Sections

2003 SD220

Discovered on September 29 2003 by LONEOS, Anderson Mesa. Included in the list of the "Potentially Hazardous Asteroids" of the Minor Planet Center.

Orbital and Physical Characteristics

Epoch 2021 Jul 05
Mean Anomaly 357.01326°
Argument of Perihelion 326.93416°
Longitude of Ascending Node 273.91415°
Inclination 8.51459°
Eccentricity 0.2106313
Semimajor Axis 0.8266941 AU
Orbital Period 0.75 years
MOID
0.0180705 AU
Orbit type Aten
Absolute Magnitude 17.56
Diameter 791±25 m [1]; 600-1200 m [3]
Rotation period 285.0 h [2]

Radar scattering properties

SC/OC
0.17 [3]
Radar albedo 0.25 [3]

Close Approach to the Earth

Date of encounter 2021 Dec 17
Distance 0.03628 AU (14.12 lunar distances)

Observation Schedule

Date Window, UT
Receiver
Transmitter
Frequency, MHz
λ, cm
Ptx, kW
R, au
RTT, sec
SNR/RTT
2021 Dec 4 12:31 - 13:30 RT-32 (Sv, Zc, Bd) DSS-14 [4] 8560.0 3.5 440 0.05513 55 6
2021 Dec 9 06:00 - 07:20 RT-32 (Sv, Zc, Bd) DSS-14 [4] 8560.0 3.5 440 0.04501 45 13
2021 Dec 10 01:25 - 04:30 RT-32 (Bd) DSS-14 [4] 8560.0 3.5 440 0.04348 43 15
2021 Dec 20 02:35 - 05:20 RT-32 (Bd) DSS-14 [4] 8560.0 3.5 440 0.03707 37 26
2021 Dec 21 03:02 - 05:10 RT-32 (Bd) DSS-14 [4] 8560.0 3.5 440 0.03788 38 24

Echo power spectrum

Bistatic DSS-14/RT-32 continuous wave echo power spectra of 2003 SD220 obtained at Badary observatory on December 4, 2021 on 5 radar transmit-receive cycles from 12:39 UT and on December 9 from 06:55 to 17:15 UT. Solid and dashed lines denote echo power in the opposite circular (OC) and same circular (SC) polarizations as that of the transmitted wave. The broadening of the obtained spectra corresponds to an asteroid of at least 570 meters on December 4 and at least 1140 meters on December 9, assuming that its rotation period is 285.0 h [2]. These results characterize an object with a noticeably elongated shape, which is consistent with radar observations on December 17-22, 2018.

Remarks

  1. Nugent, C.R. et al., NEOWISE Reactivation Mission Year Two: Asteroid Diameters and Albedos, The Astronomical Journal, 152(3), 2016.

  2. Warner, B.D. et al., 2009.

  3. Yu. S. Bondarenko et al., 2021.

  4. We thank L. A. Benner, S. Naidu, M. Brozovic and the technical staff at Goldstone for the help with the radar observations.