NGC 2261 (also known as Hubble's Variable Nebula or Caldwell 46) is a variable nebula located in the constellation Monoceros. The nebula is illuminated by the star R Monocerotis (R Mon), which is not directly visible itself.
Reflection nebula | |
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Variable Nebula | |
![]() An image of NGC 2261 by the Hubble Space Telescope Credit: HST/NASA/JPL/Judy Schmidt | |
Observation data: J2000.0 epoch | |
Right ascension | 6h 39m 10s[1] |
Declination | +8° 45′[1] |
Distance | 2,500 ly |
Apparent magnitude (V) | 9.0 |
Apparent dimensions (V) | 2′ |
Constellation | Monoceros |
Designations | Hubble's Variable Nebula,[1] Caldwell 46 |
See also: Lists of nebulae |
NGC 2261 was discovered in 1783 by William Herschel.[2]
NGC 2261 was imaged as Palomar Observatory's Hale Telescope's first light by Edwin Hubble on January 26, 1949,[3] some 20 years after the Palomar Observatory project began in 1928. Hubble had studied the nebula previously at Yerkes and Mt. Wilson.[3] Hale had taken photographic plates with a 24-inch (60.96 cm) reflecting telescope in 1916.[4] Also, plates were taken using the same telescope in 1908 by FC Jordan, this allowed Hale to use of a blink comparator to study any changes in the nebula.[4]
NGC 2261 was imaged by the Hubble Space Telescope, and an image of the nebula was released in 1999.[5]
The star R Monocerotis has lit up a nearby cloud of gas and dust, but the shape and brightness slowly changes visibly even in small telescopes over weeks and months, and the nebula looks like a small comet.[6]
One explanation proposed for the variability is that dense clouds of dust near R Mon periodically block the illumination from the star.[7] This casts a temporary shadow on the nearby clouds.[8]
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See also | |
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New General Catalogue 2000 to 2499 | |
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