(231937) 2001 FO32 is a near-Earth asteroid classified as a potentially hazardous asteroid of the Apollo group. With an estimated diameter around 550 m (1,800 ft), it was discovered by the Lincoln Near-Earth Asteroid Research at Socorro, New Mexico on 23 March 2001. The asteroid safely passed by Earth on 21 March 2021 16:03 UTC from a closest approach distance of 0.0135 AU (2.02 million km; 1.25 million mi), or 5.25 lunar distances (LD). During the day before closest approach, 2001 FO32 reached a peak apparent magnitude of 11.7 and was visible to ground-based observers with telescopeapertures of at least 20 cm (8 in).[7][8] It is the largest and one of the fastest asteroids to approach Earth within 10 LD (3.8 million km; 2.4 million mi) in 2021.[8][9]
With an observation arc of 20 years, 2001 FO32 has a well-determined orbit, and its trajectory is well known through the year 2196.[3] The asteroid's orbit is only potentially hazardous on a time scale of thousands of years.
Having a long observation arc nearly 20 years, the orbit of 2001 FO32 is well-defined with a condition code of 0.[3] Although it is classified as a potentially hazardous asteroid due to its large size combined with its small minimum orbit intersection distance (MOID) of 0.00375 AU (1.46 lunar distances) from Earth's orbital path, the asteroid will not make any close approaches within 0.01 AU (3.9 LD) over the next 200 years.[3] The asteroid's orbit is only potentially hazardous on a time scale of thousands of years.[8]
Close approaches
Over the course of its highly eccentric orbit, 2001 FO32 makes numerous close encounters with the inner planets—most often Mercury, Venus, and Earth.[3] Its MOIDs from Mercury and Venus are 0.036 AU (5.4 million km; 3.3 million mi) and 0.075 AU (11.2 million km; 7.0 million mi), respectively.[1]2001 FO32's most recent close encounter with either one of those planets was on 16 January 2008, when it passed by Mercury from a distance of 0.094 AU (14.1 million km; 8.7 million mi).
On 21 March 2021, 2001 FO32 passed by Earth from a distance of 0.0135 AU (2.02 million km; 1.25 million mi) or 5.25 LD and made its closest approach at 16:03 UTC.[3] During the few days leading up to closest approach, 2001 FO32 steadily became brighter and peaked at apparent magnitude 11.7 on 21 March 2021 2:00 UTC.[7] Although its maximum brightness was too faint to be seen with the naked eye, it was visible to observers using telescopes with apertures of at least 20 cm (8 in).[8] Due to its highly inclined and eccentric orbit, its relative velocity to Earth during the close approach is 34.4 km/s (21.4 mi/s), making it one of the fastest asteroids to pass by Earth in 2021.[8][10] By the time 2001 FO32 makes its closest approach to Earth, its solar elongation (angular separation from the Sun) would be 64°, too small to be observable from Earth.[7]
In the next 100 years, 2001 FO32 will not make any close approaches to Earth closer than the 21 March 2021 encounter. It will make a similarly close approach to Earth on 22 March 2052 18:57±00:03 UTC, from a slightly farther nominal distance of 0.0189 AU (2.83 million km; 1.76 million mi) or 7.37 LD.[3][10]
Observations
Preliminary observations by NEOWISE show that 2001 FO32 appears to be faint in infrared wavelengths of light, indicating that the asteroid is likely less than 1 kilometer in diameter.[10] Based on this, the diameter is estimated around 550 ± 110 m (1,800 ± 360 ft).[3]Near-infrared spectral data obtained by NASA's Infrared Telescope Facility in 2018 suggests that 2001 FO32 is a stony asteroid classified under the Sr spectral class.[5]
^ abBinzel, R. P.; DeMeo, F. E.; Turtelboom, E. V.; Bus, S. J.; Tokunaga, A.; Burbine, T. H.; et al. (May 2019). "Compositional distributions and evolutionary processes for the near-Earth object population: Results from the MIT-Hawaii Near-Earth Object Spectroscopic Survey (MITHNEOS)". Icarus. 324: 41–76. arXiv:2004.05090. Bibcode:2019Icar..324...41B. doi:10.1016/j.icarus.2018.12.035. S2CID125100787.
^"(231937) 2001FO32". Near Earth Objects – Dynamic Site. Department of Mathematics, University of Pisa, Italy. Retrieved 3 March 2021.