Discovery

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][4] 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.[3]

C/2013 A1 passed the planet Mars very closely on 19 October 2014. 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 more accurately.

All NASA Mars orbiters—including Mars Odyssey Orbiter,[5] Mars Reconnaissance Orbiter[6] and MAVEN[7]—as well as, ESA's orbiter, Mars Express,[8] and ISRO's satellite, the Mars Orbiter Mission,[9] reported a healthy status after the comet flyby on 19 October 2014.[10][11]

Contents [hide]

1 Discovery

2 Encounter with Mars

2.1 Predicted effects

2.2 Hypothetical impact

3 Observation

4 Gallery

4.1 Before comet flyby

4.2 During comet flyby

5 References

6 External links

Discovery[edit]

The comet was discovered on 3 January 2013 by professional astronomer Robert McNaught at the Siding Spring Observatory at Coonabarabran NSW Australia and received the official designation C/2013 A1.[1] The comet was named Siding Spring based on a tradition to identify the observatory that discovered it. Three images were obtained through the use of a CCD camera mounted on the Uppsala Southern Schmidt Telescope with a spherical mirror of 0.5 meters in diameter. The comet appeared as an object of apparent magnitude 18.4 to 18.6. At the time of discovery, the comet was 7.2 AU (1.08×109 km; 670,000,000 mi) from the Sun.

Precovery images by the Catalina Sky Survey from 8 December 2012 were found quickly and announced with the discovery giving the comet a 29-day observation arc.[1] On 3 March 2013, Pan-STARRS precovery images from 4 October 2012 were announced that extended the observation arc to 148 days.[12]

Comet Siding Spring Mars flyby on 19 October 2014 (artist's concepts)

Orbiters take cover from Comet Siding Spring during Mars flyby

Mars as seen from Comet Siding Spring

Comet Siding Spring as seen from Mars

Encounter with Mars[edit]

Comet Siding Spring passed extremely close to Mars on 19 October 2014 at 18:28 ± 0:01 UTC.[13] Initial observations by Leonid Elenin on 27 February 2013, suggested that it might pass 0.000276 AU (41,300 km; 25,700 mi) from the center of Mars.[14] With an observation arc of 733 days, the nominal pass is 0.000931 AU (139,300 km; 86,500 mi) from the center-point of Mars and the uncertainty region shows that it would not come closer than 0.000927 AU (138,700 km; 86,200 mi).[13]

For comparison, Mars's outer moon Deimos orbits it at a distance of 0.00016 AU (24,000 km; 15,000 mi). Due to the uncertainty region, there was the possibility that it could pass Mars as far away as 0.000934 AU (139,700 km; 86,800 mi). It passed Mars at a relative velocity of 56 km/s (35 mi/s).[13] As seen from Mars, C/2013 A1 peaked at approximately apparent magnitude −6.[15]

Comet Siding Spring encounter with Mars, 19 October 2014

Projected position of Comet Siding Spring and its closest approach to Mars.

Comet Siding Spring encounter

[show]

JPL Small-Body Database uncertainty region for close approach to Mars on 19 October 2014

Predicted effects[edit]

The main body of the comet's tail is projected to miss Mars by some 10 Mars diameters.[18] As a result, only higher than average velocity meteoroid dust, ejected earlier in the approach of the comet, allow for impacts on Mars, its moons, and orbiting spacecraft. Dust particles ejected from the nucleus of the comet, at more than double the expected velocity when the comet was 3 AU from the Sun, could reach Mars approximately 43 to 130 min after the closest approach of the comet.[19] There is a possibility for millimeter to centimeter size particles released more than 13 AU from the Sun, however, this is considered unlikely,[19] although massive ejections from farther out have been deduced.[20]

Comet Siding Spring as seen by NEOWISE on 16 January 2014

In 2013 it was thought possible that Comet Siding Spring would create a meteor shower on Mars or be a threat to the spacecraft in Mars orbit.[21] Studies in 2014 showed the threat to orbiting spacecraft to be minimal.[22] The greatest threat would be about 100 minutes after closest approach.[22] Mars passed about 27,000 km (17,000 mi) from the comet's orbit around 20:10 UT.[23]

The coma of the comet is projected to more than double the amount of hydrogen in the high atmosphere for a period of several tens of hours and to warm it by about 30 K for a few hours—the combination increasing the effect of atmospheric drag on Mars Reconnaisance Orbiter and MAVEN spacecrafts causing a measurable increase in orbital decay because of atmospheric ram pressure.[24] These spacecraft will be approaching Mars to minimum altitudes of 250 km and 150 km and orbital periods of 3 and 4 hours, respectively. The amount of drag cannot be narrowed down greatly until the production rate of the comet is known, but it could be from 1.6 to 40 times normal drag. MAVEN, in particular, also has instruments to observe any changes to the gas composition of the atmosphere. The closest orbiting moon of Mars, Phobos, orbits far higher at a minimum distance of 9,234.42 km (5,738.00 mi)[25] more than 10 times the height of Mars' atmosphere.[26]

Hypothetical impact[edit]

Hypothetical comet impact at 56 km/s

into sedimentary rock[27]

Impactor

diameter Kinetic energy Crater

diameter

3 km (1.9 mi) 5.3 million Mt 45 km (28 mi)

5 km (3.1 mi) 24.5 million Mt 71 km (44 mi)

8 km (5.0 mi) 100 million Mt 108 km (67 mi)

15 km (9.3 mi) 660 million Mt 188 km (117 mi)

20 km (12 mi) 1.57 billion Mt 242 km (150 mi)

50 km (31 mi) 24 billion Mt 544 km (338 mi)

Estimates for the diameter of the nucleus have varied from 1 to 50 km (1 to 31 mi),[28][29] but now the nucleus is known to be only approximately 700 meters (0.4 mi) in diameter,[30] roughly twice the diameter of asteroid 2010 XG11 that approached Mars on 29 July 2014.[31] Based on early upper-limit size estimates, the resulting upper-limit energy of a hypothetical impact with Mars

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