Astronomy:Inuit group
The Inuit group is a dynamical grouping of the prograde irregular satellites of Saturn which follow similar orbits. Their semi-major axes range between 11 and 19 Gm, their inclinations between 45° and 50°, and their eccentricities between 0.11 and 0.39. They take an average of 2 years to orbit Saturn.
The International Astronomical Union (IAU) uses names taken from Inuit mythology for these moons.
The group appeared quite homogeneous in early observations, the satellites displaying light-red colour (colour indices B−V = 0.79 and V−R = 0.51, similar to that of the Gallic group)[1] and similar infrared spectra.[2] Recent observations, however, revealed that Ijiraq is distinctly redder than Paaliaq, Siarnaq and Kiviuq. In addition, unlike the other three, Ijiraq's spectrum does not display weak absorption near 0.7 μm. This feature is attributed to a possible water hydration.[3]
The spectral homogeneity (with the exception of Ijiraq) is consistent with a common origin in the break-up of a single object but the dispersion of the orbital parameters requires further explanation. Recently reported secular resonances among the members could provide the explanation of the post-collisional dispersion.
Names
The twelve known members of the Inuit group are (sorted by distance from Saturn in their respective subgroups):
| Name | Diameter (Km) | Period (days)[4] |
|---|---|---|
| S/2019 S 1 | 6 | 445.51 |
| Kiviuq | 19 | 449.13 |
| S/2005 S 4 | 5 | 450.22 |
| S/2020 S 1 | 4 | 451.10 |
| Ijiraq | 15 | 451.46 |
| Paaliaq | 30 | 687.08 |
| S/2004 S 31 | 5 | 866.10 |
| Tarqeq | 7 | 884.98 |
| S/2019 S 14 | 4 | 893.14 |
| Siarnaq | 39.3 | 895.87 |
| S/2020 S 3 | 3 | 907.99 |
| S/2020 S 5 | 3 | 933.88 |
In addition, S/2019 S 6 has also been categorized in the Inuit group by some sources.[lower-alpha 1]
See also
Notes
- ↑ JPL's mean orbital elements suggest an inclination that is similar to those of the Gallic group; however other sources say it belongs to the Inuit group.
References
- ↑ Grav, Tommy; Holman, Matthew J.; Gladman, Brett; Aksnes, Kaare (November 2003). "Photometric Survey of the Irregular Satellites". Icarus 166 (1): 33–45. doi:10.1016/j.icarus.2003.07.005. http://arxiv.org/abs/astro-ph/0301016.
- ↑ Grav, Tommy; Holman, Matthew J. (2004-04-20). "Near-Infrared Photometry of Irregular Satellites of Jupiter and Saturn". The Astrophysical Journal 605 (2): L141–L144. doi:10.1086/420881. ISSN 0004-637X. http://arxiv.org/abs/astro-ph/0312571.
- ↑ Grav, Tommy; Bauer, James (2007-11-01). "A deeper look at the colors of the Saturnian irregular satellites". Icarus 191 (1): 267–285. doi:10.1016/j.icarus.2007.04.020. http://arxiv.org/abs/astro-ph/0611590.
- ↑ "Planetary Satellite Mean Elements". Jet Propulsion Laboratory. California Institute of Technology. 25 January 2024. https://ssd.jpl.nasa.gov/sats/elem/.
External links
Mean orbital parameters: from JPL
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