Eukelade: Difference between revisions
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{{Infobox planet |
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'''Eukelade''' ''(ew-kel'-ə-dee,'' {{IPA2|jʊˈkɛlədi}}; Greek ''Ευκελαδη),'' or '''Jupiter XLVII''', is a [[retrograde motion|retrograde]] [[irregular satellite]] of [[Jupiter (planet)|Jupiter]]. |
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It was discovered by a team of astronomers from the [[University of Hawaii]] led by [[Scott S. Sheppard]] in [[2003]], and received the temporary designation '''S/2003 J 1'''. |
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| image = Eukelade s2003j1movie arrow.gif |
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| image_scale = |
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| caption = Images of Eukelade taken by [[Scott Sheppard]] on 4 March 2003 |
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| pronounced = {{IPAc-en|j|uː|ˈ|k|ɛ|l|ə|d|iː}} |
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| adjective = Eukeladean {{IPAc-en|ˌ|juː|k|ᵻ|l|ə|ˈ|d|iː|ə|n}} |
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| named_after = [[Eucelade|Ευκελάδη]] ''Eykeladē'' |
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| discoverer = [[Scott S. Sheppard]] et al. |
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| discovered = 2003 |
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| mpc_name = Jupiter XLVII |
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| alt_names = S/2003 J 1 |
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| orbit_ref =  <ref>[https://sites.google.com/carnegiescience.edu/sheppard/moons/jupitermoons S.S. Sheppard (2019), Moons of Jupiter, ''Carnegie Science'', on line]</ref> |
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| semimajor = {{val|23661000|u=km}} |
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| inclination = 165.5° |
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| eccentricity = 0.272 |
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| arg_peri = 325.6° |
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| asc_node = 206.3° |
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| mean_anomaly = 98.4° |
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| period = −693.02 days<ref name="MPC127088"/> |
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| satellite_of = [[Jupiter]] |
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| group = [[Carme group]] |
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| magnitude = 22.6 |
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| abs_magnitude = 15.9<ref name="MPC127088"/> |
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| spectral_type = B–V = 0.79 ± 0.07, V–R = 0.50 ± 0.07<ref name="GraykowskiJewitt2018"/> |
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| mean_diameter = 4 km |
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}} |
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'''Eukelade''' {{IPAc-en|j|uː|ˈ|k|ɛ|l|ə|d|iː}}, also known as '''{{nowrap|Jupiter XLVII}}''', is a [[retrograde motion|retrograde]] [[irregular satellite]] of [[Jupiter]]. It was discovered by a team of astronomers from the [[University of Hawaii]] led by [[Scott S. Sheppard]] in 2003, and received the temporary designation '''{{nowrap|S/2003 J 1}}'''.<ref>[http://www.cbat.eps.harvard.edu/iauc/08000/08087.html IAUC 8087: ''Satellites of Jupiter''] 2003 March 4 (discovery)</ref><ref>[http://cfa-www.harvard.edu/iau/mpec/K03/K03E11.html MPEC 2003-E11: ''S/2003 J 1, 2003 J 2, 2003 J 3, 2003 J 4, 2003 J 5, 2003 J 6, 2003 J 7''] 2003 March 4 (discovery and ephemeris)</ref><ref>[http://cfa-www.harvard.edu/mpec/K03/K03E29.html MPEC 2003-E29: ''S/2003 J 9, 2003 J 10, 2003 J 11, 2003 J 12; S/2003 J 1, 2003 J 6''] 2003 April 3 (revised ephemeris)</ref> |
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⚫ | Eukelade is about 4 kilometres in diameter, and orbits Jupiter at an average distance of 23,484 |
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⚫ | Eukelade is about 4 kilometres in diameter, and orbits Jupiter at an average distance of 23,484,000 km in 693.02 days, at an [[inclination]] of 164° to the [[ecliptic]] (165° to Jupiter's equator), in a [[retrograde motion|retrograde]] direction and with an [[eccentricity (orbit)|eccentricity]] of 0.2829. |
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It is named after [[Eukelade]], described by some Greek writers as one of the [[Muse]]s, and thus a daughter of [[Zeus]] (Jupiter). [http://www.educnet.education.fr/musagora/muses/musesfr/scholies.pdf] |
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It was named in March 2005 after [[Eucelade]] - according to [[John Tzetzes]], listed by some (unnamed) Greek writers as one of the [[Muse]]s.<ref>* Marta Cardin, Olga Tribulato: ''Enumerating the Muses: Tzetzes in Hes. Op. 1 and the Parody of Catalogic Poetry in Epicharmus.'' In: Marco Ercoles, Lara Pagani, Filippomaria Pontani, Giuseppe Ucciardello: ''Approaches to Greek Poetry: Homer, Hesiod, Pindar, and Aeschylus in Ancient Exegesis'' (= ''Trends in Classics.'' Supplementary Volumes 73). De Gruyter, Berlin/Boston 2019, p. 161–192; here p. 171.</ref> |
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Eukelade belongs to the [[Carme group]], made up of irregular retrograde moons orbiting Jupiter at a distance ranging between 23 and 24 Gm and at an inclination of about 165°. |
Eukelade belongs to the [[Carme group]], made up of irregular retrograde moons orbiting Jupiter at a distance ranging between 23 and 24 Gm and at an inclination of about 165°. |
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==References== |
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<br clear="all" /> |
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{{reflist|refs= |
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<center>''... | [[Cyllene (moon)|Cyllene]] | '''Eukelade''' | [[S/2003 J 4]] | ...''</center> |
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<ref name="MPC127088">{{cite web |
