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  2. (35396) 1997 XF11 - Wikipedia

    en.wikipedia.org/wiki/(35396)_1997_XF11

    Additional precovery observations of the asteroid from 1990 were quickly found that refined the orbit and it is now known the asteroid will pass Earth on 26 October 2028, at a distance of 929,000 km (2.42 LD). [3] [14] [15] During the close approach, the asteroid should peak at about apparent magnitude 8.2, [16] and will be visible in ...

  3. List of missions to minor planets - Wikipedia

    en.wikipedia.org/wiki/List_of_missions_to_minor...

    Insertion reattempted successfully on 14 February 2000. Impacted asteroid at 20:01 on 12 February 2001 at end of mission, but survived impact and continued to operate on surface until 1 March. [6] – Cassini-Huygens Cassini: 15 October 1997 [1] Titan IV(401)B Centaur-T [7] NASA: 2685 Masursky: Flyby —

  4. List of exceptional asteroids - Wikipedia

    en.wikipedia.org/wiki/List_of_exceptional_asteroids

    Most highly inclined known main-belt asteroid from September 26, 2008, to March 8, 2010 [citation needed] MPC: 2010 EQ 169: 91.606° March 8, 2010 Most highly inclined known main-belt asteroid (orbit is not well-known) [citation needed] MPC: 2024 TF 3: 89.154° March 8, 2010 Extremely high-inclined trans-Neptunian object. [citation needed] MPC

  5. Asteroid belt - Wikipedia

    en.wikipedia.org/wiki/Asteroid_belt

    The asteroid belt is a torus-shaped region in the Solar System, ... then NEAR imaged 253 Mathilde in 1997 and landed on near–Earth asteroid 433 Eros in February 2001.

  6. Nobuhiro Kawasato - Wikipedia

    en.wikipedia.org/wiki/Nobuhiro_Kawasato

    As of 2016, most of his discoveries, such as the inner main-belt asteroid (9942) ... (46732) 1997 TD 19: 8 October 1997: list (47079) 1998 YA 3: 16 December 1998: list

  7. 19367 Pink Floyd - Wikipedia

    en.wikipedia.org/wiki/19367_Pink_Floyd

    19367 Pink Floyd (provisional designation 1997 XW 3) is a dark background asteroid from the inner regions of the asteroid belt, approximately 7 kilometers in diameter. It was discovered on 3 December 1997, by European astronomers of the ODAS survey at the CERGA Observatory near Caussols, France. [ 5 ]

  8. Amor asteroid - Wikipedia

    en.wikipedia.org/wiki/Amor_asteroid

    Common orbital subgroups of Near-Earth Objects (NEOs). The Amor asteroids are a group of near-Earth asteroids named after the archetype object 1221 Amor / ˈ eɪ m ɔːr /.The orbital perihelion of these objects is close to, but greater than, the orbital aphelion of Earth (i.e., the objects do not cross Earth's orbit), [1] with most Amors crossing the orbit of Mars.

  9. OCA–DLR Asteroid Survey - Wikipedia

    en.wikipedia.org/wiki/OCA–DLR_Asteroid_Survey

    The OCA–DLR Asteroid Survey (ODAS) was an astronomical survey to search for small Solar System bodies focusing on near-Earth objects in the late 1990s. This European scientific project was a collaboration between the French Observatoire de la Côte d'Azur (OCA) and the German Aerospace Center (DLR).