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2020 PP1 is a sub-kilometer asteroid, classified as a near-Earth object of the Apollo group, that is a temporary quasi-satellite of the Earth. There are over a dozen known Earth quasi-satellites, some of which switch periodically between the quasi-satellite and horseshoe co-orbital states.[6]

2020 PP1
Discovery[1][2]
Discovered byPan-STARRS 1
Discovery siteHaleakalā Obs.
Discovery date12 August 2020
Designations
MPC designation
2020 PP1
Alternative designations
P113Iyv[3]
Minor planet category
  • NEO[4]
  • Apollo
  • Earth crosser
Orbital characteristics[4]
Epoch 1 July 2021 (JD 2459396.5)
Uncertainty parameter 1
Observation arc3.94 yr (1,438 days)
Earliest precovery date24 August 2017
Aphelion1.075 AU
Perihelion0.9278 AU
Semi-major axis
1.001 AU
Eccentricity0.07356
Orbital period (sidereal)
3.99 yr
Mean anomaly
87.711°
Mean motion
0° 59m 0.667s / day
Inclination5.8636°
Longitude of ascending node
140.603°
Time of perihelion
2 April 2021 19:40 UT[4]
Argument of perihelion
43.210°
Earth MOID0.03257 AU
TJupiter6.066
Physical characteristics
Mean diameter
0.9–2.0 km (assumed albedo 0.04–0.20)[5]
Apparent magnitude
20.4 (at discovery)[1]
Absolute magnitude (H)
26.7[4] · 26.6[2]

    Discovery


    2020 PP1 was discovered on 12 August 2020 by the Pan-STARRS 1 survey at the Haleakalā Observatory.[1] It was later recovered by the Karl Schwarzschild Observatory in August 2021, which allowed for precovery in earlier Pan-STARRS observations from 24 July 2017.[7]


    Orbit and orbital evolution


    2020 PP1 is currently an Apollo asteroid (Earth-crossing but with a period longer than a year). Its semi-major axis (currently 1.001715 AU) is similar to that of Earth (0.999789 AU), but it has both low eccentricity (0.07384) and low orbital inclination (5.827°). It alternates between being an Aten asteroid and being an Apollo asteroid, although its orbital evolution is not fully stable and it can be considered as a temporary quasi-satellite of the Earth; its orbital evolution is akin to that of 469219 Kamoʻoalewa.[6]


    Physical properties


    With an absolute magnitude of 26.6, it has a diameter in the range 10–30 meters (for an assumed albedo range of 0.20–0.04 respectively).[5]


    See also



    References


    1. "MPEC 2020-P68 : 2020 PP1". Minor Planet Electronic Circular. Minor Planet Center. 13 August 2020. Retrieved 20 January 2021.
    2. "2020 PP1". Minor Planet Center. International Astronomical Union. Retrieved 3 August 2021.
    3. "2020 PP1". NEO Exchange. Las Cumbres Observatory. 13 August 2020. Retrieved 3 August 2021.
    4. "JPL Small-Body Database Browser: 2020 PP1" (2021-08-01 last obs.). Jet Propulsion Laboratory. Retrieved 3 August 2021.
    5. Bruton, Dan. "Conversion of Absolute Magnitude to Diameter for Minor Planets". Department of Physics, Engineering, and Astronomy. Stephen F. Austin State University. Retrieved 3 August 2021.
    6. de la Fuente Marcos, Carlos; de la Fuente Marcos, Raúl (March 2021). "Using Mars co-orbitals to estimate the importance of rotation-induced YORP break-up events in Earth co-orbital space". Monthly Notices of the Royal Astronomical Society. 501 (4): 6007–6025. arXiv:2101.02563. Bibcode:2021MNRAS.501.6007D. doi:10.1093/mnras/stab062.
    7. "MPEC 2021-P17 : 2020 PP1". Minor Planet Electronic Circular. Minor Planet Center. 3 August 2021. Retrieved 3 August 2021.

    Further reading







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