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Tinia (moon)

From Wikipedia, the free encyclopedia
Moon of 55637 Uni
Tinia
Hubble Space Telescope image of55637 Uni and its moon Tinia at 10 o'clock.
Discovery
Discovered byBrown et al.
Discovery dateAugust 2005
Designations
Designation
(55637) Uni I
Named after
Tinia
Orbital characteristics
4750±40 km[1]
Eccentricity0.17±0.03[2]
8.3095 d (prograde)[1]
Inclination63.1°[1]
Satellite of55637 Uni
Physical characteristics
105±15 km[3]
Uni + 2.5

Tinia is the only knownnatural satellite of thetrans-Neptunian object55637 Uni.

Discovery and naming

[edit]

Tinia was discovered in August 2005, by observations with theHubble Space Telescope, and announced on 22 February 2007.[4]It was named together with Uni on 1 September 2025 afterTinia, theEtruscan sky god and husband of the Etruscan goddess of love and fertilityUni.[5]

Physical characteristics

[edit]

Tinia was discovered at 0.16arcseconds from Uni with a difference inapparent magnitude of 2.5[6] Its diameter is estimated at210±30 km. Assuming analbedo similar to its primary, Tinia should have a diameter of approximately 190 km;[2] assuming an albedo of 0.05, typical of cool classical KBOs of similar size, it should have a diameter of approximately 260 km.[7]

Orbital characteristics

[edit]
A simulated circular orbit of Tinia at a distance of 4,770 km from Uni.

Tinia completes one complete orbit around Uni every8.309±0.0002 days, at a distance of4770±40 km, indicating a total system mass of(1.25±0.03)×1020 kg.[7][2] Its orbital eccentricity is0.17±0.03.[2]

References

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  1. ^abc"2002 UX25 System parameters". Will Grundy. Retrieved2023-08-29.
  2. ^abcd"(55637) Uni and Tinia".www.johnstonsarchive.net. Retrieved2025-09-06.
  3. ^"(55637) 2002 UX25". Retrieved28 July 2023.
  4. ^"IAUC 8812: Satellites of 2003 AZ_84, (50000), (55637), (90482); V1281 Sco; V1280 Sco".www.cbat.eps.harvard.edu. Retrieved2025-09-06.
  5. ^"WGSBN Bulletin (Vol. 5, No. 20)"(PDF).IAU. 2025-09-01. p. 6.
  6. ^"Αρχειοθετημένο αντίγραφο". Archived fromthe original on 2007-09-12. Retrieved2018-10-06.
  7. ^abM.E. Brown (2013). "The density of mid-sized Kuiper belt object 2002 UX25 and the formation of the dwarf planets".The Astrophysical Journal Letters.778 (2): L34.arXiv:1311.0553.Bibcode:2013ApJ...778L..34B.doi:10.1088/2041-8205/778/2/L34.S2CID 17839077.
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