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{{short description|Trojan moon of Saturn}} {{Infobox planet | name = Helene | image = Leading hemisphere of Helene - 20110618.jpg | image_scale = | caption = High-resolution view of leading hemisphere, showing gullies and apparent dust ([[regolith]]) flows (''[[Cassini–Huygens|Cassini]]'', June 2011) | discovery_ref = {{sfn|Lecacheux1980}} | discoverer = [[Pierre Laques|P. Laques]]<br />[[Jean Lecacheux|J. Lecacheux]] | discovered = March 1, 1980 | discovery_site = [[Pic du Midi Observatory]] | mpc_name = Saturn XII | alt_names = {{plainlist | * Dione B * S/1980 S 6 }} | pronounced = {{IPAc-en|ˈ|h|ɛ|l|ə|n|iː}}<ref>John Walker (1839) ''A Critical Pronouncing Dictionary and Expositor of the English Language'';<br>also per {{OED|Helena}}</ref> | named_after = [[Helen of Troy]] (Ἑλένη ''Helenē'') | adjective = Helenean {{IPAc-en|h|ɛ|l|ə|ˈ|n|iː|ə|n}}<ref>Clarified as ''Helenéan'' in Earle (1841) ''Marathon: and other poems'', p. 76.</ref> | semimajor = {{val|377600|u=km}}<ref name="jpl-satelem"/> | eccentricity = {{val|0.007}}<ref name="jpl-satelem"/> | period = {{val|2.736916|u=d}}<ref name="jpl-satelem"/> | inclination = 0.199° (to Saturn's equator) | satellite_of = [[Saturn]] | group = [[Trojan moon|L<sub>4</sub> Dione trojan]] | dimensions = {{val|45.2|x|39.2|x|26.6}} km<br/>(± {{val|0.4|x|0.6|x|0.4}} km){{sfn|Thomas|Helfenstein|2020|p=2}} | mean_diameter = {{val|36.2|0.4|u=km}}{{sfn|Thomas|Helfenstein|2020|p=2}} | volume = {{val|24840|u=km3}}{{efn|Calculated from Helene's volume-equivalent sphere radius of {{val|18.1|0.2|u=km}} given by Thomas et al. (2020){{sfn|Thomas|Helfenstein|2020|p=2}}}} | mass = {{val|7.1|0.2|e=15|u=kg}}{{sfn|Jacobson|2022|p=6}} | density = {{val|0.2926|0.0217|u=g/cm3}}{{sfn|Jacobson|2022|p=6}} | surface_grav = {{Gr|7.1e-6|22.6|4}} m/s<sup>2</sup> at longest axis<br/>to {{Gr|7.1e-6|13.3|4}} m/s<sup>2</sup> at poles | escape_velocity = {{V2|7.1e-6|22.6|4}} km/s at longest axis<br/>to {{V2|7.1e-6|13.3|4}} km/s at poles<!-- V2 template uses mass in terms of e+21 kg, radius in terms of km, and number of decimal places --> | rotation = assumed [[synchronous rotation|synchronous]] | albedo = {{val|1.67|0.20}} {{nowrap|([[geometric albedo|geometric]]){{sfn|Verbiscer|French|Showalter|Helfenstein|2007}}}} | axial_tilt = zero }} '''Helene''' {{IPAc-en|ˈ|h|ɛ|l|ə|n|iː}} is a [[natural satellite|moon]] of [[Saturn]]. It was discovered by [[Pierre Laques]] and [[Jean Lecacheux]] in 1980 from ground-based observations at [[Pic du Midi Observatory]],{{sfn|Lecacheux1980}} and was designated '''{{nowrap|S/1980 S 6}}'''.{{sfn|IAUC 3496}} In 1988 it was officially named after [[Helen of Troy]], who was the granddaughter of [[Cronus]] (Saturn) in [[Greek mythology]].{{sfn|IAUC 4609}} Helene is also designated '''{{nowrap|Saturn XII}}''' (12), which it was given in 1982, and '''Dione B''',<ref>Transactions of the International Astronomical Union, Vol. XVIIIA, 1982 (mentioned in [[#{{sfnRef|IAUC 3872}}|IAUC 3872: ''Satellites of Jupiter and Saturn'']], September 30, 1983</ref> because it is [[co-orbital]] with [[Dione (moon)|Dione]] and located in its leading [[Lagrangian point]] ({{L4}}). It is one of four known [[trojan moon]]s. [[File:Animation of Polydeuces's orbit relative to Saturn and Dione.gif|thumb|left|Animation of Helene's orbit relative to Saturn and Dione<br>{{legend2|Magenta|Polydeuces }}{{·}}{{legend2|Cyan|Helene}}{{·}}{{legend2|Lime|Dione}}{{·}}{{legend2|DarkOrange|Saturn}}]] == Exploration == Helene was initially observed from Earth in 1980,{{sfn|IAUC 3496}} and ''[[Voyager program|Voyager]]'' flybys of Saturn in the early 1980s allowed much closer views. The ''[[Cassini–Huygens]]'' mission, which went into orbit around Saturn in 2004, provided still better views, and allowed more in-depth analysis of Helene, including views of the surface under different lighting conditions. Some of the closest images of Helene to date are from the ''Cassini'' spacecraft's 1800 km flyby on March 3, 2010, and another very successful imaging sequence occurred in June 2011. There were many other approaches over the course of the ''Cassini'' mission. == Geology == Images of Helene taken by the Cassini spacecraft, with resolutions of up to 24 meters per pixel, show a landscape characterized by broad 2–10km scale depressions with interior slopes no greater than 12°.