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  2. NGC 1 - Wikipedia

    en.wikipedia.org/wiki/NGC_1

    The NGC 1 and 2 pair are not physically related. NGC 1 lies at a distance of ~200 million l.y. with NGC 2 at roughly 320 million l.y. [5] The initial observers missed NGC 2, which is much fainter. NGC 1 appears to be quite close to NGC 2, in reality however, the two objects are far apart and unrelated. NGC 2 was first observed as a "companion ...

  3. List of NGC objects - Wikipedia

    en.wikipedia.org/wiki/List_of_NGC_objects

    The following is a list of NGC objects, that is objects listed in the New General Catalogue (NGC). It is one of the largest comprehensive astronomical catalogues for deep sky objects such as star clusters, nebulae, and galaxies. List of NGC objects (1–1000) List of NGC objects (1001–2000) List of NGC objects (2001–3000)

  4. List of NGC objects (1–1000) - Wikipedia

    en.wikipedia.org/wiki/List_of_NGC_objects_(1–1000)

    This is a list of NGC objects 1–1000 from the New General Catalogue (NGC). The astronomical catalogue is composed mainly of star clusters, ... 11.2 46: Star [1]

  5. List of planetary nebulae - Wikipedia

    en.wikipedia.org/wiki/List_of_planetary_nebulae

    Lists of planets; References This page was last edited ... NGC 6881: 1881 5.2 ± 1.6 13.8 Cygnus: NGC 6884: 1883 6.5 10.9 Cygnus: NGC 6891 1884 7.2 10.5 Delphinus:

  6. List of the most distant astronomical objects - Wikipedia

    en.wikipedia.org/wiki/List_of_the_most_distant...

    z = 2.554 (11.1 Gly) Observations from ALMA has shown that the lensed galaxy 9io9 contains a magnetic field. Planet: SWEEPS-11 / SWEEPS-04 (27,710 ly) [96] An analysis of the lightcurve of the microlensing event PA-99-N2 suggests the presence of a planet orbiting a star in the Andromeda Galaxy. [97]

  7. TrES-2b - Wikipedia

    en.wikipedia.org/wiki/TrES-2b

    The radial velocity of GSC 03549–02811 over time, caused by the presence of TrES-2 b. TrES-2b was discovered on August 21, 2006 by the Trans-Atlantic Exoplanet Survey (TrES) by detecting the transit of the planet across its parent star using Sleuth (Palomar Observatory, California) and PSST (Lowell Observatory, Arizona), part of the TrES network of 10–cm telescopes.

  8. HR 8799 - Wikipedia

    en.wikipedia.org/wiki/HR_8799

    The inner and outer edges of this belt are close to 4:1 and 2:1 resonances with the planet. [8] A broad zone of cold dust (T ≈ 45 K) with a sharp inner edge orbiting just outside the outermost planet (b). The inner edge of this belt is approximately in 3:2 resonance with said planet, similar to Neptune and the Kuiper belt. [8]

  9. NGC 2 - Wikipedia

    en.wikipedia.org/wiki/NGC_2

    NGC 1 and NGC 2 as an optical double. NGC 2 is located about 345 million light-years from the Solar System, with a magnitude of +14.2, while the distance to NGC 1 is 210 million light-years. Although visually close in the sky, NGC 1 and NGC 2 are at very different distances; were they stars, they would be referred to as an "optical double" as ...