Siarnaq

Siarnaq, also designated Saturn XXIX, is a prograde irregular satellite of Saturn. It was discovered at the Mauna Kea Observatory by astronomers Brett Gladman and John Kavelaars in 2000, and given the temporary designation S/2000 S 3.[2] It was named after Siarnaq, the Inuit goddess of the sea, it is the largest member of the Inuit group of irregular satellites.[10][7]

Siarnaq
Composite of three images taken by the Cassini spacecraft in 2013, showing Siarnaq's location at ten-minute intervals[lower-alpha 1]
Discovery[1][2]
Discovered byBrett J. Gladman
John J. Kavelaars[lower-alpha 3]
Discovery siteMauna Kea Obs.
Discovery date23 September 2000
Designations
Designation
Saturn XXIX
Pronunciation/ˈsiːɑːrnɑːk/
Named after
Siarnaq (Inuit mythology)
S/2000 S 3
AdjectivesSiarnaupian, Siarnaqian[lower-alpha 4]
Orbital characteristics[3][4]
Epoch 17 December 2020 (JD 2459200.5)
Observation arc18.78 yr (6,860 days)
0.1187382 AU (17,763,000 km)
Eccentricity0.5293834
+2.42 yr (+883.87 d)
35.08520°
Inclination43.80073° (to ecliptic)
40.96116°
79.59603°
Satellite ofSaturn
GroupInuit group
Physical characteristics
Mean diameter
39.3±5.9 km[5]
10.18785±0.00005 h[6][7]
98°±15°[7]
−23°±15°[7]
Albedo0.050±0.017[5]
Spectral type
D (reddish)[8]
B−V=0.87±0.01[8]
V−R=0.48±0.01
V−I=1.03±0.01
19.9 (R)[9]
10.9±0.05[5]

    Discovery
    Discovery images of Siarnaq taken by the CFHT in September 2000

    Siarnaq was discovered by Canadian astronomers Brett Gladman and John Kavelaars at the Mauna Kea Observatory on 23 September 2000. The discovery of Siarnaq formed part of an observational campaign to search for distant irregular satellites around Saturn. The campaign was coordinated by Gladman in late 2000 and consisted of an international team of eight astronomers[lower-alpha 2] using various ground-based telescopes with CCD cameras to survey Saturn's Hill sphere, the region within which satellites can have stable orbits around the planet.[12][13]

    On 23 September 2000 Gladman and Kavelaars conducted a wide-area survey down to a limiting magnitude of 24.5 with the 3.6-meter Canada-France-Hawaii Telescope (CFHT) at the Mauna Kea Observatory in Hawaii.[14] They reobserved their previous irregular satellite discoveries (Ymir and Paaliaq) identified two new irregular satellite candidates needing further confirmation: Siarnaq and Tarvos.[15] Siarnaq, the brighter of the two, was detected at an apparent magnitude of 20.[2]

    Follow-up and confirmation
    Offset plot showing the positions and ephemerides of 13 irregular satellites relative to Saturn in 2001. Siarnaq (S/2000 S 3) is located at the upper left from the center.

    Between 25–29 September 2000, follow-up observations of Siarnaq and other newly-discovered Saturnian irregular satellites were made at various observatories.[16] Preliminary orbit calculations ruled out the possibility that the satellites could be foreground asteroids and confirmed they were indeed orbiting Saturn.[15] The discovery of Ymir, Paaliaq, Siarnaq, and Tarvos were formally reported by the International Astronomical Union on 25 October 2000[2][17] and announced by Gladman's team a day later at a meeting hosted by the American Astronomical Society's Division for Planetary Sciences.[13] The discovery of the four satellites raised Saturn's known moons to 22, surpassing Uranus's moon count of 21 at the time.[15]

    Although Siarnaq was confirmed as a satellite, its orbit was poorly known due to an insufficient number of observations.[18] The moon was reobserved by the Kitt Peak National Observatory in December 2000,[19] and later by the Palomar and La Palma observatories in early 2001.[16] In the interim, Gladman's team had discovered eight more irregular satellites of Saturn, six of which were found in CFHT images from September 2000.[14] By February 2001, the team surveyed 90 percent of Saturn's Hill sphere down to a limiting magnitude of 23 and discovered a total of 12 irregular satellites around Saturn, raising the planet's number of known moons to 30 and resultingly overtaking Jupiter as the planet with the most known moons until 2003.[12][20]

