P/2020 MK4 (PanSTARRS)

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P/2020 MK4 (PanSTARRS)
Discovery
Discovered by Pan-STARRS 1
Discovery site Haleakala Obs.
Discovery date24 June 2020
Designations
2020 MK4
Chiron-type comet [1]
centaur [2]
Orbital characteristics [1]
Epoch 17 December 2020 (JD 2459200.5)
Uncertainty parameter 4
Observation arc 857 days (2.348 yr)
Aphelion 6.25417 AU (0.935611 Tm)
Perihelion 6.0253 AU (901.37 Gm)
6.14521 AU (0.919310 Tm)
Eccentricity 0.01952
15.23 yr (5564.22 d)
138.7°
0° 3m 52.917s / day
Inclination 6.72263°
1.446°
164.5°
Earth  MOID 5.03147 AU (752.697 Gm)
Jupiter  MOID 0.578149 AU (86.4899 Gm)
TJupiter 3.005
Physical characteristics
11.3 [1]

    P/2020 MK4 (PanSTARRS) is a Chiron-type comet or active centaur orbiting in the outer Solar System between Jupiter and Saturn. [3] It was discovered on 24 June 2020, by the Pan-STARRS survey at Haleakala Observatory in Hawaii, United States. [4]

    Contents

    Size

    A lower limit for the absolute magnitude of the nucleus is Hg = 11.30±0.03 that, for an albedo in the range 0.1—0.04, gives an upper limit for its size in the interval 23–37 km. [3]

    Colors

    The comet's color indices, (g′r′) = 0.42±0.04 and (r′i′) = 0.17±0.04, indicates the comet's nucleus has a neutral or gray color. [3]

    Activity

    P/2020 MK4 was discovered in outburst state and by late 2020, it had returned to its regular brightness. [5] [3] It was recovered by the Lowell Discovery Telescope at an extremely faint apparent magnitude of 24.5 in September 2022. [6] It was officially recognized as a comet by the Minor Planet Center on 20 November 2022, in which it was given the periodic comet designation P/2020 MK4. [7] [8]

    Orbital evolution

    Centaurs have short dynamical lives due to strong interactions with the giant planets. [9] P/2020 MK4 follows a very chaotic orbital evolution that may lead it to be ejected from the Solar System during the next 200,000 yr. [3] Extensive numerical simulations indicate that P/2020 MK4 may have experienced relatively close flybys with comet 29P/Schwassmann–Wachmann, in some cases with one of both objects were transient Jovian satellites; during these events, P/2020 MK4 may have crossed the coma of comet 29P when in outburst. [3]

    See also

    References

    1. 1 2 3 "JPL Small-Body Database Browser: 2020 MK4" (2020-06-06 last obs.). Jet Propulsion Laboratory . Retrieved 5 April 2021.
    2. "Orbit Fit and Astrometric record for 20MK4". Southwest Research Institute . Retrieved 11 August 2021. The Deep Ecliptic Survey Object Classifications
    3. 1 2 3 4 5 6 de la Fuente Marcos, C.; de la Fuente Marcos, R.; Licandro, J.; Serra-Ricart, M.; Martino, S.; de Leon, J.; Chaudry, F.; Alarcón, M. R. (13 May 2021). "The active centaur 2020 MK4". Astronomy & Astrophysics . 649 (1): A85 (15 pages). arXiv: 2104.01668 . Bibcode:2021A&A...649A..85D. doi:10.1051/0004-6361/202039117. S2CID   233024896.
    4. "MPEC 2020-N36: 2020 MK4". Minor Planet Electronic Circular. Minor Planet Center. 11 July 2020. Retrieved 5 April 2021.
    5. "2020 MK4 belatedly confirmed outburst". Minor Planet Mailing List . Retrieved 6 April 2021.
    6. "MPEC 2022-W16: 2020 MK4". Minor Planet Electronic Circular. Minor Planet Center. 16 November 2022. Retrieved 20 November 2022.
    7. "MPEC 2022-W78 : COMET P/2020 MK4 (PANSTARRS)". Minor Planet Electronic Circular. Minor Planet Center. 20 November 2022. Retrieved 20 November 2022.
    8. Green, Daniel W. E. (20 November 2022). "COMET P/2020 MK_4 (PANSTARRS)". Central Bureau Electronic Telegrams. Central Bureau for Astronomical Telegrams. Retrieved 20 November 2022.
    9. Horner, J.; Evans, N.W.; Bailey, M. E. (2004). "Simulations of the Population of Centaurs I: The Bulk Statistics". Monthly Notices of the Royal Astronomical Society . 354 (3): 798. arXiv: astro-ph/0407400 . Bibcode:2004MNRAS.354..798H. doi: 10.1111/j.1365-2966.2004.08240.x . S2CID   16002759.