra showing prominent broad emission lines of ionised helium and highly ionised nitrogen or carbon. The spectra indicate very high surface ...
WR 124 WR 124 is a Wolf–Rayet star in the constellation of Sagitta surrounded by a ring nebula of expelled material known as M1-67. It is one of the fastest runaway stars in the Milky Way with a radial velocity around . It was discovered by Pau ...
, at the nucleus of the ejecta nebula PK 50+3 1 in
Sagitta Sagitta is a dim but distinctive constellation in the northern sky. Its name is Latin for 'arrow', not to be confused with the significantly larger constellation Sagittarius 'the archer'. It was included among the 48 constellations listed by t ...
(which it created). Named after
Paul W. Merrill Paul Willard Merrill (August 15, 1887 – July 19, 1961) was an American astronomer whose specialty was spectroscopy. He was the first to define S-type stars in 1922. Career He received his Ph.D. at the University of California (now UC Berkeley) ...
. *Olbers' Star is a peculiar star in Virgo (mentioned in the Deep-Sky Name Index 2000.0 by Hugh C. Maddocks) (Foxon-Maddocks Associates). Named after
Heinrich Wilhelm Matthias Olbers Heinrich Wilhelm Matthias Olbers (; ; 11 October 1758 – 2 March 1840) was a German physician and astronomer. Life and career Olbers was born in Arbergen, Germany, today part of Bremen, and studied to be a physician at Göttingen (1777–80) ...
. *Osawa's Star is V436 Cassiopeiae (HD 221568). Named after Kiwoteru Osawa. *Pearce's Star is
AO Cassiopeiae AO Cassiopeiae, also known as Pearce's Star, is a binary system composed of an O8 main sequence star and an O9.2 bright giant that respectively weigh anywhere between 20.30 and 57.75 times and 14.8 and 31.73 times the mass of the Sun. T ...
. Named after
Joseph Algernon Pearce Joseph Algernon Pearce (February 7, 1893 – September 8, 1988) was a Canadians, Canadian astrophysicist, who was notable for studies on the structure of Milky Way and O-type stars. Born in Brantford, Ontario, Brantford, Ontario, Pearce enlis ...
. *Persson's Star is V733 Cephei, an FU Orionis type object. Named after R. Persson. *Piazzi's Flying Star, see Bessel's Star. * Plaskett's Star (also designated HR 2422) is one of the most massive
binary stars A binary star is a system of two stars that are gravitationally bound to and in orbit around each other. Binary stars in the night sky that are seen as a single object to the naked eye are often resolved using a telescope as separate stars, in wh ...
known, with a total mass of about one hundred times that of the
Sun The Sun is the star at the center of the Solar System. It is a nearly perfect ball of hot plasma, heated to incandescence by nuclear fusion reactions in its core. The Sun radiates this energy mainly as light, ultraviolet, and infrared radi ...
. It is named after
John Stanley Plaskett John Stanley Plaskett (November 17, 1865 – October 17, 1941) was a Canadian astronomer. Career He worked as a machinist, and was offered a job as a mechanician at the Department of Physics at the University of Toronto, constructing appar ...
, the Canadian astronomer who discovered its binary nature in 1922. *Popper's Star is HD 124448, an
extreme helium star An extreme helium star (abbreviated EHe) is a low-mass supergiant that is almost devoid of hydrogen, the most common chemical element of the Universe. Since there are no known conditions where stars devoid of hydrogen can be formed from molecular c ...
in
Centaurus Centaurus is a bright constellation in the southern sky. One of the 88 modern constellations by area, largest constellations, Centaurus was included among the 48 constellations listed by the 2nd-century astronomer Ptolemy, and it remains one o ...
. Named after Daniel M. Popper. * Przybylski's Star (also designated HD 101065) is a star that shows unusually high abundance of
lanthanide The lanthanide () or lanthanoid () series of chemical elements comprises the 15 metallic chemical elements with atomic numbers 57–71, from lanthanum through lutetium. These elements, along with the chemically similar elements scandium and yttr ...
elements in its spectral lines, named for
Antoni Przybylski Antoni Przybylski (1913 — September 21, 1985),Przybylski, Antoni
...
