2020 SO
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As it approached Earth, the trajectory indicated the geocentric orbital eccentricity was less than 1 by 15 October 2020,[10][b] and the object became temporarily captured on 8 November when it entered Earth's Hill sphere.[11] It entered via the outer Lagrange point L2 and will exit via Lagrange point L1. During its geocentric orbit around Earth, 2020 SO made a close approach to Earth on 1 December 2020 at a perigee distance of approximately 0.13 lunar distances (50,000 km; 31,000 mi).[4] It also made another close approach on 2 February 2021, at a perigee distance of approximately 0.58 LD (220,000 km; 140,000 mi).[4] Since discovery the time of uncertainty for February 2021 closest approach to Earth was reduced from ±3 days to less than 1 minute.[4] It left Earth's Hill sphere at around 8 March 2021.[12][b]

Paul Chodas of the Jet Propulsion Laboratory suspects 2020 SO of being the Surveyor 2 Centaur rocket booster, launched on 20 September 1966.[11][12][13] The Earth-like orbit and low relative velocity suggest a possible artificial object. Spectroscopy may help determine if it is covered in white titanium dioxide paint.[14] Goldstone radar produced bistatic observations on 30 November 2020 transmitting from the 70-meter DSS-14 and receiving at the 34-meter DSS-13.[15] As a result of the bistatic DSS-14/RT-32 radar observations, a rotation period of about 9.5 seconds was obtained,[16] which corresponds to the photometric observations.[6] Obtained range-Doppler radar images[16] confirm that the object has an elongated shape with a length of about 10 meters and a width of about 3 meters.
Around the time of closest approach on 1 December 2020, the object was only brightened to about apparent magnitude 14.1,[7] and required a telescope with roughly a 150mm (6") objective lens to be seen visually.[17] It displays a large light curve amplitude of 2.5 magnitudes, signifying a highly elongated shape or albedo variations on its surface. It has a rotation period of approximately 9 seconds.[18]
At the time of its discovery, 2020 SO had unremarkable motion typical of a main-belt asteroid.[citation needed] However, the four observations that Pan-STARRS obtained over the course of 1.4 hours showed non-linear motion due to the rotation of the observer around Earth's axis, which is a signature of a nearby object.[1][10]
| Parameter | Epoch | Orbit type |
Period (p) |
Aphelion (Q) |
Perihelion (q) |
Semi-major axis (a) |
Inclination (i) |
Heliocentric eccentricity (e) |
Geocentric eccentricity (e)[10][c] |
|---|---|---|---|---|---|---|---|---|---|
| Units | (years) | AU | (°) | ||||||
| 2020-May-31[4] | Apollo | 1.056 | 1.0722 | 1.0020 | 1.0371 | 0.14061° | 0.03389 | 737 | |
| 2020-Dec-17[2] | Atira | 0.980 | 0.9882 | 0.9847 | 0.9865 | 0.13842° | 0.00180 | 0.89934 | |
In January and February 2036, it will again approach Earth with a geocentric eccentricity less than 1 since the relative velocities will be small,[10] but will not be within Earth's Hill sphere of 0.01 AU (1.5 million km).[4][d]
See also
- J002E3 – a near-Earth object discovered in 2002 that was identified as the S-IVB third stage of the Apollo 12 Saturn V rocket
- WT1190F – temporarily orbiting space debris that entered Earth's atmosphere in 2015
- 2018 AV2 – an artificial object discovered in a temporary orbit around Earth in 2018, now suspected to be the Snoopy module from Apollo 10
- 6Q0B44E – another artificial object discovered in orbit around Earth in 2018
- Space debris
- Temporary satellite