A light echo is a physical phenomenon caused by light reflected off surfaces distant from the source, and arriving at the observer with a delay relative to this distance. The phenomenon is analogous to an echo of sound, but due to the much faster speed of light, it mostly manifests itself only over astronomical distances.
Images showing the expansion of the light echo of V838 Monocerotis. Credit: NASA/ESA.
An echo of ShaSS 073 galaxy's light detected by ESO's VLT Survey Telescope.
A Hubble Space Telescope image of NGC 5972, a quasar ionisation echo.
V838 Monocerotis is a spectroscopic binary star system in the constellation Monoceros about 19,000 light years from the Sun. The previously unremarked star was observed in early 2002 experiencing a major outburst, and was one of the largest known stars for a short period following the outburst. Originally believed to be a typical nova eruption, it was then identified as the first of a new class of eruptive variables known as luminous red novae. The reason for the outburst is still uncertain, but is thought to have been a merger of two stars within a triple system.
Hubble Space Telescope image of V838 Monocerotis and the surrounding nebula on September 9, 2006 Credit: NASA/ESA
Light echo of V838 Mon as imaged April 30, 2002
Images showing the expansion of the light echo. Credit: NASA/ESA.
Two pictures taken in November 2005 and September 2006 showing the changes that occurred to the bright echo of V838 Mon.