. *Ptolemy's Cluster is the open star cluster
Messier 7 Messier 7 or M7, also designated NGC 6475 and sometimes known as the Ptolemy Cluster, is an open cluster of stars in the constellation of Scorpius. The cluster is easily detectable with the naked eye, close to the "stinger" of Scorpius. With a d ...
(NGC 6475) in
Scorpius Scorpius is a zodiac constellation located in the Southern celestial hemisphere, where it sits near the center of the Milky Way, between Libra to the west and Sagittarius to the east. Scorpius is an ancient constellation that pre-dates the Gre ...
. Named after
Ptolemy Claudius Ptolemy (; grc-gre, Πτολεμαῖος, ; la, Claudius Ptolemaeus; AD) was a mathematician, astronomer, astrologer, geographer, and music theorist, who wrote about a dozen scientific treatises, three of which were of importanc ...
. *The Roberts–Altizer Variable Star is a galactic
U Geminorum star A U Geminorum-type variable star, or dwarf nova (pl. novae) is one of several types of cataclysmic variable star, consisting of a close binary star system in which one of the components is a white dwarf that accretes matter from its companion. Dwa ...
near NGC 3147, in
Draco Draco is the Latin word for serpent or dragon. Draco or Drako may also refer to: People * Draco (lawgiver) (from Greek: Δράκων; 7th century BC), the first lawgiver of ancient Athens, Greece, from whom the term ''draconian'' is derived * D ...
. *Rosino's Supernova is a supernova that was discovered by in 1965, near NGC 4753. *The Rosino–Zwicky Object (Star) is a variable star near
Messier 88 Messier 88 (also known as M88 or NGC 4501) is a spiral galaxy about 50 to 60 million light-years away from Earth in the constellation Coma Berenices. It was discovered by Charles Messier in 1781. Properties M88 is one of the fifteen Messier ob ...
in Coma Berenices. Named after Rosino and
Fritz Zwicky Fritz Zwicky (; ; February 14, 1898 – February 8, 1974) was a Swiss astronomer. He worked most of his life at the California Institute of Technology in the United States of America, where he made many important contributions in theoretical and ...
. *
Sakurai's Object Sakurai's Object (V4334 Sagittarii) is a star in the constellation of Sagittarius. It is thought to have previously been a white dwarf that, as a result of a very late thermal pulse, swelled and became a red giant. It is located at th ...
(also designated V4334 Sgr) is an unusual red giant, named after . *Sanduleak's Star is a possible
symbiotic star A symbiotic binary is a type of binary star system, often simply called a symbiotic star. They usually contain a white dwarf with a companion red giant. The cool giant star loses material via Roche lobe overflow or through its stellar wind, whic ...
in the
Large Magellanic Cloud The Large Magellanic Cloud (LMC), or Nubecula Major, is a satellite galaxy of the Milky Way. At a distance of around 50 kiloparsecs (≈160,000  light-years), the LMC is the second- or third-closest galaxy to the Milky Way, after the ...
(LMC). Named after Nicholas Sanduleak. *The Sanduleak–Pesch Binary Star is a
white dwarf A white dwarf is a stellar core remnant composed mostly of electron-degenerate matter. A white dwarf is very dense: its mass is comparable to the Sun's, while its volume is comparable to the Earth's. A white dwarf's faint luminosity comes fro ...
binary in
Hercules Hercules (, ) is the Roman equivalent of the Greek divine hero Heracles, son of Jupiter and the mortal Alcmena. In classical mythology, Hercules is famous for his strength and for his numerous far-ranging adventures. The Romans adapted the Gr ...
. Named after Sanduleak and
Peter Pesch Peter may refer to: People * List of people named Peter, a list of people and fictional characters with the given name * Peter (given name) ** Saint Peter (died 60s), apostle of Jesus, leader of the early Christian Church * Peter (surname) Peter ...
