Inuit group#S/2019 S 24

{{Short description|Category of satellites of Saturn}}

File:Animation of Saturn's Inuit group of satellites.gif}}{{·}}{{legend2|Lime| Ijiraq}}{{·}}{{legend2|Gold| Paaliaq}}{{·}}{{legend2|OrangeRed| Siarnaq}}{{·}}{{legend2|Cyan|Tarqeq}}]]

File:Saturn irregular moon orbits a vs. i.png, those above 90° are retrograde. The X-axis is labeled in terms of Saturn's Hill radius.]]

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){{Cite journal |last1=Grav |first1=Tommy |last2=Holman |first2=Matthew J. |author-link2=Matthew J. Holman |last3=Gladman |first3=Brett |author-link3=Brett J. Gladman |last4=Aksnes |first4=Kaare |author-link4=Kaare Aksnes |date=November 2003 |title=Photometric Survey of the Irregular Satellites |journal=Icarus |volume=166 |issue=1 |pages=33–45 |doi=10.1016/j.icarus.2003.07.005 |arxiv=astro-ph/0301016 |bibcode=2003Icar..166...33G }} and similar infrared spectra.{{Cite journal |last1=Grav |first1=Tommy |last2=Holman |first2=Matthew J. |author-link2=Matthew J. Holman |date=2004-04-20 |title=Near-Infrared Photometry of Irregular Satellites of Jupiter and Saturn |journal=The Astrophysical Journal |volume=605 |issue=2 |pages=L141–L144 |doi=10.1086/420881 |issn=0004-637X |arxiv=astro-ph/0312571 |bibcode=2004ApJ...605L.141G }} 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.{{Cite journal |last1=Grav |first1=Tommy |last2=Bauer |first2=James |author-link2=James Bauer (astronomer) |date=2007-11-01 |title=A deeper look at the colors of the Saturnian irregular satellites |journal=Icarus |volume=191 |issue=1 |pages=267–285 |doi=10.1016/j.icarus.2007.04.020 |arxiv=astro-ph/0611590 |bibcode=2007Icar..191..267G }}

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.