{{sfn|Hirata et al. 2014}} These basins are likely the decayed remains of old impact craters.{{sfn|Umurhan|Howard|Moore|Schenk|2015}} Thin, elongated km-scale raised grooves trace the slopes of many of Helene's basins, likely representing [[Mass wasting|mass flow]] features and indicating that the moon is undergoing active geologic processes such as [[Mass wasting|mass-wasting]] and erosion. Digital elevation models suggest that the grooves have a positive relief of between 50 and 100 meters. Helene has more than 70 craters, while it shows a bimodal appearance—the heavily cratered trailing hemisphere exhibits a crater density ten times greater than the smooth-looking leading hemisphere.{{sfn|Hirata et al. 2014}} Simulation models show that the time series of surface activity on Helene is chaotic.{{citation needed|date=February 2024}} == Surface material == Helene's surface material is of relatively high reflectance, suggesting grain sizes between 1 and 100 micrometers. Small craters appear somewhat buried, suggesting recent [[Accretion (astrophysics)|accretional processes]] of some sort. Stress-strain laboratory testing of [[Impact gardening|impact-gardened]] lunar regolith samples shows that at low packing densities, they behave like [[Non-Newtonian fluid|Non-Newtonian “Bingham” materials]], i.e., having the plastic quality of candle-wax and glaciers. This observation suggests that Helene's snow-like surface material may behave as a non-Newtonian mass flow and could be primarily responsible for the visible flow patterns seen on its low-gravity surface.{{sfn|Umurhan|Howard|Moore|Schenk|2015}} == Selected observations == Mostly raw greyscale images with near infrared or ultraviolet channels. <gallery heights=150 widths=150> File:PIA12758 Helene crop.jpg|Flow-like features on Helene's leading hemisphere (''Cassini'', January 2011) File:Helene over Saturn.jpg|Image of Helene against the backdrop of Saturn's clouds (''Cassini'', March 3, 2010) File:N00152209 Helene.jpg|Helene's Saturn-facing side, lit by [[Planetshine|saturnshine]] (''Cassini'', March 2010) File:N00152248 Helene.jpg|Close-up of Helene with Saturn in the background (''Cassini'', March 2010) File:Helene rev 127 raw 1.jpg|''[[Cassini–Huygens|Cassini]]'' image from March 3, 2010 File:PIA 10544 Helene.jpg|''Cassini'' orbiter image from November 2008 File:Cassini Helene N00086698 CL.jpg|''Cassini'' image taken July 2007 File:Helene - Voyager 2.jpg|''[[Voyager 2]]'' image (August 1981) </gallery> == Notes == {{notelist}} == References == === Citations === {{reflist|20em|refs= <ref name="jpl-satelem">{{cite web |title = Planetary Satellite Mean Orbital Parameters |url = https://ssd.jpl.nasa.gov/sats/elem/sep.html |publisher = [[Jet Propulsion Laboratory]] |access-date = 5 June 2023}}</ref> }} === Sources === '''Sources''' * {{cite journal | last = Lecacheux | first = Jean. | title = A new satellite of Saturn: Dione B | date = July 1980 | journal = Icarus | volume = 43| issue = 1 | pages = 111–115 | doi = 10.1016/0019-1035(80)90093-7 |bibcode = 1980Icar...43..111L }} * {{cite journal | last = Marsden | first = Brian G. | title = Satellites of Saturn | date = July 31, 1980 | format = discovery | journal = IAU Circular | volume = 3496 | url = http://www.cbat.eps.harvard.edu/iauc/03400/03496.html | access-date = 2011-12-23 | ref = {{sfnRef|IAUC 3496}} }} * {{cite journal | last = Marsden | first = Brian G. | title = Satellites of Jupiter and Saturn | date = September 30, 1983 | journal = IAU Circular | volume = 3872 | url = http://www.cbat.eps.harvard.edu/iauc/03800/03872.html | access-date = 2011-12-23 | ref = {{sfnRef|IAUC 3872}} }} * {{cite journal | last = Marsden | first = Brian G. | title = Satellites of Saturn and Uranus | date = June 8, 1988 | format = naming | journal = IAU Circular | volume = 4609 | url = http://www.cbat.eps.harvard.edu/iauc/04600/04609.html | access-date = 2011-12-23 | ref = {{sfnRef|IAUC 4609}} }} * {{cite journal| doi=10.1016/j.icarus.2010.01.025| last1=Thomas| first1=P. C.