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1054 Forsytia / f ɔːr ˈ s ɪ t i ə / is a dark background asteroid, approximately 46 kilometers in diameter, from the outer regions of the asteroid belt.It was discovered on 20 November 1925, by astronomer Karl Reinmuth at the Heidelberg-Königstuhl State Observatory in southwest Germany and assigned provisional designation 1925 WD. [14]
L1, L2, and L3 are unstable orbits[6], meaning that small perturbations will cause the orbiting craft to drift out of the orbit without periodic corrections. P/2 orbit, a highly-stable 2:1 lunar resonant orbit, that was first used with the spacecraft TESS (Transiting Exoplanet Survey Satellite) in 2018. [29] [30]
Estimates from an IAU question-and-answer press release from 2006, giving 800 km radius and 0.5 × 10 21 kg mass as cut-offs that normally would be enough for hydrostatic equilibrium, while stating that observation would be needed to determine the status of borderline cases. [50]
Second row (green lights) 6-1=5. Third Row (orange light)71+09= 80. Bottom Row (light blue light) 63-32= 31. The doors will open automatically once you enter all the numbers correctly. Continue ...
2000 FE 8 is part of a group of trans-Neptunian objects that orbit in a 2:5 resonance with Neptune. [6] That means that for every five orbits that Neptune completes, 2000 FE 8 makes only two. [ 3 ] Several other objects are in the same orbital resonance, the largest of which is (84522) 2002 TC 302 .
SPOTLIGHT2, which provides a resolution of 1 m (3 ft 3 in) over a 10 × 10 km (6.2 × 6.2 mi) area. Spotlight polarization is limited to either HH or VV; There are two Stripmap modes: HIMAGE, which provides a resolution of between 3 and 5 m (9.8 and 16.4 ft) over a swath of 40 km (25 mi), and
Clickable image, highlighting medium altitude orbits around Earth, [a] from Low Earth to the lowest High Earth orbit (geostationary orbit and its graveyard orbit, at one ninth of the Moon's orbital distance), [b] with the Van Allen radiation belts and the Earth to scale To-scale diagram of low, medium, and high Earth orbits Space of Medium Earth orbits (MEO) as pink area, with Earth and the ...
Johnson is a stony S-type asteroid and member of the dynamical Hungaria group, which forms the innermost dense concentration of asteroids in the Solar System. [3] [4] It is, however, not a member of collisional Hungaria family, but a non-family asteroid of the main belt's background population when applying the hierarchical clustering method to its proper orbital elements.