Chrysalis (hypothetical moon) and Saturn's rings

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Chrysalis (hypothetical moon)

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From Wikipedia, the free encyclopedia

Hypothetical moon of Saturn

Chrysalis was a hypothetical former moon of Saturn, named in 2022 by scientists of the Massachusetts Institute of Technology using data from the Cassini–Huygens mission.[1] The moon is hypothesized to have been torn apart by Saturn's tidal forces, somewhere between 200 and 100 million years ago. Up to 99% of the moon's mass would have been swallowed by Saturn, with the remaining 1% forming the rings of Saturn.[2] The origin of Saturn's rings from the destruction of a satellite has been previously proposed by other authors.[3]

Chrysalis was hypothesized to be similar in size and mass to Iapetus, with a similar water-ice composition, and to have orbited somewhere between Iapetus and Titan. Its orbit around Saturn may have been degraded as a result of Titan's orbit expanding due to interactions of the Saturnian system with a resonance with Neptune, resulting in the increasing eccentricity of Chrysalis's orbit until being torn apart during a close encounter with Saturn by its parent planet's gravitational force.[4]

The hypothetical moon was named after the pupa stage of a butterfly, with the rings of Saturn representing its emergence from the chrysalis.[4]

See also<br>[edit]

List of hypothetical Solar System objects

Rings of Saturn § Formation and evolution of main rings

Phaeton

References<br>[edit]

↑ "Saturn's rings could have come from a destroyed moon named Chrysalis". New Scientist. 15 September 2022.

↑ Wisdom, Jack; Dbouk, Rola; Militzer, Burkhard; Hubbard, William B.; Nimmo, Francis; Downey, Brynna G.; French, Richard G. (September 16, 2022). "Loss of a satellite could explain Saturn's obliquity and young rings". Science. 377 (6612): 1285–1289. Bibcode:2022Sci...377.1285W. doi:10.1126/science.abn1234. hdl:1721.1/148216. PMID 36107998. S2CID 252310492.

↑ Charnoz, Sébastien; Morbidelli, Alessandro; Dones, Luke; Salmon, Julien (February 2009). "Did Saturn's rings form during the Late Heavy Bombardment?". Icarus. 199 (2): 413–428. arXiv:0809.5073. Bibcode:2009Icar..199..413C. doi:10.1016/j.icarus.2008.10.019. ISSN 0019-1035. S2CID 119229648.

1 2 Dunham, Will (15 September 2022). "Violent death of moon Chrysalis may have spawned Saturn's rings". Reuters. Retrieved 17 September 2022.

Further reading<br>[edit]

https://www.hou.usra.edu/meetings/lpsc2026/pdf/1132.pdf

Moons of Saturn<br>Listed in approximate increasing distance from Saturn<br>Inner ring moons<br>S/2009 S 1

Pan

Daphnis

Atlas

Prometheus

Pandora

+1 moon

Co-orbitals<br>Epimetheus

Janus

Ring-embedded moons<br>Aegaeon

Methone

Anthe

Pallene

Major moons<br>(with trojans)<br>Mimas

Enceladus

Tethys<br>Telesto

Calypso

Dione<br>Helene

Polydeuces

Rhea

Titan

Hyperion

Iapetus

Inuit group (39)<br>Kiviuq subgroup (23)<br>S/2019 S 1

Kiviuq

Ijiraq

+20 moons

Paaliaq<br>Paaliaq

Siarnaq subgroup (15)<br>S/2004 S 31

Tarqeq

Siarnaq

S/2020 S 5

+11 moons

Gallic group (19)<br>Albiorix

Bebhionn

Saturn LX

Erriapus

Tarvos

S/2020 S 4

S/2006 S 12

S/2004 S 24

+11 moons

Norse group (210)<br>Low-inclination (15)<br>Skathi

Hyrrokkin

Narvi

Bestla

+11 moons

Kari subgroup (16)<br>S/2006 S 1

Farbauti

S/2006 S 3

Kari

Geirrod

S/2004 S 21

S/2004 S 36

+9 moons

Mundilfari subgroup (146)<br>S/2004 S 37

Skoll

S/2004 S 13

Mundilfari

Gridr

Bergelmir

Jarnsaxa

Hati

S/2004 S 17

S/2004 S 12

Eggther

Aegir

Beli

Gunnlod

Saturn LXVII

S/2005 S 5

S/2004 S 28

Fenrir

Surtur

Loge

S/2004 S 39

Thiazzi

Saturn LXIV

Fornjot

+122 moons

Phoebe subgroup (33)<br>Phoebe

S/2006 S 20

S/2006 S 9

S/2007 S 2

Greip

Suttungr

S/2007 S 3

Thrymr

Angrboda

Gerd

Skrymir

Alvaldi

Ymir

Saturn LVIII

+19 moons

See also<br>Rings of Saturn

Moonlets<br>S/2004 S 3

S/2004 S 4

S/2004 S 6

Peggy

Bleriot

Earhart

Santos-Dumont

Cassini–Huygens

In fiction

Chiron

Chrysalis

Themis

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