(7888) 1993 UC
Discovery[1] | |
---|---|
Discovered by | Robert H. McNaught |
Discovery date | 20 October 1993 |
Designations | |
none | |
Apollo NEO[1] | |
Orbital characteristics[1] | |
Epoch 13 January 2016 (JD 2457400.5) | |
Aphelion | 4.0540 AU (606.47 Gm) (Q) |
Perihelion | 0.81827 AU (122.411 Gm) (q) |
2.4361 AU (364.44 Gm) (a) | |
Eccentricity | 0.66411 (e) |
3.80 yr (1388.8 d) | |
274.28° (M) | |
Inclination | 26.082° (i) |
165.92° (Ω) | |
323.07° (ω) | |
Physical characteristics | |
Dimensions | ~2.7 km (1.7 mi)[2] |
Equatorial escape velocity | ~1.3 m/s (3 mph) |
2.340 h (0.0975 d)[1] | |
U | |
14.1 (2013 peak)[3] | |
15.1[1] | |
|
(7888) 1993 UC is a near-Earth minor planet in the Apollo group.[1] It was discovered by Robert H. McNaught at the Siding Spring Observatory in Coonabarabran, New South Wales, Australia, on October 20, 1993.[1] The asteroid has an observation arc of 23 years and has a well determined orbit.[1] Its estimated size is 2.3 to 5.2 km.[4]
On March 20, 2013, the asteroid passed 49 lunar distances or 0.12598 AU (18,846,000 km; 11,711,000 mi) from Earth at a relative velocity of 21.8 km/s (49,000 mph).[1] The approach posed no threat to Earth. (7888) 1993 UC is not classified as a potentially hazardous asteroid (PHA) because its Earth MOID (Minimum Orbit Intersection Distance) is only 0.089 AU,[1] and only objects with an Earth MOID less than 0.05 AU are considered PHAs.[5]
It was discovered to be a binary asteroid by Arecibo Observatory in March 2013.[6]
On April 29, 2146, the asteroid will pass 0.0346 AU (5,180,000 km; 3,220,000 mi) from asteroid 4 Vesta.[1]
See also
References
- 1 2 3 4 5 6 7 8 9 10 11 "JPL Close-Approach Data: 7888 (1993 UC)". Retrieved 11 April 2016.
2012-11-25 last obs (arc=23 years)
- ↑ (E.A.R.N.) physical data for (7888) 1993UC
- ↑ "1993 UC Ephemerides for 20 March 2013". NEODyS (Near Earth Objects – Dynamic Site). Retrieved 2013-03-19.
- ↑ NASA "NEO Earth Close Approach Tables", Retrieved on 21 December 2012.
- ↑ NASA/JPL "NEO Program FAQ", Retrieved on 21 December 2012.
- ↑ Dr. Lance A. M. Benner (2013-11-18). "Binary and Ternary near-Earth Asteroids detected by radar". NASA/JPL Asteroid Radar Research. Retrieved 2014-03-01.