Top Qs
Timeline
Chat
Perspective
1999 SF10
Near-Earth asteroid From Wikipedia, the free encyclopedia
Remove ads
1999 SF10 is a small, quickly rotating unnamed near-Earth asteroid (NEA). First observed on 30 September 1999 by the Lincoln Near-Earth Asteroid Research (LINEAR) program in Socorro, New Mexico, United States, it is an Earth-crossing Apollo asteroid. Its diameter is estimated to be around 60 metres (200 ft) in size with a very rapid rotation period of 2.47 minutes, indicating that it is a monolithic object.
Remove ads
History
1999 SF10 was first observed on 30 September 1999 by the Lincoln Near-Earth Asteroid Research (LINEAR) program from its Experimental Test Site (ETS) in Socorro, New Mexico, United States.[1] It was given the provisional designation 1999 SF10 by the Minor Planet Center (MPC), and its detection was announced in a Minor Planet Electronic Circular on 4 October 1999.[5] At the time of its first observation, it was rapidly approaching Earth, and on 12 October it passed within a distance of 0.0076 astronomical units (AU; 3.0 LD).[4]: 481
As of 2025[update], it has not been numbered or named by the MPC.[2] It also has not been formally assigned a discoverer, which will happen when it is numbered.[1]
Remove ads
Orbit

1999 SF10 is classified as a near-Earth asteroid (NEA). It orbits the Sun at an average distance—its semi-major axis—of 1.28 AU, taking 1.45 years to complete one revolution. It has a low orbital inclination of 1.45° relative to the ecliptic plane. Along its orbit, its distance from the Sun varies between 0.96 AU at perihelion to 1.60 AU at aphelion due to its orbital eccentricity of 0.25.[2] Because its perihelion lies below 1 AU, it is also classified as an Earth-crossing Apollo asteroid.[6][2]
Remove ads
Physical characteristics
1999 SF10 has an estimated mean diameter of 60 metres (200 ft) with dimensions of 85 by 55 metres (279 ft × 180 ft), assuming a geometric albedo of 0.110–0.117; its estimated size may be off by a factor of 2.[4]: 481 [3]: 150 Observations of its lightcurve, or variations in its observed brightness, suggest that it has a rotation period of 2.47 minutes,[4]: 481 classifying it as a monolithic fast-rotating asteroid (MFRA).[3]: 150 MFRAs have rotation periods much faster than those typically observed in asteroids, rotating faster than the critical period below which a strengthless body will self-destruct due to centrifugal forces.[3]: 148
See also
Notes
- Discoverer not yet assigned by the MPC
References
External links
Wikiwand - on
Seamless Wikipedia browsing. On steroids.
Remove ads