Discovery[1] | |
---|---|
Discovered by | Siding Spring Observatory 0.5-m Schmidt (E12) |
Discovery date | 3 January 2013 |
Orbital characteristics[2][3][4] | |
Epoch | 30 October 2014 (JD 2456960.5) |
Observation arc | 3.53 years |
Number of observations | 449 |
Orbit type | Oort cloud |
Aphelion | 52000 AU (inbound) 13000 AU (outbound) |
Perihelion | 1.39875 AU (q) |
Eccentricity | 1.00043 |
Orbital period | several million years inbound (Barycentric solution for epoch 1950) ~500000 years outbound (Barycentric solution for epoch 2050) |
Inclination | 129.033° |
300.999° | |
Argument of periapsis | 2.449° |
Last perihelion | 25 October 2014 |
TJupiter | –0.919 |
Earth MOID | 0.3836 AU |
Jupiter MOID | 3.6748 AU |
Physical characteristics[2][5][6] | |
Dimensions | ~400–700 m (0.25–0.43 mi) |
Comet total magnitude (M1) | 8.5 |
Comet nuclear magnitude (M2) | 12.0 |
C/2013 A1 (Siding Spring) is an Oort cloud comet discovered on 3 January 2013 by Robert H. McNaught at Siding Spring Observatory using the 0.5-meter (20 in) Uppsala Southern Schmidt Telescope.[1][7]
At the time of discovery it was 7.2 AU from the Sun and located in the constellation Lepus. Comet C/2013 A1 probably took millions of years to come from the Oort cloud. After leaving the planetary region of the Solar System, the post-perihelion orbital period (epoch 2050) is estimated to be roughly 1 million years.[4]
C/2013 A1 passed the planet Mars very closely on 19 October 2014, at a distance of 140,496.6 ± 4.0 km (87,300.5 ± 2.5 mi; 0.000939162 ± 2.7×10−8 au).[8] After its discovery, there was thought to be a chance of a collision with Mars, but this possibility was excluded when its orbit was determined with about a 200-day observation arc.[9]
All NASA Mars orbiters—including 2001 Mars Odyssey,[10] Mars Reconnaissance Orbiter[11] and MAVEN[12]—as well as ESA's orbiter, Mars Express,[13] and ISRO's orbiter, the Mars Orbiter Mission,[14] reported a healthy status after the comet flyby on 19 October 2014.[15][16] During the flyby, orbiters around Mars detected thousands of kilograms per hour of comet dust composed of magnesium, iron, sodium, potassium, manganese, nickel, chromium and zinc.[17] In addition, the comet nucleus was determined to be between 400 and 700 meters (0.2 and 0.4 mi),[5][6][17] much smaller than originally assumed. The nucleus rotates once every eight hours.[18]
MPEC2013-A14
was invoked but never defined (see the help page).jpldata
was invoked but never defined (see the help page).MPEC2014-L52
was invoked but never defined (see the help page).barycenter
was invoked but never defined (see the help page).HiRISE141021
was invoked but never defined (see the help page).Swift
was invoked but never defined (see the help page).NYT-20140804
was invoked but never defined (see the help page).esa
was invoked but never defined (see the help page).NASA-20141019-ODY
was invoked but never defined (see the help page).NASA-20141019-MRO
was invoked but never defined (see the help page).NASA-20141019-MAV
was invoked but never defined (see the help page).ESA-20141020
was invoked but never defined (see the help page).ISRO MOM safe after Mars comet flyby
was invoked but never defined (see the help page).NASA-20141019
was invoked but never defined (see the help page).NYT-20141019
was invoked but never defined (see the help page).NYT-20141107-KC
was invoked but never defined (see the help page).JPL141107
was invoked but never defined (see the help page).