This image of Comet McNaught comes from the Heliospheric Imager on one of the STEREO spacecraft, taken Jan. 11, 2007. To the right is the comet nucleus, so bright it saturates the detector creating a bright vertical band in the image. The comet's dynamic tails extend up and to the left.
The lowest of the tails is the ion tail, which points along the direction of the solar wind. Above that is the comet's dust tail pushed out by radiation pressure from the sun. The tail is highly structured, probably the result of dynamic activity in the comet itself.
Although the two STEREO observatories have been turning on their instruments since mid-December, the Heliospheric Imagers on this spacecraft turned on for the first time on Jan. 11 - just in time to see the spectacular Comet McNaught.
The Heliospheric Imagers are designed to observe the space between the Sun and the Earth in order to watch solar storms as they head our way. But here the Heliospheric Imagers are also able to observe Comet McNaught as it heads towards the sun.
STEREO's SECCHI/HI instrument was built by a consortium led by the Naval Research Laboratory (USA), and includes the University of Birmingham (UK), Rutherford Appleton Laboratory (UK) and Centre Spatiale de Liege (Belgium). Image credit: NASA
Source: NASA, by Rani Gran
Explore further: Physicist helps explain characteristics of swirling solar wind