Artist's concept of a near-Earth object. Image: Courtesy NASA/JPL-Caltech |
Background
(as of 2020-07-20 )
(Check links for Updates)
- Object: 2020 NK1
- Orbit Type: Apollo [NEO, PHA]
- Approximate Diameter: 420 m - 940 m (1377.95 to 3083.99 Feet) (Absolute H= 19.0 )
- On the Sentry Risk Table: YES [26 Number of Potential Impacts 2084-2106]
- for more information read Understanding Risk Pages by Jon Giorgini
- On the NEODyS CLOMON2 risk page: YES[46 Number of Potential Impacts 2080-2103]
- Listed on The Near-Earth Object Human Space Flight Accessible Targets Study (NHATS):NO
- Listed on the Goldstone Asteroid Radar Schedule:NO
- Listed on the Arecibo Asteroid Radar Schedule:YES(Priority Level High)
- Radar Observations: none (yet)
- Discovery observation was made:2020 07 13.567919 by ATLAS-MLO, Mauna Loa(MPC Code T08)
- Last Observation(publish) was made:2020 07 19.607192 by ATLAS-HKO, Haleakala(MPC Code T05)
- Number of Optical Observations(published): 29
- Oppositions: 1
- Number of Observatories Reporting (Published) Observations :6
- Observatories Reporting (Published) Observations(MPC Code):
- (474) Mount John Observatory, Lake Tekapo, New Zealand.
- (E10) Siding Spring-Faulkes Telescope South, Australia/NSW.
- (T05) ATLAS-HKO, Haleakala, US/Hawaii. Observer
- (T08) ATLAS-MLO, Mauna Loa,US/Hawaii. Observers
- (W88) Slooh.com Chile Observatory, La Dehesa,Chile.
- (Z84) Calar Alto-Schmidt, Spain.
- Perihelion Distance: 0.49 AU
- Aphelion Distance: 2.28 AU
- Earth MOID: 0.00278361 AU (1.083 Lunar Distance) 65.29 Earth radii
- Close-Approach to Earth: 2020-Jul-31 Minimum Distance 0.052769696480622 (AU) 20.536 Lunar Distance (LD)
- JPL Small-Body Database Browser (2020 NK1)
- Sentry: Earth Impact Monitoring 2020 NK1 -- Earth Impact Risk Summary
- NEODyS-2 2020NK1
- Understanding Risk Pages by Jon Giorgini
- Arecibo Asteroid Radar Schedule
- MPC Observations Database 2020 NK1
- Torino Scale
- Sentry: Earth Impact Monitoring Introduction
- Palermo Technical Impact Hazard Scale
- Quantifying the risk posed by potential Earth impacts Steven R. Chesley (JPL), Paul W. Chodas (JPL), Andrea Milani (Univ. Pisa), Giovanni B. Valsecchi Icarus 159, 423-432 (2002) (PDF)
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