427P/ATLAS

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427P/ATLAS
File:Shape-Shifting Asteroid with a Comet-like Tail - Noaoann19003a.jpg
Comet 427P/ATLAS photographed from the WIYN Observatory (left) and the Hubble Space Telescope (right).[1]
Discovery[2]
Discovered byAren Heinze
Discovery siteATLASHKO (T05)
Discovery date27 September 2017
Designations
P/2017 S5, P/2021 L6
Orbital characteristics[4][5]
Epoch23 November 2017 (JD 2458080.5)
Observation arc3.89 years
Earliest precovery date11 September 2017
Number of
observations
438
Aphelion4.163 AU
Perihelion2.178 AU
Semi-major axis3.171 AU
Eccentricity0.31304
Orbital period5.646 years
Inclination11.849°
252.39°
Argument of
periapsis
99.944°
Mean anomaly20.594°
Last perihelion19 March 2023[3]
Next perihelion31 October 2028[3]
TJupiter3.092
Earth MOID1.210 AU
Jupiter MOID1.664 AU
Physical characteristics[6][7]
Mean radius
0.45 ± 0.06 km (0.280 ± 0.037 mi)
~1.4 hours
0.06±0.02
(V–R) = 0.43±0.05
Comet total
magnitude
(M1)
10.7
Comet nuclear
magnitude (M2)
15.8

427P/ATLAS is a periodic comet and an active asteroid with a 5.65-year orbit around the Sun. It is the second comet discovered by the Asteroid Terrestrial-impact Last Alert System after 478P/ATLAS.[8]

Orbit

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The comet orbits within the main asteroid belt at distances between 2.18 AU (326 million km) and 4.16 AU (622 million km) from the Sun.[4] Studies of its orbital trajectory revealed that it is highly likely a member of the Theobalda collisional family,[9] a group of asteroids formed from a large, shattered parent body about 7 million years ago.[10] The main-belt comets 455P/PANSTARRS and 483P/PANSTARRS also belong to this group.

Physical characteristics

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Like most of the main-belt comets, the observed activity from 427P/ATLAS is driven by the sublimation of water ice on its surface, which its mass loss rate is estimated to be about ~5.0±3.0 kg/sec-1 during its perihelion in 2017.[11]

Photometric observations from the Lisnyky Observatory showed that this comet has some notable instability of color, likely caused by the injection of fresh material to its coma.[6]

Observations from the Hubble Space Telescope in 2019 had determined that its nucleus has an effective radius of 0.450±0.060 km, assuming a geometric albedo of 0.06±0.02.[7][11]

References

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