T Tauri: A Star is Formed
Explanation:
What does a star look like when it is forming?
The prototypical example is the
variable star T Tauri,
visible as the bright orange star near the image center.
The orange star centered in this remarkable
telescopic skyview is T Tauri, prototype of the class of
T Tauri
variable stars.
Surrounding T Tauri is a dusty yellow cosmic cloud named the
Hind's
Variable Nebula (NGC 1555/1554).
Over 400 light-years away, at the edge of a
molecular cloud,
both star and nebula
are seen to vary significantly in
brightness but not necessarily at the same time, adding to the mystery of
the intriguing region.
T Tauri stars are now generally recognized as young --
less than a few million years old -- sun-like stars still in the
early stages of
formation.
To
further
complicate the picture,
infrared observations indicate that
T Tauri itself is part of a multiple
star system. Surprisingly, due to a close gravitational pass near one of these stars,
T Tauri may now be headed out of the system.
The dramatic color
image above captures
a region that spans about 4
light-years.
Authors & editors:
Robert Nemiroff
(MTU) &
Jerry Bonnell
(USRA)
NASA Web Site Statements, Warnings,
and Disclaimers
NASA Official: Jay Norris.
Specific
rights apply.
A service of:
LHEA at
NASA /
GSFC
& Michigan Tech. U.
