The V838 Monocerotis Light Echo and the New Class of Luminous Transients
Howard Bond(STScI)
A "light echo" is one of the rarest and most beautiful phenomena in
astronomy. The most spectacular light echo in history is occurring
around the previously unknown star V838 Monocerotis, and is being
imaged regularly by the Hubble Space Telescope.
A light echo is created when light from a sudden stellar brightening
spreads out into space and illuminates nearby interstellar dust.
Because of the detour that the light takes in going out to the dust,
scattering off it, and then traveling to the Earth, the light
arrives months or years after the light from the star itself.
The light echo around V838 Mon, which had a sudden outburst in early
2002, leads to a direct geometric determination of the distance to
the star through a novel technique based on polarimetric imaging
with the Hubble telescope. The resulting distance of 20,000
light-years shows that V838 Mon was temporarily one of the brightest
stars in the Milky Way. Its unusual outburst--the star expanded to
become a red supergiant within a few weeks--poses a severe puzzle to
stellar theoreticians. Transients of similar behavior have been
discovered in the galaxies M31 and M85. The mystery is deepened by
our recent discovery that V838 Mon belongs to a young stellar
cluster, lying at the outer edge of our Galaxy.
Perhaps more important to the non-specialist, however, the images of
the light echo are among the most stunning obtained to date by the
Hubble Space Telescope.
