List of adjectivals and demonyms of astronomical bodies

Last updated

The adjectival forms of the names of astronomical bodies are not always easily predictable. Attested adjectival forms of the larger bodies are listed below, along with the two small Martian moons; in some cases they are accompanied by their demonymic equivalents, which denote hypothetical inhabitants of these bodies.

Contents

For Classical (Greco-Roman) names, the adjectival and demonym forms normally derive from the oblique stem, which may differ from the nominative form used in English for the noun form. For instance, for a large portion of names ending in -s, the oblique stem and therefore the English adjective changes the -s to a -d, -t, or -r, as in Mars–Martian, Pallas–Palladian and Ceres–Cererian; [note 1] occasionally an -n has been lost historically from the nominative form, and reappears in the oblique and therefore in the English adjective, as in Pluto–Plutonian and Atlas–Atlantean.

Many of the more recent or more obscure names are only attested in mythological or literary contexts, rather than in specifically astronomical contexts. Forms ending in -ish or -ine, such as "Puckish", are not included below if a derivation in -an is also attested. Rare forms, or forms only attested with spellings not in keeping with the IAU-approved spelling (such as c for k), are shown in italics.

Note on pronunciation

The suffix -ian is always unstressed: that is, /iən/ . The related ending -ean, from an e in the root plus a suffix -an, has traditionally been stressed (that is, /ˈən/ ) if the e is long ē in Latin (or is from ηē in Greek); but if the e is short in Latin, the suffix is pronounced the same as -ian. In practice forms ending in -ean may be pronounced as if they were spelled -ian even if the e is long in Latin. This dichotomy should be familiar from the dual pronunciations of Caribbean as /ˌkærɪˈbən/ KARR-ə-BEE-ən and /kəˈrɪbiən/ kə-RIB-i-ən.

Generic bodies

NameAdjective Demonym
asteroid asteroidal, asteroidicAsterite
comet cometary
cosmos, universe cosmic, cosmian, universal
ecliptic ecliptical, zodiacal
galaxy galactic, galactian
meteoroid meteoroidal
nebula nebular
planet planetary, planetic
planetoid planetoidal
quasar quasaric, quasarian
sky celestial
star astral, sidereal, siderean, stellar
supernova supernovan

Constellations

Derivative forms of constellations are used primarily for meteor showers. The genitive forms of the constellations are used to name stars. (See List of constellations.) Other adjectival forms are less common.

NameAdjectiveDerivative
Andromeda AndromedanAndromedid
Aquarius AquarianAquariid
Aries ArianArietid
Auriga AurigalAurigid
Bootes Bootid
Cancer CancerianCancrid
Carina CarinalCarinid
Capricorn CapricornianCapricornid
Centaurus Centaurean, CentaurianCentaurid
Cetus Cetid
Coma Berenices ComalComa Berenicid
Corona Austrina CoronalCorona Austrinid
Crux CrucialCrucid
Cygnus CygneanCygnid
Dorado Doradid
Draco DraconicDraconid
Eridanus Eridanid
Gemini GeminianGeminid
Hydra, Hydrus Hydrid
Leo Leonic, Leonian, LeoneanLeonid
Leo Minor Leo Minorid
Libra LibranLibrid
Lyra Lyrid
Monoceros Monocerotid
Norma Normid
Ophiuchus Ophiuchid
Orion Orionid
Pavo Pavonid
Pegasus Pegasean, PegasarianPegasid
Perseus Perseid
Phoenix PhoeniceanPhoenicid
Pisces Piscean, PiscianPiscid
Piscis Austrinus Piscis Austrinid
Puppis Puppid
Sagittarius SagittarianSagittariid
Scorpius Scorpian, ScorpionicScorpiid
Taurus Taurean, TaurianTaurid
Ursa Major, Ursa Minor UrsalUrsid
Vela Velar, VelicVelid
Virgo Virginal, VirginianVirginid
zodiac zodiacal

Sun

NameAdjective Demonym
Sun, Sol, Helios Solar, Heliacal, Phoebean, PhebeanSolarian