. *The Sanduleak–Stephenson Star/Object is also known as Sanduleak-Stephenson 433,
SS 433 SS 433 is one of the most exotic star systems observed. It is located in the Milky Way galaxy, and is an eclipsing X-ray binary system, with the primary being a stellar-mass black hole. The spectrum of the secondary companion star sugg ...
in Aquila, a
neutron star A neutron star is the collapsed core of a massive supergiant star, which had a total mass of between 10 and 25 solar masses, possibly more if the star was especially metal-rich. Except for black holes and some hypothetical objects (e.g. white ...
in radio source W50. Named after Sanduleak and
Charles Bruce Stephenson Charles Bruce Stephenson (February 9, 1929 – December 3, 2001) was an American astronomer. He was born on a ranch in Little Rock, Arkansas, the only son of Chauncey Elvira Stephenson and Ona Richards. During his youth he made a telescope and w ...
. *Schaeberle's Flaming Star is the source of the Flaming Star Nebula IC 405 (aka Cederblad 42) in Auriga,
AE Aurigae AE Aurigae (abbreviated as AE Aur) is a runaway star in the constellation Auriga; it lights the Flaming Star Nebula. Description AE Aurigae is a blue O-type main sequence dwarf with a mean apparent magnitude of +6.0. It is classifie ...
. Named after
John Martin Schaeberle John Martin Schaeberle (January 10, 1853 – September 17, 1924) was a German-American astronomer. Biography He was born Johann Martin Schäberle in Württemberg, Germany, but in 1854 immigrated as an infant to the United States. Most sources r ...
. *Scheiner's Star is BD +15°2083 (HD 83225) in Leo. Named after
Julius Scheiner Julius Scheiner (25 November 1858 – 20 December 1913) was a German astronomer, born in Cologne and educated at Bonn. He became assistant at the astrophysical observatory in Potsdam in 1887 and its observer in chief in 1898, three years after h ...
. *
Sidus Ludoviciana Sidus Ludoviciana , also known as HD 116798 is an 8th-magnitude giant star in the asterism of the Big Dipper in the constellation Ursa Major, halfway between Mizar and Alcor. It was discovered on 2 December 1722 by Johann Georg Liebkn ...
, an 8th-magnitude star in the asterism of the
Big Dipper The Big Dipper ( US, Canada) or the Plough ( UK, Ireland) is a large asterism consisting of seven bright stars of the constellation Ursa Major; six of them are of second magnitude and one, Megrez (δ), of third magnitude. Four define a "bowl" ...
in the constellation
Ursa Major Ursa Major (; also known as the Great Bear) is a constellation in the northern sky, whose associated mythology likely dates back into prehistory. Its Latin name means "greater (or larger) bear," referring to and contrasting it with nearby Ursa ...
, halfway between
Mizar and Alcor Mizar and Alcor are two stars forming a naked eye double in the handle of the Big Dipper (or Plough) asterism in the constellation of Ursa Major. Mizar is the second star from the end of the Big Dipper's handle, and Alcor its fainter companion. ...
. It was discovered on 2 December 1722 by Johann Georg Liebknecht, who mistook it for a planet and named it after
Louis V, Landgrave of Hesse-Darmstadt Louis may refer to: * Louis (coin) * Louis (given name), origin and several individuals with this name * Louis (surname) * Louis (singer), Serbian singer * HMS ''Louis'', two ships of the Royal Navy See also Derived or associated terms * Lewis (d ...
. *
Scholz's star Scholz's Star ( WISE designation WISE 0720−0846 or fully WISE J072003.20−084651.2) is a dim binary stellar system from the Sun in the constellation Monoceros near the galactic plane. It was discovered in 2013 by astronomer Ralf- ...
is a late-M dwarf + T-type
brown dwarf Brown dwarfs (also called failed stars) are substellar objects that are not massive enough to sustain nuclear fusion of ordinary hydrogen ( 1H) into helium in their cores, unlike a main-sequence star. Instead, they have a mass between the most ...
(M9.5 + T5) system, discovered in 2013 by Ralf-Dieter Scholz. It has large parallax, but relatively small proper motion, and it is known for its close flyby to the Sun about 70,000 years ago. *The Schweizer–Middleditch Star is a star near the center of SN 1006 in Centaurus. Named after Francois Schweizer and
John Middleditch John is a common English name and surname: * John (given name) * John (surname) John may also refer to: New Testament Works * Gospel of John, a title often shortened to John * First Epistle of John, often shortened to 1 John * Second ...
