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  2. Vela (constellation) - Wikipedia

    en.wikipedia.org/wiki/Vela_(constellation)

    Vela is a constellation in the southern sky, which contains the Vela Supercluster. Its name is Latin for the sails of a ship, and it was originally part of a larger constellation, the ship Argo Navis , which was later divided into three parts, the others being Carina and Puppis .

  3. Vela (satellite) - Wikipedia

    en.wikipedia.org/wiki/Vela_(satellite)

    Vela was the name of a group of reconnaissance satellites developed as the Vela Hotel element of Project Vela by the United States to detect nuclear detonations and monitor Soviet Union compliance with the 1963 Partial Test Ban Treaty. Vela started out as a small budget research program in 1959.

  4. NGC 3256 - Wikipedia

    en.wikipedia.org/wiki/NGC_3256

    NGC 3256 is a peculiar galaxy formed from the collision of two separate galaxies in the constellation of Vela. NGC 3256 is located about 100 million light-years away and belongs to the Hydra–Centaurus Supercluster complex. NGC 3256 provides a nearby template for studying the properties of young star clusters in tidal tails. The system hides a ...

  5. NGC 3132 - Wikipedia

    en.wikipedia.org/wiki/NGC_3132

    NGC 3132 (also known as the Eight-Burst Nebula, [2] the Southern Ring Nebula, [2] or Caldwell 74) is a bright and extensively studied planetary nebula in the constellation Vela. Its distance from Earth is estimated at 613 pc or 2,000 light-years .

  6. NGC 3201 - Wikipedia

    en.wikipedia.org/wiki/NGC_3201

    NGC 3201 (also known as Caldwell 79) is a low galactic latitude globular cluster in the southern constellation of Vela. It has a very low central concentration of stars. [ 10 ] This cluster was discovered by James Dunlop on May 28, 1826 and listed in his 1827 catalogue.

  7. Vela Supernova Remnant - Wikipedia

    en.wikipedia.org/wiki/Vela_Supernova_Remnant

    The Vela supernova remnant includes NGC 2736. Viewed from Earth, the Vela supernova remnant overlaps the Puppis A supernova remnant, which is four times more distant. Both the Puppis and Vela remnants are among the largest and brightest features in the X-ray sky. The Vela supernova remnant is one of the closest known to us.

  8. Vela Pulsar - Wikipedia

    en.wikipedia.org/wiki/Vela_Pulsar

    Gamma ray and optical (visible light) light curves for the pulsar, adapted from Spolon et al. (2019) [3]. Vela is the brightest pulsar (at radio frequencies) in the sky and spins 11 times per second [4] (i.e. a period of 89.33 milliseconds—the shortest known at the time of its discovery) and the remnant from the supernova explosion is estimated to be travelling outwards at 1,200 km/s (750 mi ...

  9. Luhman 16 - Wikipedia

    en.wikipedia.org/wiki/Luhman_16

    Luhman 16 is located in the southern celestial hemisphere in the constellation Vela. As of July 2015, its components are the nearest-known celestial objects in this constellation outside the Solar System. Its celestial coordinates: RA = 10 h 49 m 18.723 s, Dec = −53° 19′ 09.86″. [1]

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