Sections

1998 OR2

Discovered on July 24, 1998 by NASA's Near-Earth Asteroid Tracking (NEAT) program on Haleakala, Hawaii. Included in the list of the "Potentially Hazardous Asteroids" of the Minor Planet Center.

Orbital and Physical Characteristics

Epoch 2020 May 31
Mean Anomaly 12.10139°
Argument of Perihelion 174.56624°
Longitude of Ascending Node 27.01542°
Inclination 5.86588°
Eccentricity 0.5730840
Semimajor Axis 2.3844355 AU
Orbital Period 3.68 years
MOID
0.0154377 AU
Orbit type Amor
Absolute Magnitude 15.8
Diameter ~2060 m
Rotation period 4.112 h [1]

Radar scattering properties

SC/OC
0.38 [2]
Radar albedo 0.11 [2]

Close Approach to the Earth

Date of encounter 2020 Apr 29
Distance 0.0420 AU (16.4 lunar distances)

Observation Schedule

Date Window, UT
Receiver
Transmitter
Frequency, MHz
λ, cm
Ptx, kW
R, au
RTT, sec
SNR/RTT
2020 Apr 19 22:09 - 23:50 RT-32 (Sv) Arecibo [3] 2380.0 12.6 350 0.063 63 3
22:09 - 22:30 RT-32 (Zc)
2020 Apr 20 22:14 - 23:30 RT-32 (Sv) Arecibo [3] 2380.0 12.6 350 0.060 59 4
2020 Apr 21 22:21 - 23:15 RT-32 (Sv) Arecibo [3] 2380.0 12.6 350 0.056 56 5
2020 Apr 22 22:33 - 22:58 RT-32 (Sv) Arecibo [3] 2380.0 12.6 350 0.053 53 6

Range-Doppler radar images

Bistatic Arecibo/RT-32 range-Doppler radar images of 1998 OR2 obtained at Svetloe observatory on April 20, 2020 from 23:11 to 23:30 UT in "Gray" and "Hot" palettes. Range (distance from the observer) increases down at 150 m per pixel and Doppler frequency increases to the right at 1 Hz per pixel. The images have been scaled to the same spatial range. The images are normalized so that the noise has zero mean and unit standard deviation.

Echo power spectrum

Bistatic Arecibo/RT-32 continuous wave echo power spectra of 1998 OR2 obtained at Svetloe observatory on April 22, 2020 from 22:33 to 22:58 UT and on April 20, 2020 from 22:53 to 23:08 UT. Solid and dashed lines denote echo power in the opposite circular (OC) and same circular (SC) polarizations as that of the transmitted wave.

Remarks

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

  2. Yu. Bondarenko et al., 2020.

  3. We thank P. A. Taylor, A. K. Virkki, S. E. Marshall, F. Venditti and the technical staff at Arecibo for the help with the radar observations.