| date=July 2010| title=Sizes, shapes, and derived properties of the saturnian satellites after the Cassini nominal mission| journal=Icarus| volume=208| issue=1| pages=395–401| url=http://www.ciclops.org/media/sp/2011/6794_16344_0.pdf| bibcode=2010Icar..208..395T| access-date=2015-09-04| archive-date=2018-12-23| archive-url=https://web.archive.org/web/20181223003125/http://www.ciclops.org/media/sp/2011/6794_16344_0.pdf| url-status=dead}} * {{cite journal | last = Hirata | first = N. | title = Particle deposition on the saturnian satellites from ephemeral cryovolcanism on Enceladus | date = May 27, 2014 | journal = Geophysical Research Letters | volume = 41 | issue = 12 | pages = 4135–4141 | doi = 10.1002/2014GL060470 | arxiv = 2205.11265 | bibcode = 2014GeoRL..41.4135H | url = https://doi.org/10.1002/2014GL060470 | access-date = 2024-03-04 | ref = {{sfnRef|Hirata et al. 2014}} }} * {{cite journal |first1 = P. C. |last1 = Thomas |first2 = P. |last2 = Helfenstein |title = The small inner satellites of Saturn: Shapes, structures and some implications |journal = Icarus |date = July 2020 |volume = 344 |id = 113355 |pages = 20 |doi = 10.1016/j.icarus.2019.06.016 |bibcode = 2020Icar..34413355T|s2cid = 197474587 }} * {{cite journal |first1 = Robert A. |last1 = Jacobson |title = The Orbits of the Main Saturnian Satellites, the Saturnian System Gravity Field, and the Orientation of Saturn's Pole |journal = The Astronomical Journal |date = November 2022 |volume = 164 |issue = 5 |id = 199 |pages = 19 |doi-access = free |doi = 10.3847/1538-3881/ac90c9 |bibcode = 2022AJ....164..199J}} * {{cite conference |last1=Umurhan |first1=O. M. |last2=Howard |first2=A. D. |last3=Moore |first3=J. M. |last4=Schenk |first4=P. |last5=White |first5=O. L. |date=2015 |title=Reconstructing Helene's Surface History – Plastics and Snow |conference=46th Lunar and Planetary Science Conference |url=https://www.hou.usra.edu/meetings/lpsc2015/pdf/2400.pdf |access-date=2021-02-12}} * {{cite journal| doi=10.1126/science.1134681| last1=Verbiscer| first1=A.| last2=French| first2=R.| last3=Showalter| first3=M.| last4=Helfenstein| first4=P.| title=Enceladus: Cosmic Graffiti Artist Caught in the Act| journal=Science| volume=315| issue=5813| page=815| date=9 February 2007| pmid=17289992| bibcode=2007Sci...315..815V| s2cid=21932253}} (supporting online material, table S1) == External links == {{Commons category|Helene (moon)|Helene}} {{Spoken Wikipedia|Helene (moon).ogg|date=2010-02-06}} * [https://web.archive.org/web/20151120054640/http://solarsystem.nasa.gov/planets/profile.cfm?Object=Sat_Helene Helene Profile] by [http://solarsystem.nasa.gov NASA's Solar System Exploration]; see instead [https://web.archive.org/web/20140421054529/http://saturn.jpl.nasa.gov/science/moons/helene/ Cassini Solstice Mission: Helene] * [http://www.planetary.org/explore/topics/saturn/helene.html The Planetary Society: Helene] * [http://www.planetary.org/blog/article/00002385/ Helene has two faces] {{Webarchive|url=https://web.archive.org/web/20100616022007/http://planetary.org/blog/article/00002385/ |date=2010-06-16 }}—[[The Planetary Society]] : Helene Mini Atlas—Mar. 11, 2010 * [http://www.planetary.org/blog/article/00003072/ Cassini catches Helene] {{Webarchive|url=https://web.archive.org/web/20120401234936/http://www.planetary.org/blog/article/00003072/ |date=2012-04-01 }}—The Planetary Society : Video & Views—Jun. 20, 2011 {{Moons of Saturn|state=uncollapsed}} {{Saturn}} {{DEFAULTSORT:Helene (Moon)}} [[Category:Moons of Saturn]] [[Category:Trojan moons]] [[Category:Astronomical objects discovered in 1980|19800301]] [[Category:Moons with a prograde orbit]] [[Category:Helen of Troy]]
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