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|title = M.P.C. 127088 |
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|url = https://minorplanetcenter.net/iau/ECS/MPCArchive/2020/MPC_20201117.pdf |
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|work = Minor Planet Circular |
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|publisher = Minor Planet Center |
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|date = 17 November 2020}}</ref> |
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<ref name="GraykowskiJewitt2018">{{Cite journal |
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|last=Graykowski |first=Ariel |
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|last2=Jewitt |first2=David |
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|date=2018-04-05 |
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|title=Colors and Shapes of the Irregular Planetary Satellites |
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|url=https://iopscience.iop.org/article/10.3847/1538-3881/aab49b |
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|journal=The Astronomical Journal |
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|language=en |
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|volume=155 |
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|issue=4 |
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|pages=184 |
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|doi=10.3847/1538-3881/aab49b |
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|issn=1538-3881 |
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|doi-access=free|arxiv=1803.01907 |
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}}</ref> |
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}} |
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{{Moons of Jupiter}} |
{{Moons of Jupiter}} |
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{{DEFAULTSORT:Eukelade (Moon)}} |
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[[Category: |
[[Category:Carme group]] |
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[[Category:Moons of Jupiter]] |
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[[Category:Irregular satellites]] |
[[Category:Irregular satellites]] |
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[[Category:Discoveries by Scott S. Sheppard]] |
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[[Category:Astronomical objects discovered in 2003]] |
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[[als:Eukelade (Mond)]] |
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[[Category:Moons with a retrograde orbit]] |
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[[br:Eukelade (loarenn)]] |
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[[bg:Евкелада (спътник)]] |
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[[da:Eukelade (måne)]] |
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[[de:Eukelade (Mond)]] |
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[[fr:Eukélade (lune)]] |
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[[hr:Eukelada (mjesec)]] |
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[[lt:Eukeladė (palydovas)]] |
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[[nl:Eukelade (maan)]] |
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[[ja:エウケラデ (衛星)]] |
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[[pl:Eukelade (księżyc)]] |
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[[sk:Eukelade (mesiac)]] |
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[[zh:木卫四十七]] |
Latest revision as of 16:30, 6 November 2024
Discovery | |
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Discovered by | Scott S. Sheppard et al. |
Discovery date | 2003 |
Designations | |
Designation | Jupiter XLVII |
Pronunciation | /juːˈkɛlədiː/ |
Named after | Ευκελάδη Eykeladē |
S/2003 J 1 | |
Adjectives | Eukeladean /ˌjuːkɪləˈdiːən/ |
Orbital characteristics [1] | |
23661000 km | |
Eccentricity | 0.272 |
−693.02 days[2] | |
98.4° | |
Inclination | 165.5° |
206.3° | |
325.6° | |
Satellite of | Jupiter |
Group | Carme group |
Physical characteristics | |
4 km | |
Spectral type | B–V = 0.79 ± 0.07, V–R = 0.50 ± 0.07[3] |
22.6 | |
15.9[2] | |
Eukelade /juːˈkɛlədiː/, also known as Jupiter XLVII, is a retrograde irregular satellite of Jupiter. It was discovered by a team of astronomers from the University of Hawaii led by Scott S. Sheppard in 2003, and received the temporary designation S/2003 J 1.[4][5][6]
Eukelade is about 4 kilometres in diameter, and orbits Jupiter at an average distance of 23,484,000 km in 693.02 days, at an inclination of 164° to the ecliptic (165° to Jupiter's equator), in a retrograde direction and with an eccentricity of 0.2829.
It was named in March 2005 after Eucelade - according to John Tzetzes, listed by some (unnamed) Greek writers as one of the Muses.[7]
Eukelade belongs to the Carme group, made up of irregular retrograde moons orbiting Jupiter at a distance ranging between 23 and 24 Gm and at an inclination of about 165°.
References
[edit]- ^ S.S. Sheppard (2019), Moons of Jupiter, Carnegie Science, on line
- ^ a b "M.P.C. 127088" (PDF). Minor Planet Circular. Minor Planet Center. 17 November 2020.
- ^ Graykowski, Ariel; Jewitt, David (2018-04-05). "Colors and Shapes of the Irregular Planetary Satellites". The Astronomical Journal. 155 (4): 184. arXiv:1803.01907. doi:10.3847/1538-3881/aab49b. ISSN 1538-3881.
- ^ IAUC 8087: Satellites of Jupiter 2003 March 4 (discovery)
- ^ MPEC 2003-E11: S/2003 J 1, 2003 J 2, 2003 J 3, 2003 J 4, 2003 J 5, 2003 J 6, 2003 J 7 2003 March 4 (discovery and ephemeris)
- ^ MPEC 2003-E29: S/2003 J 9, 2003 J 10, 2003 J 11, 2003 J 12; S/2003 J 1, 2003 J 6 2003 April 3 (revised ephemeris)
- ^ * Marta Cardin, Olga Tribulato: Enumerating the Muses: Tzetzes in Hes. Op. 1 and the Parody of Catalogic Poetry in Epicharmus. In: Marco Ercoles, Lara Pagani, Filippomaria Pontani, Giuseppe Ucciardello: Approaches to Greek Poetry: Homer, Hesiod, Pindar, and Aeschylus in Ancient Exegesis (= Trends in Classics. Supplementary Volumes 73). De Gruyter, Berlin/Boston 2019, p. 161–192; here p. 171.