Global InformationEnceladus information
 Enceladus imaged by the Cassini orbiter, October 2015[a] | |||||||||||||
| Discovery | |||||||||||||
|---|---|---|---|---|---|---|---|---|---|---|---|---|---|
| Discovered by | William Herschel | ||||||||||||
| Discovery date | August 28, 1789[1] | ||||||||||||
| Designations | |||||||||||||
Designation | Saturn II | ||||||||||||
| Pronunciation | /ɛnˈsɛlədəs/[2] | ||||||||||||
Named after | Ἐγκέλαδος Egkelados | ||||||||||||
| Adjectives | Enceladean /ɛnsəˈleɪdiən/[3][4] | ||||||||||||
| Orbital characteristics | |||||||||||||
Semi-major axis | 237948 km[5] | ||||||||||||
| Eccentricity | 0.0047[5][6] | ||||||||||||
Orbital period (sidereal) | 1.370218 d[5] | ||||||||||||
| Inclination | 0.009° (to Saturn's equator)[5] | ||||||||||||
| Satellite of | Saturn | ||||||||||||
| Physical characteristics | |||||||||||||
| Dimensions | 513.2 × 502.8 × 496.6 km[5][7] | ||||||||||||
Mean radius | 252.1±0.2 km[7][8] (0.0395 Earths, 0.1451 Moons) | ||||||||||||
| Mass | (1.080318±0.00028)×1020 kg[8] (1.8×10−5 Earths) | ||||||||||||
Mean density | 1.6097±0.0038 g/cm3[8] | ||||||||||||
Surface gravity | 0.113 m/s2 (0.0116 g) | ||||||||||||
Moment of inertia factor | 0.3305±0.0025[9] | ||||||||||||
Escape velocity | 0.239 km/s (860.4 km/h)[5] | ||||||||||||
Synodic rotation period | Synchronous | ||||||||||||
Axial tilt | 0 | ||||||||||||
| Albedo | 1.375±0.008 (geometric at 550 nm)[10] or 0.81±0.04 (Bond)[11] | ||||||||||||
| |||||||||||||
Apparent magnitude | 11.7[13] | ||||||||||||
| Atmosphere | |||||||||||||
Surface pressure | Trace, significant spatial variability[14][15] | ||||||||||||
| Composition by volume | 91% water vapor 4% nitrogen 3.2% carbon dioxide 1.7% methane[16] | ||||||||||||
Enceladus is the sixth-largest moon of Saturn and the 19th-largest in the Solar System. It is about 500 kilometers (310 miles) in diameter,[5] about a tenth of that of Saturn's largest moon, Titan. It is mostly covered by fresh, clean ice, making it one of the most reflective bodies of the Solar System. Consequently, its surface temperature at noon reaches only −198 °C (75.1 K; −324.4 °F), far colder than a light-absorbing body would be. Despite its small size, Enceladus has a wide variety of surface features, ranging from old, heavily cratered regions to young, tectonically deformed terrain.
Enceladus was discovered on August 28, 1789, by William Herschel,[1][17][18] but little was known about it until the two Voyager spacecrafts, Voyager 1 and Voyager 2, flew by Saturn in 1980 and 1981.[19] In 2005, the spacecraft Cassini started multiple close flybys of Enceladus, revealing its surface and environment in greater detail. In particular, Cassini discovered water-rich plumes venting from the south polar region.[20] Cryovolcanoes near the south pole shoot geyser-like jets of water vapor, molecular hydrogen, other volatiles, and solid material, including sodium chloride crystals and ice particles, into space, totaling about 200 kilograms (440 pounds) per second.[15][19][21] More than 100 geysers have been identified.[22] Some of the water vapor falls back as "snow"; the rest escapes and supplies most of the material making up Saturn's E ring.[23][24] According to NASA scientists, the plumes are similar in composition to comets.[25] In 2014, NASA reported that Cassini had found evidence for a large south polar subsurface ocean of liquid water with a thickness of around 10 km (6 mi).[26][27][28] The existence of Enceladus' subsurface ocean has since been mathematically modelled and replicated.[29]
These observations of active cryoeruptions, along with the finding of escaping internal heat and very few (if any) impact craters in the south polar region, show that Enceladus is currently geologically active. Like many other satellites in the extensive systems of the giant planets, Enceladus participates in an orbital resonance. Its resonance with Dione excites its orbital eccentricity, which is damped by tidal forces, tidally heating its interior and driving the geological activity.[30]
Cassini performed chemical analysis of Enceladus's plumes, finding evidence for hydrothermal activity,[31][32] possibly driving complex chemistry.[33] Ongoing research on Cassini data suggests that Enceladus's hydrothermal environment could be habitable to some of Earth's hydrothermal vent's microorganisms, and that plume-found methane could be produced by such organisms.[34][35]
Cite error: There are <ref group=lower-alpha> tags or {{efn}} templates on this page, but the references will not show without a {{reflist|group=lower-alpha}} template or {{notelist}} template (see the help page).