    Name

    The moon is named after Siarnaq, the Inuit sea giantess or goddess and ruler of the Inuit underworld.[21] In other variants of Inuit legend, she is also known by other names such as Nuliajuk and Sedna. Siarnaq is said to reside at the bottom of the ocean and to have conceived all sea life, which she will withhold from Inuit hunters when angered. In some versions of Inuit legend, Siarnaq was once a beautiful maiden who was tricked into marrying a bird-man and then was rescued by her father. They came under attack by a storm, which provoked the girl's desperate father to throw her overboard and crop off her fingers in order to save himself.[22]

    The moon received its name in a formal notice published by the IAU on 8 August 2003, one month after its approval by the IAU's Working Group for Planetary System Nomenclature in a general assembly held in July 2003.[22] Siarnaq was also assigned the Roman numeral designation Saturn XXIX, the 29th moon of Saturn.[10]

    Background

    The moon was given the provisional designation S/2000 S 3 in its discovery announcement.[lower-alpha 5] The provisional designation indicates that it was the third Saturnian satellite identified in images taken in 2000.[2] Siarnaq is among the first Saturnian irregular satellites discovered since Phoebe in 1898; the discovery of new satellite groups of Saturn provided the opportunity for their discoverers to establish new naming conventions for each of them.[12][22]

    Kavelaars was advised by his colleagues to propose names from different cultures other than those from the traditional Greco-Roman mythology theme for Jovian and Saturnian moons. Throughout late 2000, Kavelaars spent several months consulting Amerindian scholars for appropriate name suggestions that were both multicultural and Canadian in origin. In March 2001, he was reading the Inuit tale Hide and Sneak to his children and had a revelation. He contacted the author of the tale, Michael Kusugak, to get his assent, and the latter suggested the names Kiviuq and Sedna.[23] Kavelaars then decided that the selected Inuit names should end in the letter q to distinguish the group—hence the name Sedna was changed to Siarnaq.[22] The former name was later used for 90377 Sedna, a distant trans-Neptunian object discovered in 2003.[21]

    I sent [Kavelaars] that bit about Siarnaq, or we call her Nuliajuk, that creature that lives under the sea, who's also know [sic] as Sedna. She's got so many names ... sometimes she's simply called the Old Woman Who Lives Down There. Anyway, I was talking about the realm of the shaman in this book, and I said, "And the only person who can go down there and comb her hair and make her feel better is the shaman Paaliaq." And this was just something I made up in my story. So I was really surprised when the final approved list of names of these four moons of Saturn included Paaliaq, because I just made him up. That was fun.

    — Michael Kusugak, in a Windspeaker interview[22]

    Physical characteristics

    Diameter and albedo
    Siarnaq observed in the infrared by the WISE spacecraft in 2010

    From infrared observations by the Wide-field Infrared Survey Explorer (WISE) spacecraft, Siarnaq is estimated to be 39.3 km (24.4 mi) in diameter.[5]

    Color

    It is light red in color, and the Siarnaupian (Siarnaqan)[lower-alpha 4] spectrum in the infrared is very similar to the Inuit-group satellites Paaliaq and Kiviuq, supporting the thesis of a possible common origin in the break-up of a larger body.[8][14][24]

    Shape and rotation
    Siarnaq as observed by Cassini from a distance of 22 million km (14 million mi)

    The rotation period of Siarnaq was measured by the Cassini spacecraft to be 10.19 hours; this is the shortest rotation period of all prograde irregular moons of Saturn.[6] Siarnaq displays a light curve with three maxima and minima over a full rotation, implying a roughly triangular shape.[7] From Cassini observations of Siarnaq at different phase angles, the orientation of its north rotational pole has been determined to be pointing toward 98° ecliptic latitude and −23° ecliptic longitude.[lower-alpha 6] This corresponds to a sideways axial tilt, indicating that Siarnaq experiences long, extreme seasons similar to the planet Uranus.[7]

    Orbit
    Siarnaq - Saturn XXIX
    Mean orbital elements [26]
    Epoch 1 January 2000 (JD 2451544.5)
    Semi-major axis0.1215392 AU (18,182,000 km)
    Eccentricity0.2802
    Inclination45.809° *
    Orbital period+2.45 yr (+895.51 d)
    Apsidal precession period457.40 yr
    Nodal precession period454.20 yr
    Irregular prograde groups of satellites of Saturn: Inuit (blue) and Gallic (red). The eccentricity of the orbits is represented by the yellow segments extending from the pericentre to the apocentre.
    Animation of Saturn's Inuit group of satellites from 2018–2027
      Kiviuq ·   Ijiraq ·   Paaliaq ·   Siarnaq ·   Tarqeq

