Discovery[1][2] | |
---|---|
Discovered by | Pan-STARRS 2 |
Discovery site | Haleakala Obs. |
Discovery date | 27 April 2020 |
Designations | |
2020 HS7 | |
NEO · Apollo[3][1] | |
Orbital characteristics[3] | |
Epoch 9 August 2022 (JD 2459800.5) | |
Uncertainty parameter 6 | |
Observation arc | 1 day |
Aphelion | 2.904 AU |
Perihelion | 0.793 AU |
1.849 | |
Eccentricity | 0.5709 |
2.51 yr (918 days) | |
308.988° | |
0° 23m 31.807s / day | |
Inclination | 4.732° |
38.531° | |
245.692° | |
Physical characteristics | |
Dimensions | a/b ≥ 1.04[4] |
4–8 m[5] | |
2.9945±0.0002 s[4] 2.9938±0.0002 s[4] | |
29.10±0.36[3] | |
2020 HS7 is a very small asteroid classified as a near-Earth object of the Earth-crossing Apollo group. When it was discovered by the Pan-STARRS 2 survey on 27 April 2020, the asteroid was initially calculated to have a 10% chance of impact with Earth before being ruled out by improved orbit determinations from additional observations.[6] Although there is now no risk of impact with Earth, it did make a close approach 42,700 kilometres (26,500 mi) from Earth on 28 April 2020, with a flyby speed of 15.6 kilometres per second (9.7 mi/s) relative to Earth.[3][7][5] The asteroid will not make any close encounters within 1 lunar distance (380,000 km; 240,000 mi) of Earth in the next 100 years.[3]
Observations by Kiso Observatory in Nagano, Japan show that the asteroid rotates extremely rapidly with a rotation period of 3 seconds, making it the fastest-rotating asteroid known as of 2022[update].[4] No other near-Earth asteroid of similar size is known to have a rotation period shorter than 10 seconds, which could be attributed to the tangential component of the YORP effect accelerating their rotation far beyond this period.[4] The asteroid exhibits a very small light curve amplitude of 0.07 magnitudes, which either implies a nearly spherical shape or a pole-on rotation during observations.[4]
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