- ^ a b "Planetary Body Names and Discoverers". Gazetteer of Planetary Nomenclature. USGS Astrogeology Science Center. Archived from the original on August 25, 2009. Retrieved January 12, 2015.
- ^ "Enceladus". Lexico UK English Dictionary. Oxford University Press. Archived from the original on July 31, 2020.
"Enceladus". Merriam-Webster.com Dictionary. - ^ Freitas, R. A. (1983). "Terraforming Mars and Venus Using Machine Self-Replicating Systems (SRS)". Journal of the British Interplanetary Society. 36: 139. Bibcode:1983JBIS...36..139F.
- ^ Postberg et al. "Plume and surface composition of Enceladus", p. 129–130, 148, 156; Lunine et al. "Future Exploration of Enceladus and Other Saturnian Moons", p. 454; in Schenk et al., eds. (2018) Enceladus and the Icy Moons of Saturn
- ^ a b c d e f g "Enceladus: Facts & Figures". Solar System Exploration. NASA. August 12, 2013. Archived from the original on October 16, 2013. Retrieved April 26, 2014.
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Roatsch et al. 2009was invoked but never defined (see the help page). - ^ a b c Jacobson, Robert. A. (November 1, 2022). "The Orbits of the Main Saturnian Satellites, the Saturnian System Gravity Field, and the Orientation of Saturn's Pole". The Astronomical Journal. 164 (5): 199. Bibcode:2022AJ....164..199J. doi:10.3847/1538-3881/ac90c9. S2CID 252992162.
- ^ McKinnon, W. B. (2015). "Effect of Enceladus's rapid synchronous spin on interpretation of Cassini gravity". Geophysical Research Letters. 42 (7): 2137–2143. Bibcode:2015GeoRL..42.2137M. doi:10.1002/2015GL063384.
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- ^ a b Hansen, Candice J.; Esposito, L.; et al. (2006). "Enceladus' Water Vapor Plume". Science. 311 (5766): 1422–5. Bibcode:2006Sci...311.1422H. doi:10.1126/science.1121254. PMID 16527971. S2CID 2954801.
- ^ Waite, Jack Hunter Jr.; Combi, M. R.; et al. (2006). "Cassini Ion and Neutral Mass Spectrometer: Enceladus Plume Composition and Structure". Science. 311 (5766): 1419–22. Bibcode:2006Sci...311.1419W. doi:10.1126/science.1121290. PMID 16527970. S2CID 3032849.
- ^ Herschel, W. (January 1, 1790). "Account of the Discovery of a Sixth and Seventh Satellite of the Planet Saturn; With Remarks on the Construction of Its Ring, Its Atmosphere, Its Rotation on an Axis, and Its Spheroidal Figure". Philosophical Transactions of the Royal Society of London. 80: 1–20. doi:10.1098/rstl.1790.0004. Archived from the original on April 27, 2014. Retrieved April 27, 2014.
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Herschel_1795was invoked but never defined (see the help page). - ^ a b Lovett, Richard A. (September 4, 2012). "Secret life of Saturn's moon: Enceladus". Cosmos Magazine. Archived from the original on August 15, 2014. Retrieved August 29, 2013.
