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Naming of natural satellites

From Wikipedia, the free encyclopedia

The naming of natural satellites has been the responsibility of the IAU's committee for Planetary System Nomenclature since 1973. That committee is known today as the Working Group for Planetary System Nomenclature (WGPSN).

Prior to its formation, the names of satellites have had varying histories. The choice of names is often determined by a satellite's discoverer; however, historically some satellites were not given names for many decades or even centuries after their discovery.

Contents

[edit] Naming of satellites by planet

[edit] Mars

The moons of Mars (Phobos and Deimos) were named by Asaph Hall in 1878, soon after he discovered them.

[edit] Jupiter

The Galilean moons of Jupiter (Io, Europa, Ganymede and Callisto) were named by Simon Marius soon after their discovery in 1610. However, by the late 19th century these names had fallen out of favor, and for a long time (until the mid 20th century) it was most common to refer to them in the astronomical literature simply as "Jupiter I", "Jupiter II", etc., or as "the first satellite of Jupiter", "Jupiter's second satellite", etc.

The moons of Jupiter discovered between 1904 and 1951 were not named until 1975, being known until then simply by their Roman numeral designations (Jupiter VI through Jupiter XII). The moon Amalthea (Jupiter V), discovered in 1892, was unofficially named but its name was also not made official until 1975. Since the names of the Galilean satellites themselves had fallen out of favor, it is perhaps not unusual that the discoverers of the new smaller satellites did not see fit to name them either.

Most likely Charles Kowal's discovery of Leda (Jupiter XIII) in 1974 finally prompted the International Astronomical Union to establish a formal nomenclature process. Under the new process, informal names given to seven of the satellites were abandoned in favor of new names.[1][2]

Number Unofficial name (pre-1975) Official name (since 1975)
Jupiter V Amalthea Amalthea
Jupiter VI Hestia Himalia
Jupiter VII Hera Elara
Jupiter VIII Poseidon Pasiphaë
Jupiter IX Hades Sinope
Jupiter X Demeter Lysithea
Jupiter XI Pan Carme
Jupiter XII Adrastea Ananke

Current practice is that newly discovered moons of Jupiter must be named after lovers of the mythological Jupiter (Zeus). A convention has also emerged among the outer moons, whereby prograde moons are given names ending in 'a' or 'o', and retrograde moons receive names ending in 'e'. In 2004, with new Jovian moons continuing to be discovered, these rules were found to be excessively restrictive, and so the IAU agreed to permit moons to be named after Zeus's descendants as well.

[edit] Saturn

The seven known moons (at the time) of Saturn were named in 1847 by John Herschel. Herschel's system was to name Saturn's moons after the mythological Greek Titans. Until then, Titan was known as the "Huygenian (or Huyghenian) satellite of Saturn" and the other moons had Roman numeral designations in order of their distance from Saturn. Subsequent discoverers of Saturnian moons followed Herschel's scheme: Hyperion was discovered soon after in 1848; the ninth moon, Phoebe was named by its discoverer in 1899 soon after its discovery; and the name of Janus was suggested by its discoverer, Audouin Dollfus.

Current IAU practice for newly discovered inner moons is to continue with Herschel's system, naming them after Titans or their descendants. However, the increasing number of moons that were being discovered in the 21st century caused the IAU to draw up a new scheme for the outer moons, which are named after giants in the mythologies of other cultures. Since the outer moons fall naturally into three groups, one group is named after Norse giants, one after Gallic giants, and one after Inuit giants. The only moon that fails to fit this scheme is the Greek-named Phoebe, which is in the Norse group.

[edit] Uranus

The first two Uranian moons, discovered in 1787, did not receive names until 1852, a year after two more moons had been discovered. The responsibility for naming was taken by John Herschel, son of the discoverer of Uranus. Herschel broke with tradition: instead of assigning names from Greek mythology, he named the moons after magical spirits in English literature: Oberon and Titania from William Shakespeare's A Midsummer Night's Dream, and Ariel and Umbriel from Alexander Pope's The Rape of the Lock.

