NGC 2261 - Hubble's Variable Nebula
seen from Brazil
seen from United States
seen from China

seen from United States

seen from T1

seen from T1
seen from T1
seen from United States
seen from Canada
seen from China
seen from United States
seen from South Korea
seen from China
seen from China

seen from Singapore

seen from Brazil
seen from China
seen from China
seen from China
seen from China
NGC 2261 - Hubble's Variable Nebula
Hind's Variable Nebula, NGC 1555 // George Hatfield
Hubble's Variable Nebula, NGC 2261 // AnaTa
Hubble's Variable Nebula, NGC 2261 // Rajat Kumar
Hubble's Variable Nebula, C46 // Kent Wood
The bright star at the corner of the "fan" is R Monocerotis, a very young binary star system. Light from this star lights up the nearby cloud of gas and dust, but observations over just weeks shows that the nebula changes brightness. One explanation is that dense clouds of dust near R Monocerotis pass in front of it, periodically blocking light and casting a shadow on the nearby clouds.
Hubble's Variable Nebula, C46 // Haejong Kim
Hubble's Variable Nebula (NGC 2261) is cloud of gas and dust extending from a bright star like smoke rising from a newly lit fire. This reflection variable nebula lies about 2,500 light years away in the constellation of Monoceros, the Unicorn.
Although it was first discovered by William Herschel (1738-1822) in 1783, it was Edwin Hubble (1889-1953) who performed the first detailed analysis of this peculiar fan-shaped nebula.
Hind's Variable Nebula, NGC 1555 // FrancoisGAP
Hind's Variable Nebula, NGC 1555 // Roger Bertuli