    Siarnaq orbits Saturn at an average distance of 17.9 million km (11.1 million mi) in 897 days (2.5 years).[3] The moon has been found to be in a secular resonance with Saturn, involving the precession of its periapsis and that of the planet.[27][lower-alpha 7]

    The studies of these resonances are key to understand the capture mechanism for the irregular satellites and, assuming a common origin of a given dynamical group in the break-up of a single body, to explain today's dispersion of the orbital elements.

    Notes
    1. Merger of three images, colored red, green, and blue respectively, to highlight Siarnaq as it moves relative to the background stars.
    2. Brett J. Gladman, John J. Kavelaars, Jean-Marc Petit, Hans Scholl, Matthew Holman, Brian G. Marsden, Phil Nicholson and Joseph A. Burns.[11]
    3. The Jet Propulsion Laboratory's Solar System Dynamics page credits the discovery to Gladman and Kavelaars[1] while the International Astronomical Union's Gazetteer of Planetary Nomenclature credits the team of astronomers involved in the survey.[lower-alpha 2]
    4. The genitive form of Siarnaq is Siarnaup. Thus the adjectival form could be absolutive Siarnaqian or genitive Siarnaupian, parallel to nominative Venusian and genitive Venerian for Venus. See Inuktitut morphology
    5. Gladman's astrometry page for Siarnaq notes that the moon was temporarily given the designation S/2000 S 2 before being renumbered to S 3 in the discovery announcement.[16]
    6. For geocentric equatorial coordinates, the north pole orientation of Siarnaq is RA = 97°±15°, Dec = 0°±15°.[25]
    7. The ecliptic longitudes of the periapsis of the satellite and the planet are locked.