. *
Sneden's Star BPS CS22892-0052 (Sneden's Star) is an old population II star located at a distance of 4.7 kpc in the galactic halo. It belongs to a class of ultra- metal-poor stars ( Metallicity e/H-3.1), specifically the very rare subclass of neut ...
is a giant star, named after Chris Sneden. The star is known for its high-resolution spectroscopic observations. *
SN Refsdal SN Refsdal is the first detected multiply-lensed supernova, visible within the field of the galaxy cluster MACS J1149+2223. It was given its nickname in honor of the Norwegian astrophysicist Sjur Refsdal, who, in 1964, first proposed using time ...
is the first detected multiply-lensed supernova. *Stepanian's Star is LX Serpentis, a 14th magnitude flare star (?). Named after
Jivan A. Stepanian Jivan may refer to: * Jivan Avetisyan, Armenian film director * Bhai Jivan Singh * Alin Jivan, Romanian artist gymnast * Kantilal Jivan * Bhanwarlal Jivan, Indian politician * Jag Jivan Ram, Indian politician * Jivan Gasparyan, Armenian musi ...
. *Sugano's Star is a variable star in Orion, either V369 or V1143 Orionis. *Tabby's Star, see Boyajian's Star. * Teegarden's star, a nearby star discovered in 2003 in archived data taken years earlier for
NASA The National Aeronautics and Space Administration (NASA ) is an independent agency of the US federal government responsible for the civil space program, aeronautics research, and space research. NASA was established in 1958, succeeding t ...
's
Near Earth Asteroid Tracking Near-Earth Asteroid Tracking (NEAT) was a program run by NASA and the Jet Propulsion Laboratory, surveying the sky for near-Earth objects. NEAT was conducted from December 1995 until April 2007, at GEODSS on Hawaii (Haleakala-NEAT; 566), as wel ...
program. The star is named in honor of
Bonnard J. Teegarden Bonnard John Teegarden (born August 23, 1940) is an American astrophysicist formerly with NASA's Goddard Space Flight Center, now retired. He spent most of his career studying cosmic gamma ray A gamma ray, also known as gamma radiation (sy ...
, the
NASA The National Aeronautics and Space Administration (NASA ) is an independent agency of the US federal government responsible for the civil space program, aeronautics research, and space research. NASA was established in 1958, succeeding t ...
astrophysicist that led the discovery team. *Tombaugh's Star is
TV Corvi TV Corvi, also known as Tombaugh's Star, is a dwarf nova of the SU Ursae Majoris type in the constellation Corvus that was first discovered by accident as a mysterious 12th magnitude star on a plate by Clyde Tombaugh while looking for r ...
. Named after
Clyde Tombaugh Clyde William Tombaugh (February 4, 1906 January 17, 1997) was an American astronomer. He discovered Pluto in 1930, the first object to be discovered in what would later be identified as the Kuiper belt. At the time of discovery, Pluto was cons ...
. *Tycho's Star, name given to the
supernova A supernova is a powerful and luminous explosion of a star. It has the plural form supernovae or supernovas, and is abbreviated SN or SNe. This transient astronomical event occurs during the last evolutionary stages of a massive star or when ...
later designated
SN 1572 SN 1572 ('' Tycho's Supernova'', ''Tycho's Nova''), or B Cassiopeiae (B Cas), was a supernova of Type Ia in the constellation Cassiopeia, one of eight supernovae visible to the naked eye in historical records. It appeared in early November 1572 ...
, after
Tycho Brahe Tycho Brahe ( ; born Tyge Ottesen Brahe; generally called Tycho (14 December 154624 October 1601) was a Danish astronomer, known for his comprehensive astronomical observations, generally considered to be the most accurate of his time. He was k ...
, though he did not have priority of discovery. *Van Biesbroeck's Star is
VB 10 VB 10 or Van Biesbroeck's star is a very small and very dim red dwarf located in the constellation Aquila. It is part of a binary star system. VB 10 is historically notable as it was the coolest, least massive and least luminous k ...
