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  2. Near-Earth Asteroid Tracking - Wikipedia

    en.wikipedia.org/wiki/Near-Earth_Asteroid_Tracking

    Near-Earth Asteroid Tracking (NEAT) was a program run by NASA and the Jet Propulsion Laboratory, surveying the sky for near-Earth objects. NEAT was conducted from December 1995 until April 2007, at GEODSS on Hawaii (Haleakala-NEAT; 566 ), as well as at Palomar Observatory in California (Palomar-NEAT; 644 ).

  3. Cameras for All-Sky Meteor Surveillance - Wikipedia

    en.wikipedia.org/wiki/Cameras_for_All-Sky_Meteor...

    CAMS [3] networks around the world use an array of low-light video surveillance cameras to collect astrometric tracks and brightness profiles of meteors in the night sky. . Triangulation of those tracks results in the meteor's direction and speed, from which the meteors’ orbit in space is calculated and the material's parent body can be identifi

  4. Asteroid Terrestrial-impact Last Alert System - Wikipedia

    en.wikipedia.org/wiki/Asteroid_Terrestrial...

    NASA's Near Earth Observation Program initially provided a US$5 million grant, with $3.5 million covering the first three years of design, construction and software development, and the balance of the grant to fund the systems operation for two years following its entry into full operational service in late 2015. [41]

  5. C/2024 G3 (ATLAS) - Wikipedia

    en.wikipedia.org/wiki/C/2024_G3_(ATLAS)

    The comet was reported to have a nuclear shadow, a dark lane in the tail, and was marginally visible with naked eye on that day. [10] On 7 January the comet was reported to be of first magnitude, with a tail about 20 arcminutes long. [5] The comet was photographed by cosmonaut Ivan Vagner onboard the International Space Station on 10 January. [11]

  6. Wide-field Infrared Survey Explorer - Wikipedia

    en.wikipedia.org/wiki/Wide-field_Infrared_Survey...

    [52] [58] Few objects smaller than 100 m (330 ft) in diameter were detected by NEOWISE's automated detection software, known as the WISE Moving Object Processing Software (WMOPS), because it requires five or more detections to be reported. [59] The average albedo of asteroids larger than 100 m (330 ft) discovered by NEOWISE is 0.14. [59]

  7. The horned “devil comet,” notable for a recent series of explosive outbursts, is visible in the night sky now and will appear during April’s total solar eclipse.

  8. List of missions to comets - Wikipedia

    en.wikipedia.org/wiki/List_of_missions_to_comets

    Entered orbit around 67P at 09:06 UTC on 6 August 2014. On 30 September 2016 mission ended in an attempt to slow land on the comet's surface near a 130 m (425 ft) wide pit called Deir el-Medina. Ariane 5G+ Philae: 2 March 2004: ESA / DLR Germany: 67P/Churyumov–Gerasimenko: Lander Successful: Carried by Rosetta.

  9. List of minor planets and comets visited by spacecraft

    en.wikipedia.org/wiki/List_of_minor_planets_and...

    first soft landing on a comet (November 2014) Notes: (a) Due to a non-spherical, irregular shape, a comet's x, y, and z axes instead of an (average) diameter are often used to describe its dimensions. (b) Closest approach given in multiples of the comet's (average mean) radius · List ordered in ascending order by a comet's first visit.