Planets

Planets and planetoids
NameAdjective Demonym
Ceres Cererian, [1] Cererean [2] Cererian
Earth, Terra, Tellus, Gaia, Gaea earthly, Terran, Terrestrial, Terrene, Tellurian, [3] Telluric, Gaian, GaeanEarthling, Terran, Terrestrial, Tellurian, Earthian, Earther, Earthican
Eris Eridian [4]
Haumea Haumean [5]
Jupiter Jovian, Jupiterian, ZeusianJovian
Makemake Makemakean [6]
Mars Martian, Martial, Arean [7] Martian
Mercury;
Hermes (in the evening),
Apollo (in the morning)
Mercurian, Mercurial, Hermean/Hermeian, Cyllenian, [8] CylleneanMercurian, Hermean
Neptune Neptunian, Neptunial, Poseidean [9] Neptunian
Orcus Orcean, [10] Orcan
Pallas Palladian
Pluto Plutonic, PlutonianPlutonian
Saturn Saturnian, Saturnine, Cronian, [9] Kronian, [11] Saturnial [12] Saturnian
Sedna Sednian [13]
Uranus Uranian, CaelianUranian
Vesta Vestian, [14] [15] Vestan, [16] [17] VestalianVestan, Vestian
Venus;
Hesperus , Vesper (in the evening),
Eosphorus, Phosphorus, Phosphor (in the morning),
Lucifer (in the day)
Venerian, Venusian, Cytherean, [18] Cytherian, [19] Hesperian, [20] Luciferian, [21] Phosphorian, [22] Aphroditan [23] Venusian, Cytherean

Moons

Earth and Mars
NameAdjective Demonym
Moon (Luna, Selene)Lunar, Selenian, CynthianLunarian, Selenite
Deimos Deimian [24]
Phobos Phobian [25]
Jupiter
NameAdjective, demonym
Callisto Callistoan, [26] Callistonian [27]
Europa Europan [28]
Ganymede Ganymedean, [29] Ganymedian
Io Ionian [30]
Saturn
NameAdjective, demonym
Dione Dionean [31] [32]
Enceladus Enceladean, [33] [34] Enceladan [35] [36]
Hyperion Hyperionian [37]
Iapetus Iapetian, [38] Japetian
Mimas Mimantean, [34] Mimantian, [39]
Rhea Rhean [40] [41]
Tethys Tethyan [42] [43]
Titan Titanian /tˈtniən/ , [44] Titanean [45]
Uranus
NameAdjective, demonym
Ariel Arielian [46]
Miranda Mirandan, [47] Mirandian [48]
Oberon Oberonian [49]
Titania Titanian /tɪˈtɑːniən/ [50]
Umbriel Umbrielian [50]
Neptune, Pluto and Eris
NameAdjective, demonym
Triton Tritonian [51]
Charon Charonian [52]
Dysnomia Dysnomian

Galaxies

NameAdjective
Milky Way Galaxy Galactic, [53] Lacteal [54]
Andromeda Galaxy Andromedan
Magellanic Clouds Magellanic

See also

Notes

  1. This is reflected in Russian Паллада Pallada 'Pallas' and Церера Tserera 'Ceres', as well as in Italian Pallade 'Pallas' and Cerere 'Ceres', as in these (and several other) languages the nominal forms of the names often also reflect the oblique. This is not always the case, however – for Mars, Italian Marte parallels the English adjective but Russian Марс Mars parallels the English noun.

Related Research Articles

<span class="mw-page-title-main">Ecliptic</span> Apparent path of the Sun on the celestial sphere

The ecliptic or ecliptic plane is the orbital plane of Earth around the Sun. From the perspective of an observer on Earth, the Sun's movement around the celestial sphere over the course of a year traces out a path along the ecliptic against the background of stars. The ecliptic is an important reference plane and is the basis of the ecliptic coordinate system.

<span class="mw-page-title-main">Jet Propulsion Laboratory</span> Research and development center and NASA field center in California, United States

Jet Propulsion Laboratory (JPL) is a Federally Funded Research and Development Center (FFRDC) in La Cañada Flintridge, California, Crescenta Valley, United States. Founded in 1936 by Caltech researchers, the laboratory is now owned and sponsored by the National Aeronautics and Space Administration (NASA) and administered and managed by the California Institute of Technology.

<span class="mw-page-title-main">4 Vesta</span> Second largest asteroid of the main asteroid belt

Vesta is one of the largest objects in the asteroid belt, with a mean diameter of 525 kilometres (326 mi). It was discovered by the German astronomer Heinrich Wilhelm Matthias Olbers on 29 March 1807 and is named after Vesta, the virgin goddess of home and hearth from Roman mythology.