Subsequent naming choices have accorded with Herschel's choices. In 1949, the fifth moon, Miranda, was named by its discoverer after a character in Shakespeare's The Tempest. Current IAU practice is to name moons after characters from Shakespeare's plays and The Rape of the Lock (although the names from Shakespeare far outnumber those from Pope). At first, the outermost moons were all named after characters from one play, The Tempest; but with Margaret being named from Much Ado About Nothing that trend has ended.

[edit] Neptune

The one known moon (at the time) of Neptune was not named for many decades. Although the name Triton was suggested in 1880, it did not come into general use until the mid 20th-century. In the astronomical literature it was simply referred to as "the satellite of Neptune". Later, the second known moon, Nereid, was named by its discoverer in 1949 soon after its discovery.

Current IAU practice for newly discovered Neptunian moons is to accord with these first two choices by naming them after Greek sea deities.

[edit] Pluto

The name of Pluto moon Charon was suggested by James W. Christy, its discoverer, soon after its discovery.

As of June 22, 2006, the other two moons are named Hydra and Nix.

[edit] Eris

The name of Eris's moon Dysnomia was suggested by its discoverer Michael E. Brown, who also suggested the name of the dwarf planet. The names were accepted by the IAU on 14 September 2006.

[edit] Roman numeral designations

The Roman numbering system for satellites arose with the very first discovery of natural satellites other than Earth's Moon: Galileo referred to the Galilean moons as I through IV (counting from Jupiter outward), in part to spite his rival Simon Marius, who had proposed the names now adopted. Similar numbering schemes naturally arose with the discovery of moons around Saturn, Uranus, and Mars. The numbers initially designated the moons in orbital sequence, and were re-numbered after each new discovery; for instance, before the discovery of Mimas and Enceladus in 1789, Tethys was Saturn I, Dione Saturn II, etc.[3], but after the new moons were discovered, Mimas became Saturn I, Enceladus Saturn II, Tethys Saturn III and Dione Saturn IV.

After the mid-to-late nineteenth century, however, the numeration became fixed, and later discoveries failed to conform with the orbital sequence scheme. Amalthea, discovered in 1892, was labelled "Jupiter V" although it orbits closer to Jupiter than does Io (Jupiter I). The unstated convention then became, at the close of the nineteenth century, that the numbers more or less reflected the order of discovery, except for prior historical exceptions (see Timeline of discovery of Solar System planets and their natural satellites); though if a large number of satellites were discovered in a short span of time, the group could be numbered in orbital sequence, or according to other principles than strictly by order of discovery. The convention has been extended to natural satellites of minor planets, such as (87) Sylvia I Romulus.

Roman numerals are usually not assigned to satelllites until they are named, so many satellites that have been discovered but only have provisional designations do not have Roman numerals assigned to them. Since the International Astronomical Union began assigning names to all satellites in 1975, the use of Roman numeral designations has diminished, and some are very rarely used; Phobos and Deimos are rarely referred to as Mars I and Mars II, and the Moon is never referred to as "Earth I".

The last thirteen named satellites of Saturn, from Aegir to Surtur, were named in alphabetical order corresponding to their Roman numerals.

[edit] Table of natural satellites by Roman numeral

(with year of discovery and actual order of distance)