, a very small, faint,
red dwarf ''Red Dwarf'' is a British science fiction comedy franchise created by Rob Grant and Doug Naylor, which primarily consists of a television sitcom that aired on BBC Two between 1988 and 1999, and on Dave since 2009, gaining a cult following. T ...
named after
George Van Biesbroeck George A. Van Biesbroeck (or Georges-Achille Van Biesbroeck, , January 21, 1880 – February 23, 1974) was a Belgian–American astronomer. He worked at observatories in Belgium, Germany and the United States. He specialized in the observation o ...
, who discovered it in 1944 – the smallest and faintest star then known. *
Van Maanen's Star Van Maanen 2, or van Maanen's Star, is the closest known solitary white dwarf to the solar system. It is a dense, compact stellar remnant no longer generating energy and has equivalent to about 68% of the Sun's mass but only 1% of its r ...
is a
white dwarf A white dwarf is a stellar core remnant composed mostly of electron-degenerate matter. A white dwarf is very dense: its mass is comparable to the Sun's, while its volume is comparable to the Earth's. A white dwarf's faint luminosity comes fro ...
, discovered in 1917 by
Adriaan van Maanen Adriaan van Maanen (March 31, 1884 – January 26, 1946) was a Dutch–American astronomer. Van Maanen, born into a well-to-do family in Friesland, studied astronomy at the University of Utrecht (earning his Ph.D. in 1911) and worked briefl ...
, only the second white dwarf discovered. *Wachmann's Flare Star is V371 Orionis. Named after
Arno Arthur Wachmann Arno Arthur Wachmann (8 March 1902 – 24 July 1990) was a German astronomer and discoverer of comets and minor planets, who worked for many years at the Bergedorf Observatory in Hamburg.BAT99-6 in the Large Magellanic Cloud (LMC) in
Dorado Dorado () is a constellation in the southern sky. It was named in the late 16th century and is now one of the 88 modern constellations. Its name refers to the dolphinfish (''Coryphaena hippurus''), which is known as ''dorado'' in Spanish, altho ...
. Named after Nolan R. Walborn. It was found to be a binary between a slash star and an O-type main sequence star. *Warren and Penfold's (WP) Star is the optical counterpart of X-3 in the Large Magellanic Cloud. Named after P. R. Warren and J. E. Penfold. *Wild's Supernova is SN 1966j in NGC 3198 (in Ursa Major). Named after Paul Wild. *Wischnjewsky's Supernova in Fornax A. Named after Marina Wischnjewsky. *The Zealey–Lee Supernova in the nucleus of an anonymous galaxy in Grus. Named after W. Zealey and S. Lee. (Note that '' Pandora's Star'' and ''
Ratner's Star ''Ratner's Star'' is a 1976 novel by Don DeLillo. It relates the story of a child prodigy mathematician who arrives at a secret installation to work on the problem of deciphering a mysterious message that appears to come from outer space. The no ...
'' are the names of novels, not actual stars.)


Covertly named stars

Some stars were given names that were disguised names of individuals, which names subsequently appeared in star catalogues and thus into more general usage. The earliest noted example was
Sualocin and Rotanev Alpha Delphini (α Delphini, abbreviated Alpha Del, α Del) is a multiple star system in the constellation of Delphinus. It consists of a triple star, designated Alpha Delphini A, together with five faint, probably optical compani ...
, which names have now been approved by the IAU WGSN (see above). More recently, during the Apollo program, it was common for astronauts to be trained in
celestial navigation Celestial navigation, also known as astronavigation, is the practice of position fixing using stars and other celestial bodies that enables a navigator to accurately determine their actual current physical position in space (or on the surface of ...