<span class="mw-page-title-main">2 Pallas</span> Third-largest asteroid

Pallas is the third-largest asteroid in the Solar System by volume and mass. It is the second asteroid to have been discovered, after Ceres, and is likely a remnant protoplanet. Like Ceres, it is believed to have a mineral composition similar to carbonaceous chondrite meteorites, though significantly less hydrated than Ceres. It is 79% the mass of Vesta and 22% the mass of Ceres, constituting an estimated 7% of the mass of the asteroid belt. Its estimated volume is equivalent to a sphere 507 to 515 kilometers in diameter, 90–95% the volume of Vesta.

<span class="mw-page-title-main">Phobos (moon)</span> Larger of the two moons of Mars

Phobos is the innermost and larger of the two natural satellites of Mars, the other being Deimos. The two moons were discovered in 1877 by American astronomer Asaph Hall. Phobos is named after the Greek god of fear and panic, who is the son of Ares (Mars) and twin brother of Deimos.

<i>Cassini–Huygens</i> NASA/ESA mission sent to study Saturn and its moons (1997–2017)

Cassini–Huygens, commonly called Cassini, was a space-research mission by NASA, the European Space Agency (ESA), and the Italian Space Agency (ASI) to send a space probe to study the planet Saturn and its system, including its rings and natural satellites. The Flagship-class robotic spacecraft comprised both NASA's Cassini space probe and ESA's Huygens lander, which landed on Saturn's largest moon, Titan. Cassini was the fourth space probe to visit Saturn and the first to enter its orbit, where it stayed from 2004 to 2017. The two craft took their names from the astronomers Giovanni Cassini and Christiaan Huygens.

<span class="mw-page-title-main">Hyperion (moon)</span> Moon of Saturn

Hyperion, also known as Saturn VII, is the eighth-largest moon of Saturn. It is distinguished by its highly irregular shape, chaotic rotation, low density, and its unusual sponge-like appearance. It was the first non-rounded moon to be discovered.

<span class="mw-page-title-main">Mimas</span> Moon of Saturn

Mimas, also designated Saturn I, is the seventh-largest natural satellite of Saturn. With a mean diameter of 396.4 kilometres or 246.3 miles, Mimas is the smallest astronomical body known to be roughly rounded in shape due to its own gravity. Mimas's low density, 1.15 g/cm3, indicates that it is composed mostly of water ice with only a small amount of rock, and study of Mimas's motion suggests that it may have a liquid ocean beneath its surface ice. The surface of Mimas is heavily cratered and shows little signs of recent geological activity. A notable feature of Mimas's surface is Herschel, one of the largest craters relative to the size of the parent body in the Solar System. Herschel measures 139 kilometres across, about one-third of Mimas's mean diameter, and formed from an extremely energetic impact event. The crater's name is derived from the discoverer of Mimas, William Herschel, in 1789. The moon's presence has created one of the largest 'gaps' in Saturn's ring, named the Cassini Division, due to orbital resonance destabilising the particles' orbit there.

<span class="mw-page-title-main">Transit of Deimos from Mars</span> Transit of a Moon of Mars

A transit of Deimos across the Sun as seen from Mars occurs when Deimos passes directly between the Sun and a point on the surface of Mars, obscuring a small part of the Sun's disc for an observer on Mars. During a transit, Deimos can be seen from Mars as a small dark spot rapidly moving across the Sun's face.

<span class="mw-page-title-main">Pallene (moon)</span> Moon of Saturn

Pallene is a very small natural satellite of Saturn. It is one of three small moons known as the Alkyonides that lie between the orbits of the larger Mimas and Enceladus. It is also designated Saturn XXXIII.

<span class="mw-page-title-main">Moons of Mars</span> Natural satellites orbiting Mars

The two moons of Mars are Phobos and Deimos. They are irregular in shape. Both were discovered by American astronomer Asaph Hall in August 1877 and are named after the Greek mythological twin characters Phobos and Deimos who accompanied their father Ares into battle.