Roman
numeral
Mars Jupiter Saturn Uranus Neptune Pluto
I Phobos 1877 Io 1610 5 Mimas 1789 8 Ariel 1851 15 Triton 1846 7 Charon 1978
II Deimos 1877 Europa 1610 6 Enceladus 1789 11 Umbriel 1851 16 Nereid 1949 8 Nix 2005
III Ganymede 1610 7 Tethys 1684 12 Titania 1787 17 Naiad 1989 1 Hydra 2005
IV Callisto 1610 8 Dione 1684 15 Oberon 1787 18 Thalassa 1989 2
V Amalthea 1892 3 Rhea 1672 18 Miranda 1948 14 Despina 1989 3
VI Himalia 1904 11 Titan 1655 19 Cordelia 1986 1 Galatea 1989 4
VII Elara 1905 13 Hyperion 1848 20 Ophelia 1986 2 Larissa 1989 5
VIII Pasiphae 1908 52 Iapetus 1671 21 Bianca 1986 3 Proteus 1989 6
IX Sinope 1914 58 Phoebe 1899 24 Cressida 1986 4 Halimede 2002 9
X Lysithea 1938 12 Janus 1980 7 Desdemona 1986 5 Psamathe 2003 12
XI Carme 1938 45 Epimetheus 1980 6 Juliet 1986 6 Sao 2002 10
XII Ananke 1951 31 Helene 1980 15a Portia 1986 7 Laomedeia 2002 11
XIII Leda 1974 10 Telesto 1980 12a Rosalind 1986 8 Neso 2002 13
XIV Thebe 1979 4 Calypso 1980 12b Belinda 1986 10
XV Adrastea 1979 2 Atlas 1980 3 Puck 1985 12
XVI Metis 1979 1 Prometheus 1980 4 Caliban 1997 20
XVII Callirrhoe 1999 46 Pandora 1980 5 Sycorax 1997 23
XVIII Themisto 2000 9 Pan 1990 1 Prospero 1999 25
XIX Megaclite 2001 62 Ymir 2000 54 Setebos 1999 26
XX Taygete 2001 35 Paaliaq 2000 25 Stephano 1999 21
XXI Chaldene 2001 37 Tarvos 2000 36 Trinculo 2002 22
XXII Harpalyke 2000 27 Ijiraq 2000 23 Francisco 2003 19
XXIII Kalyke 2001 44 Suttungr 2000 42 Margaret 2003 24
XXIV Iocaste 2001 24 Kiviuq 2000 22 Ferdinand 2003 27
XXV Erinome 2001 41 Mundilfari 2000 37 Perdita 2003 11
XXVI Isonoe 2001 55 Albiorix 2000 27 Mab 2003 13
XXVII Praxidike 2001 26 Skathi 2000 26 Cupid 2003 9
XXVIII Autonoe 2002 60 Erriapo 2000 29
XXIX Thyone 2002 30 Siarnaq 2000 31
XXX Hermippe 2002 29 Thrymr 2000 46
XXXI Aitne 2002 33 Narvi 2003 41
XXXII Eurydome 2002 47 Methone 2004 9
XXXIII Euanthe 2002 21 Pallene 2004 10
XXXIV Euporie 2002 17 Polydeuces 2004 15b
XXXV Orthosie 2002 23 Daphnis 2005 2
XXXVI Sponde 2002 59 Aegir 2004 47
XXXVII Kale 2002 34 Bebhionn 2004 28
XXXVIII Pasithee 2002 48 Bergelmir 2004 40
XXXIX Hegemone 2003 53 Bestla 2004 48
XL Mneme 2003 28 Farbauti 2004 45
XLI Aoede 2003 42 Fenrir 2004 51
XLII Thelxinoe 2004 20 Fornjot 2004 56
XLIII Arche 2002 54 Hati 2004 43
XLIV Kallichore 2003 43 Hyrokkin 2004 34
XLV Helike 2003 22 Kari 2006 53
XLVI Carpo 2003 15 Loge 2006 55
XLVII Eukelade 2003 50 Skoll 2006 30
XLVIII Cyllene 2003 49 Surtur 2006 52
XLIX Kore 2003 61

[edit] Recent developments

As of the IAU General Assembly in July 2004 [1], the WGPSN:

  • named thirty-four satellites of Jupiter and Saturn and one Uranus satellite, bringing the total number of known planetary satellites to 101, with over two dozen more awaiting recovery and naming;
  • suggested it may become advisable to not name small satellites (current CCD technology makes it possible to discover satellites as small as 1 km);
  • allowed Jovian satellites to be named for Zeus' descendants in addition to his lovers and favorites which were the previous source of names;
  • allowed satellites of Saturn to have names of giants and monsters in mythologies other than the Greco-Roman, including (so far) Gallic, Inuit and Norse.

[edit] See also

[edit] Notes

[edit] References


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