, and to use a list of
naked-eye Naked eye, also called bare eye or unaided eye, is the practice of engaging in visual perception unaided by a magnifying, light-collecting optical instrument, such as a telescope or microscope, or eye protection. Vision corrected to normal ...
stars which to take bearings. As a practical joke,
Gus Grissom Virgil Ivan "Gus" Grissom (April 3, 1926 – January 27, 1967) was an American engineer, pilot in the United States Air Force, and member of the Mercury Seven selected by National Aeronautics and Space Administration's (NASA) as Project Mercur ...
gave names to three stars on this list, which were references to the three
Apollo 1 Apollo 1, initially designated AS-204, was intended to be the first crewed mission of the Apollo program, the American undertaking to land the first man on the Moon. It was planned to launch on February 21, 1967, as the first low Earth orbita ...
crew: *Navi for the star
Gamma Cassiopeiae Gamma Cassiopeiae, Latinized from γ Cassiopeiae, is a bright star at the center of the distinctive "W" asterism in the northern circumpolar constellation of Cassiopeia. Although it is a fairly bright star with an apparent visual mag ...
and which is ''Ivan'' spelled backwards, the middle name of Virgil ''Ivan'' "Gus" Grissom. *Dnoces for the star
Iota Ursae Majoris Iota Ursae Majoris (ι Ursae Majoris, abbreviated Iota UMa, ι UMa), also named Talitha , is a star system in the northern circumpolar constellation of Ursa Major. It has an apparent visual magnitude of 3.14, making it v ...
and which is ''Second'' spelled backwards, alluding to Edward Higgins White, ''II''. *Regor for the star
Gamma Velorum Gamma Velorum is a quadruple star system in the constellation Vela. This name is the Bayer designation for the star, which is Latinised from γ Velorum and abbreviated γ Vel. At a combined magnitude of +1.7, it is one of t ...
and which is ''Roger'' spelled backwards, the first name of ''Roger'' Bruce Chaffee. The names stuck, perhaps '' in memoriam'' for their deaths in the Apollo 1 fire, and were used through the rest of the program. Unknown to Grissom, these stars already had traditional names; however, those were not generally used, allowing the three new names to make their way into other records. Today, they are generally considered disused—some sources listing them as "traditional". It is possible, though unlikely, that further traditional names are in fact hidden names such as these, not yet identified;
etymologies Etymology ()The New Oxford Dictionary of English (1998) – p. 633 "Etymology /ˌɛtɪˈmɒlədʒi/ the study of the class in words and the way their meanings have changed throughout time". is the study of the history of the form of words and ...
for many star names are not currently known.


Commercial naming

As early as 1979, when the
International Star Registry The International Star Registry (ISR) is an organization founded in 1979, which sells the right to unofficially name stars. Overview The company sells the right to unofficially name a star, often as a gift or memorial. These names are recorded i ...
was formed, private companies have attempted to sell the right to unofficially name stars. These companies have no legal standing to assign any star a name, and as such these names are never recognized by the astronomical or scientific communities. The IAU does not recognize this practice, and on its website describes it as " charlatanry".


See also

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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. It operates under Division C – Education ...
*
List of astronomical objects named after people This is a list of astronomical objects named after people. While topological features on Solar System bodies — such as craters, mountains, and valleys — are often named after famous or historical individuals, many stars and deep-sky objects a ...
*
List of minor planets named after people This is a list of minor planets named after people, both real and fictional. Science Astronomers Amateur *340 Eduarda (Heinrich Eduard von Lade, German) * 792 Metcalfia (Joel Hastings Metcalf, American) *828 Lindemannia (Adolph Friedrich Lindem ...
*
List of people with craters of the Moon named after them The following is a list of people whose names were given to craters of the Moon. The list of approved names in the ''Gazetteer of Planetary Nomenclature'' maintained by the International Astronomical Union includes the person the crater is named ...
*
NameExoWorlds NameExoWorlds (also known as IAU NameExoWorlds) is the name of various projects managed by the International Astronomical Union (I.A.U.) to encourage names to be submitted for astronomical objects, which would later be considered for official ad ...
*
Stellar designations and names In astronomy, stars have a variety of different stellar designations and names, including catalogue designations, current and historical proper names, and foreign language names. Only a tiny minority of known stars have proper names; all others ha ...


References

{{DEFAULTSORT:Stars Named After People Lists of stars Lists of things named after people Astronomical nomenclature S