<span class="mw-page-title-main">Timekeeping on Mars</span> Proposed approaches to tracking date and time on the planet Mars

Though no standard exists, numerous calendars and other timekeeping approaches have been proposed for the planet Mars. The most commonly seen in the scientific literature denotes the time of year as the number of degrees on its orbit from the northward equinox, and increasingly there is use of numbering the Martian years beginning at the equinox that occurred April 11, 1955.

<span class="mw-page-title-main">Astronomy on Mars</span> Astronomical phenomena viewed from the planet Mars

Many astronomical phenomena viewed from the planet Mars are the same as or similar to those seen from Earth; but some are quite different. For example, because the atmosphere of Mars does not contain an ozone layer, it is also possible to make UV observations from the surface of Mars.

<span class="mw-page-title-main">Exploration of Saturn</span> Overview of the exploration of Saturn

The exploration of Saturn has been solely performed by crewless probes. Three missions were flybys, which formed an extended foundation of knowledge about the system. The Cassini–Huygens spacecraft, launched in 1997, was in orbit from 2004 to 2017.

Extraterrestrial liquid water is water in its liquid state that naturally occurs outside Earth. It is a subject of wide interest because it is recognized as one of the key prerequisites for life as we know it and is thus surmised to be essential for extraterrestrial life.

Jet Propulsion Laboratory Development Ephemeris designates one of a series of mathematical models of the Solar System produced at the Jet Propulsion Laboratory in Pasadena, California, for use in spacecraft navigation and astronomy. The models consist of numeric representations of positions, velocities and accelerations of major Solar System bodies, tabulated at equally spaced intervals of time, covering a specified span of years. Barycentric rectangular coordinates of the Sun, eight major planets and Pluto, and geocentric coordinates of the Moon are tabulated.

Interplanetary contamination refers to biological contamination of a planetary body by a space probe or spacecraft, either deliberate or unintentional.

<span class="mw-page-title-main">Planetary surface</span> Where the material of a planetary masss outer crust contacts its atmosphere or outer space

A planetary surface is where the solid or liquid material of certain types of astronomical objects contacts the atmosphere or outer space. Planetary surfaces are found on solid objects of planetary mass, including terrestrial planets, dwarf planets, natural satellites, planetesimals and many other small Solar System bodies (SSSBs). The study of planetary surfaces is a field of planetary geology known as surface geology, but also a focus on a number of fields including planetary cartography, topography, geomorphology, atmospheric sciences, and astronomy. Land is the term given to non-liquid planetary surfaces. The term landing is used to describe the collision of an object with a planetary surface and is usually at a velocity in which the object can remain intact and remain attached.

<span class="mw-page-title-main">Orbit of Mars</span> Martian orbit around the Sun

Mars has an orbit with a semimajor axis of 1.524 astronomical units, and an eccentricity of 0.0934. The planet orbits the Sun in 687 days and travels 9.55 AU in doing so, making the average orbital speed 24 km/s.

<span class="mw-page-title-main">Bethany Ehlmann</span> American planetary scientist

Bethany List Ehlmann is an American geologist and a professor of Planetary Science at California Institute of Technology. A leading researcher in planetary geology, Ehlmann is also the President of The Planetary Society, Director of the Keck Institute for Space Studies, and a Research Scientist at NASA's Jet Propulsion Laboratory.

