(15789) 1993 SC

(15789) 1993 SC

Discovery
Discovered by	Iwan P. Williams, Alan Fitzsimmons, and Donal O'Ceallaigh
Discovery date	17 September 1993
Designations
MPC designation	(15789) 1993 SC
Alternative designations	none
Minor planet category	Plutino [1]
Orbital characteristics [2]
Epoch 13 January 2016 (JD 2457400.5)
Uncertainty parameter 3
Observation arc	5839 days (15.99 yr)
Aphelion	46.639  AU (6.9771  Tm)
Perihelion	32.162 AU (4.8114 Tm)
Semi-major axis	39.400 AU (5.8942 Tm)
Eccentricity	0.18372
Orbital period (sidereal)	247.32 yr (90333.4 d)
Mean anomaly	66.186°
Mean motion	0° 0m 14.347s / day
Inclination	5.1667°
Longitude of ascending node	354.75°
Argument of perihelion	316.20°
Earth  MOID	31.1475 AU (4.65960 Tm)
Jupiter  MOID	27.0752 AU (4.05039 Tm)
TJupiter	5.520
Physical characteristics
Mean diameter	328±60 km [2] 363 km [3]
Geometric albedo	0.022±0.010 [2]
Absolute magnitude (H)	7.0

(15789) 1993 SC is a trans-Neptunian object of the plutino class. The discovery was made in 1993 at the La Palma Observatory with the Isaac Newton Telescope. The object measures approximately 328 km in diameter. It was the second plutino to receive an MPC number. ^[1]

Other Kuiper belt objects discovered in 1993 include: (15788) 1993 SB, (181708) 1993 FW, (385185) 1993 RO and 1993 RP.

Orbit and classification

1993 SC orbits the Sun at a distance of 32.2-46.1 AU one per 247 Earth years (90,254 days, semi-major axis of 39.4 AU). Its orbit has an eccentricity of 0.183 and an inclination of 5.166° respective to the elliptic. Its observation arc begins with Mauna Kea Observatory in 1993. ^[4]

1993 SC is a trans-Neptunian object and belongs to the plutinos, an orbital class of objects named after their largest member, Pluto. These resonant trans-Neptunian objects stay in a 2:3 mean-motion orbital resonance with Neptune, orbiting exactly two times the sun for every three orbits Neptune does.

Numbering and naming

1993 SC was numbered by the Minor Planet Center on 26 July 2000, receiving the number 15789 in the minor planet catalog. ^[5] As of 2025 ^[update] , it has not been named. According to the established naming conventions, it will get a mythological name associated with the underworld.

Physical characteristics

1993 SC has a diameter of 328 km (204 mi) and a low geometric albedo of 0.022. ^[2] It also has a very red surface color (RR) in its visible spectrum, with B-V and V-R color indices of 1.27 and 0.70 respectively. ^[6] A red surface color is typically represented with the association of tholins, polymer-like organic compounds, formed by long exposures to solar and cosmic radiation. ^[6]

See also

• 15760 Albion
• List of trans-Neptunian objects
• Kuiper belt

References

1. "MPEC 2010-S44 :Distant Minor Planets (2010 OCT. 11.0 TT)". IAU Minor Planet Center. 2010-09-25. Retrieved 2014-11-16.
2. "15789 (1993 SC)". JPL Small-Body Database . NASA/Jet Propulsion Laboratory . Retrieved 8 April 2016.
3. List of known trans-Neptunian objects at Johnston's Archive
4. "(15789) = 1993 SC". Minor Planet Center. Retrieved 24 January 2025.
5. "M.P.C. 40992" (PDF). Minor Planet Circulars. Minor Planet Center. 26 July 2000. Retrieved 24 January 2025.
6. Tegler, S. C.; Romanishin, W. (March 1997). "The Extraordinary Colors of Trans-Neptunian Objects 1994 TB and 1993 SC". Icarus. 126 (1): 212–217. Bibcode:1997Icar..126..212T. doi:10.1006/icar.1996.5646.

External links

• MPC: List of TNOs
• Grundy, W. M.; Noll, K. S.; Stephens, D. C. "Diverse albedos of small trans-neptunian objects." Icarus, Volume 176, Issue 1, p. 184-191 (07/2005) Abstract
• (15789) 1993 SC at the JPL Small-Body Database
  • Close approach  · Discovery  · Ephemeris  · Orbit viewer  · Orbit parameters  · Physical parameters