- ^ Chang, Kenneth (March 12, 2015). "Suddenly, It Seems, Water Is Everywhere in Solar System". The New York Times. Archived from the original on May 9, 2020. Retrieved March 13, 2015.
- ^ Spencer, John R.; Nimmo, F. (May 2013). "Enceladus: An Active Ice World in the Saturn System". Annual Review of Earth and Planetary Sciences. 41: 693–717. Bibcode:2013AREPS..41..693S. doi:10.1146/annurev-earth-050212-124025. S2CID 140646028.
- ^ Dyches, Preston; Brown, Dwayne; et al. (July 28, 2014). "Cassini Spacecraft Reveals 101 Geysers and More on Icy Saturn Moon". NASA/JPL. Archived from the original on July 14, 2017. Retrieved July 29, 2014.
- ^ "Icy Tendrils Reaching into Saturn Ring Traced to Their Source". NASA News. April 14, 2015. Archived from the original on April 16, 2015. Retrieved April 15, 2015.
- ^ "Ghostly Fingers of Enceladus". NASA/JPL/Space Science Institute. September 19, 2006. Archived from the original on April 27, 2014. Retrieved April 26, 2014.
- ^ Battersby, Stephen (March 26, 2008). "Saturn's moon Enceladus surprisingly comet-like". New Scientist. Archived from the original on June 30, 2015. Retrieved April 16, 2015.
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SCI-20140404was invoked but never defined (see the help page). - ^ Tjoa, J. N. K. Y.; Mueller, M.; Tak, F. F. S. van der (April 1, 2020). "The subsurface habitability of small, icy exomoons". Astronomy & Astrophysics. 636: A50. arXiv:2003.09231. Bibcode:2020A&A...636A..50T. doi:10.1051/0004-6361/201937035. ISSN 0004-6361. S2CID 214605690.
- ^ Efroimsky, M. (January 15, 2018). "Tidal viscosity of Enceladus". Icarus. 300: 223–226. arXiv:1706.09000. Bibcode:2018Icar..300..223E. doi:10.1016/j.icarus.2017.09.013. S2CID 119462312.
- ^ Waite, Jack Hunter Jr.; Glein, C. R.; Perryman, R. S.; Teolis, Ben D.; Magee, B. A.; Miller, G.; Grimes, J.; Perry, M. E.; Miller, K. E.; Bouquet, A.; Lunine, Jonathan I.; Brockwell, T.; Bolton, S. J. (2017). "Cassini finds molecular hydrogen in the Enceladus plume: Evidence for hydrothermal processes". Science. 356 (6334): 155–159. Bibcode:2017Sci...356..155W. doi:10.1126/science.aai8703. PMID 28408597.
- ^ Hsu, Hsiang-Wen; Postberg, Frank; et al. (March 11, 2015). "Ongoing hydrothermal activities within Enceladus". Nature. 519 (7542): 207–10. Bibcode:2015Natur.519..207H. doi:10.1038/nature14262. PMID 25762281. S2CID 4466621.
- ^ Postberg, Frank; et al. (June 27, 2018). "Macromolecular organic compounds from the depths of Enceladus". Nature. 558 (7711): 564–568. Bibcode:2018Natur.558..564P. doi:10.1038/s41586-018-0246-4. PMC 6027964. PMID 29950623.
- ^ Taubner, Ruth-Sophie; Pappenreiter, Patricia; Zwicker, Jennifer; Smrzka, Daniel; Pruckner, Christian; Kolar, Philipp; Bernacchi, Sébastien; Seifert, Arne H.; Krajete, Alexander; Bach, Wolfgang; Peckmann, Jörn; Paulik, Christian; Firneis, Maria G.; Schleper, Christa; Rittmann, Simon K.-M. R. (February 27, 2018). "Biological methane production under putative Enceladus-like conditions". Nature Communications. 9 (1): 748. Bibcode:2018NatCo...9..748T. doi:10.1038/s41467-018-02876-y. ISSN 2041-1723. PMC 5829080. PMID 29487311.
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