References

  1. Rüpke (2007) A companion to Roman religion
  2. Booth (1923) Flowers of Roman poesy
  3. "Definition of tellurian". www.merriam-webster.com. Retrieved 2024-06-06.
  4. "David Morrison (2008) Ask an Astrobiologist". Archived from the original on April 25, 2009.
  5. E.g. Giovanni Vulpetti (2013) Fast Solar Sailing, p. 333.
  6. Parker, A. H.; Buie, M. W.; Grundy, W. M.; Noll, K. S. (2016-04-25). "Discovery of a Makemakean Moon". The Astrophysical Journal. 825 (1): L9. arXiv: 1604.07461 . Bibcode:2016ApJ...825L...9P. doi: 10.3847/2041-8205/825/1/L9 . S2CID   119270442.
  7. "Schiaparelli on Mars" (1895 [1894]) Nature, v. 51
  8. Lewis (1888) A Latin dictionary for schools
  9. 1 2 "Enabling Exploration with Small Radioisotope Power Systems" (PDF). NASA. September 2004. Archived from the original (PDF) on 22 December 2016. Retrieved 26 January 2016.
  10. Angley (1847) De Clifford, the philosopher
  11. Müller et al. (2010) Azimuthal plasma flow in the Kronian magnetosphere, J. Geophys. Res. 115, A08203
  12. Pennsylvania school journal, v. 29 (1880)
  13. E. N. Slyuta; M. A. Kreslavsky (1990). Intermediate (20-100 KM ) Sized Volcanic Edifices on Venus (PDF). Lunar and planetary science XXI. Lunar and Planetary Institute. p. 1174(for Sedna Planitia){{cite conference}}: CS1 maint: postscript (link)
  14. Jet Propulsion Laboratory (2010) Dawn Journal, March 28
  15. Tsiolkovsky (1960) The call of the cosmos
  16. Meteoritics & planetary science, Volume 42, Issues 6–8, 2007
  17. Origin and evolution of Earth, National Research Council et al., 2008
  18. Raitala (1993) "Crustal tectonic zone on Venus", Earth, Moon, and Planets, v. 64, no. 2
  19. "A theoretical study of the martian and cytherian ionospheres", NASA Technical Reports Server, JPL-TR-32-398
  20. Goodsell Observatory (1909) Popular astronomy, v. 17
  21. Duffy (2009) The Constitution of Shelley's Poetry
  22. Boardman (2001) The poems of Francis Thompson
  23. Patricia Brace (2011) The Broadview Anthology of Sixteenth-Century Poetry and Prose, p. 607
  24. Harry Shipman (2013) Humans in Space: 21st Century Frontiers, p. 317
  25. The Century Dictionary and Cyclopedia (1911)
  26. Harland (2000) Jupiter odyssey: the story of NASA's Galileo mission
  27. Monthly notices of the Royal Astronomical Society, v.71, 1911
  28. Greenberg (2005) Europa: the ocean moon
  29. Journal of Geophysical Research, v. 95 (1990)
  30. "Electron Beams and Ion Composition Measured at Io and in Its Torus", Science, 1996 October 18
  31. Anthon (1849) The Aeneïd of Virgil
  32. "JPL (2007) Cassini Equinox Mission: Dionean Linea". Archived from the original on 2016-03-03. Retrieved 2010-05-26.
  33. JBIS: journal of the British Interplanetary Society, v. 36 (1983)
  34. 1 2 "JPL (ca. 2009) Cassini Equinox Mission: Mimas". Archived from the original on 2015-09-05. Retrieved 2010-05-26.
  35. Lebowitz (1970) Progress into silence: a study of Melville's heroes
  36. "JPL (2010) Cassini Equinox Mission: Enceladan Tectonics". Archived from the original on 2016-03-04. Retrieved 2010-05-26.
  37. "JPL (ca. 2008) Cassini Equinox Mission: Hyperion".
  38. "JPL (ca. 2008) Cassini Equinox Mission: Iapetus". Archived from the original on 2015-03-26. Retrieved 2010-05-26.
  39. Harrison (1908) Prolegomena to the study of Greek religion, ed. 2
  40. The Westminster review, v. 140 (1893)
  41. "JPL (ca. 2008) Cassini Equinox Mission: Rhea". Archived from the original on 2016-04-12. Retrieved 2010-05-26.
  42. Şengör & Atayman (2009) The Permian extinction and the Tethys
  43. "Cassini Solstice Mission: Tethys". Archived from the original on 2016-04-04. Retrieved 2010-05-26.
  44. JPL (ca. 2008) Cassini Equinox Mission: Huygens Landed with a Splat "Cassini Equinox Mission: Huygens Landed with a Splat". Archived from the original on 2010-06-20. Retrieved 2010-05-26.
  45. Milton, Hughes (2003) Complete poems and major prose
  46. DeKoven (1991) Rich and strange: gender, history, modernism
  47. Journal of Geophysical Research, v. 93 (1988)
  48. Robertson (1929) The life of Miranda
  49. Normand (1970) Nathaniel Hawthorne
  50. 1 2 James Hall III (2015) Moons of the Solar System, p. 150
  51. Bunbury (1883) A history of ancient geography
  52. Kathryn Bosher (2012) Theater outside Athens: Drama in Greek Sicily and South Italy, pp 100, 104–105
  53. When capitalized, "Galactic" refers specifically to the Milky Way galaxy.
  54. The Independent, v. 55, p. 964 (1903)