    References
    1. "Planetary Satellite Discovery Circumstances". Jet Propulsion Laboratory. 28 October 2019. Retrieved 27 July 2020.
    2. Marsden, Brian G. (25 October 2000). "IAUC 7513: S/2000 S 3, S/2000 S 4". International Astronomical Union Circular. International Astronomical Union (7513): 1. Bibcode:2000IAUC.7513....1G. Retrieved 27 July 2020.
    3. "M.P.C. 127090" (PDF). Minor Planet Circular. Minor Planet Center. 17 November 2020. Retrieved 6 February 2021.
    4. "Orbital Elements for Siarnaq (SXXIX=2000S3)". Horizons output. Jet Propulsion Laboratory. Retrieved 6 February 2021. ("Ephemeris Type" select "Orbital Elements"  · "Center" Saturn System Barycenter [500@6]  · Set "Time Span" to 2020-Dec-17)
    5. Grav, T.; Bauer, J. M.; Mainzer, A. K.; Masiero, J. R.; Nugent, C. R.; Cutri, R. M.; et al. (August 2015). "NEOWISE: Observations of the Irregular Satellites of Jupiter and Saturn". The Astrophysical Journal. 809 (1): 9. arXiv:1505.07820. Bibcode:2015ApJ...809....3G. doi:10.1088/0004-637X/809/1/3. S2CID 5834661. 3.
    6. Denk, Tilmann; Mottola, Stefano (April 2019). Schenk, Paul M.; et al. (eds.). "Studies of irregular satellites: I. Lightcurves and rotation periods of 25 Saturnian moons from Cassini observations". Icarus. 322: 80–102. Bibcode:2019Icar..322...80D. doi:10.1016/j.icarus.2018.12.040.
    7. Denk, T.; Mottola, S.; Bottke, W. F.; Hamilton, D. P. (2018). "The Irregular Satellites of Saturn". Enceladus and the Icy Moons of Saturn (PDF). 322. University of Arizona Press. pp. 409–434. Bibcode:2018eims.book..409D. doi:10.2458/azu_uapress_9780816537075-ch020. ISBN 9780816537488.
    8. Grav, Tommy; Bauer, James (November 2007). "A deeper look at the colors of the saturnian irregular satellites". Icarus. 191 (1): 267–285. arXiv:astro-ph/0611590. Bibcode:2007Icar..191..267G. doi:10.1016/j.icarus.2007.04.020. S2CID 15710195.
    9. "Planetary Satellite Physical Parameters". Jet Propulsion Laboratory. 19 February 2015. Retrieved 27 July 2020.
    10. Green, Daniel W. E. (8 August 2003). "IAUC 8177: Sats OF (22); Sats OF JUPITER, SATURN, URANUS". International Astronomical Union Circular. International Astronomical Union. Bibcode:2000IAUC.7513....1G. Retrieved 27 July 2020.
    11. "Planet and Satellite Names and Discoverers". Gazetteer of Planetary Nomenclature. USGS Astrogeology Science Center. Retrieved 30 July 2020.
    12. "The Irregular Satellites: Chips Off Older Blocks". Observatoire de la Cote d'Azur. 12 July 2001. Archived from the original on 21 November 2001. Retrieved 31 July 2020.
    13. Brand, David (26 October 2000). "Satellite-hunters find four new moons of the planet Saturn". Cornell Chronicle. Cornell University. Archived from the original on 11 December 2000. Retrieved 29 July 2020.
    14. Gladman, Brett; Kavelaars, J. J.; Holman, Matthew; Nicholson, Philip D.; Burns, Joseph A.; Hergenrother, Carl W.; et al. (July 2001). "Discovery of 12 satellites of Saturn exhibiting orbital clustering". Nature. 412 (6843): 163–166. Bibcode:2001Natur.412..163G. doi:10.1038/35084032. PMID 11449267. S2CID 4420031.
    15. "Saturn Swarming with Satellites". Observatoire de la Cote d'Azur. 26 October 2000. Archived from the original on 9 December 2000. Retrieved 29 July 2020.
    16. Gladman, Brett J. (January 2003). "Known astrometry of S/2000 S 3". Observatoire de la Cote d'Azur. Retrieved 2 August 2020.
    17. Marsden, Brian G. (25 October 2000). "IAUC 7512: S/2000 S 1, S/2000 S 2". International Astronomical Union Circular. International Astronomical Union (7512): 1. Bibcode:2000IAUC.7512....1G. Retrieved 27 July 2020.
    18. Marsden, Brian G. (18 November 2000). "IAUC 7521: S/2000 S 5, S/2000 S 6". International Astronomical Union Circular. International Astronomical Union (7521): 1. Bibcode:2000IAUC.7521....1G. Retrieved 2 August 2020.
    19. Marsden, Brian G. (19 December 2000). "MPEC 2000-Y14 : S/2000 S 3, S/2000 S 4, S/2000 S 5, S/2000 S 6, S/2000 S 10". Minor Planet Electronic Circular. Minor Planet Center.
    20. Hamilton, Douglas P. (12 July 2001). "Saturn saturated with satellites". Nature. 412 (6843): 132–133. Bibcode:2001Natur.412..132H. doi:10.1038/35084310. PMID 11449251. S2CID 4346912. Retrieved 31 July 2020.
    21. "Siarnaq In Depth". Solar System Exploration. NASA. 19 December 2019. Retrieved 5 August 2020.
    22. Petten, Cheryl (2003). "Naming Saturn's moons". Windspeaker. 21 (7). Aboriginal Multi-Media Society. p. 32. Retrieved 2 August 2020.
    23. Spitzer, Aaron (27 July 2001). "Inuktitut travels to the planets". Nunatsiaq News. Retrieved 5 August 2020.
    24. Grav, Tommy; Holman, Matthew J.; Gladman, Brett J.; Asknes, Kaare (November 2003). "Photometric survey of the irregular satellites". Icarus. 166 (1): 33–45. arXiv:astro-ph/0301016. Bibcode:2003Icar..166...33G. doi:10.1016/j.icarus.2003.07.005. S2CID 7793999.
    25. Denk, Tilmann (19 October 2019). "Siarnaq (S/2000 S 3)". Tilmann's Web Site. Retrieved 27 July 2020.
    26. "Planetary Satellite Mean Orbital Parameters". Jet Propulsion Laboratory. 17 July 2020. Retrieved 6 February 2021.
    27. Ćuk, Matija; Burns, Joseph A. (November 2004). "On the Secular Behavior of Irregular Satellites". The Astronomical Journal. 128 (5): 2518–2541. arXiv:astro-ph/0408119. Bibcode:2004AJ....128.2518C. doi:10.1086/424937. S2CID 18564122.
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