Multiwavelength Astronomy Multimedia


Title

X-ray Moon and X-ray Star

Description

This image of the Moon in X-rays was made in 1991 using data from the Roentgen Satellite (ROSAT), an X-ray observatory. In this picture, pixel brightness corresponds to X-ray intensity. The Moon reflects lower energy X-rays (shown as red) from the Sun. The source of high energy X-rays (shown as yellow) is a distant binary star system. The background is speckled with X-rays from many distant, powerful active galaxies. The picture also shows the Moon passing in front of of and obscuring the binary star, a phenomenon called occultation.

Instrument

ROSAT

Subject

  • Moon
  • Star

Spectral Type

X-ray

Date Created

1991

Credits

Max-Planck-Institut für extraterrestrische Physik (MPE), NASA

Type

Observation

Associated Lesson

X-Ray History

This material is based upon work supported by NASA under Grant Nos. NNX09AD33G and NNX10AE80G issued through the SMD ROSES 2009 Program.

Any opinions, findings, and conclusions or recommendations expressed in this website are those of the author(s) and do not necessarily
reflect the views of the National Aeronautics and Space Administration.