# 2020 SO

2020 SO is a near-Earth object identified to be the Centaur upper stage used on 20 September 1966 to launch the Surveyor 2 spacecraft. The object was discovered by the Pan-STARRS 1 survey at the Haleakala Observatory on 17 September 2020. It was initially suspected to be an artificial object due to its low velocity relative to Earth and later on the noticeable effects of solar radiation pressure on its orbit. Spectroscopic observations by NASA's Infrared Telescope Facility in December 2020 found that the object's spectrum is similar to that of stainless steel, confirming the object's artificial nature. Following the object's confirmation as space debris, the object was removed from the Minor Planet Center's database on 19 February 2021.

## Overview

As it approached Earth, the trajectory indicated the geocentric orbital eccentricity was less than 1 by 15 October 2020, and the object became temporarily captured on 8 November when it entered Earth's Hill sphere. It entered via the outer Lagrange point L$_2$ and will exit via Lagrange point L$_1$. 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). 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). Since discovery the time of uncertainty for February 2021 closest approach to Earth was reduced from ±3 days to less than 1 minute. It left Earth's Hill sphere at around 8 March 2021.
Paul Chodas of the Jet Propulsion Laboratory suspects 2020 SO of being the Surveyor 2 Centaur rocket booster, launched on 20 September 1966. 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. Goldstone radar produced bistatic observations on 30 November 2020 transmitting from the 70-meter DSS-14 and receiving at the 34-meter DSS-13. As a result of the bistatic DSS-14/RT-32 radar observations, a rotation period of about 9.5 seconds was obtained, which corresponds to the photometric observations. Obtained range-Doppler radar images 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, and required a telescope with roughly a 150mm (6") objective lens to be seen visually. 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.
At the time of its discovery, 2020 SO had unremarkable motion typical of a main-belt asteroid. 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.
Orbital Elements for May and December 2020 :
| Parameter | Epoch | Orbit type | Period (p) | Aphelion (Q) | Perihelion (q) | Semi-major axis (a) | Inclination (i) | Heliocentric eccentricity (e) | Geocentric eccentricity (e) |
| Units | | | (years) | AU | AU | AU | (°) | | |
| | 2020-May-31 | Apollo | 1.056 | 1.0722 | 1.0020 | 1.0371 | 0.14061° | 0.03389 | 737 |
| | 2020-Dec-17 | 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, but will not be within Earth's Hill sphere of 0.01 AU (1.5 million km).