NGC 2023

NGC 2023
reflection nebula
emission nebula

NGC 2023 picture created from multiple images taken with the Wide Field Camera of Hubble’s Advanced Camera for Surveys.
Observation data: J2000 epoch
Right ascension 05h 41m 37.9s[1]
Declination −02° 15 52
Distance 1467.7 ly   (450 pc)
Apparent dimensions (V) 10′x10′
Constellation Orion
Designations NGC 2023, LBN 954, VDB 52, [XT95] 6, GN 05.39.1.02, RAFGL 806, [NYS99] C-23, IRAS 05391-0217, RX J0541.8-0217, [RK68] 38

NGC 2023 (also known as LBN 954) is a reflection nebula located in the constellation of Orion (The Hunter).[2]

Regarding infrared wavelengths, it is a heavy source of fluorescent molecular hydrogen emission,[3] and at 4 light-years wide, it is one of the largest reflection nebulae in the sky. It is powered by an extremely hot B-type star (B1.5), called HD 37903, the most luminous member of a cluster of young Herbig–Haro objects that illuminate the outermost material in the Lynds 1630 molecular cloud (Barnard 33) in Orion B.

NGC 2023 forms a cavity in the surface of the cloud, some 450 parsecs from Earth. It produces a bright visual reflection nebula and an ultraviolet-excited photodissociation region. It is about a third of a degree from the Horsehead Nebula [4] and is often included (but not labeled) in images of that object.

Additionally, one of the defining features of NGC 2023 — the overtly bright streak often seen in the upper-left hand corner — is not a true feature. Instead, the flare is an artifact generated by Hubble’s optics.[5]

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Coordinates: 05h 41m 37.9s, −02° 15′ 52″