Hubble image archive
Hubble Probes the Halo of the Andromeda Galaxy
This diagram shows how scientists determined the size of the halo of the Andromeda galaxy. Because the gas in the halo is dark, the team measured it by using the light from quasars, the very distant bright cores of active galaxies powered by black holes. They observed the quasars...
- Date
- Jan 1, 2015
- Mission
- Hubble Space Telescope
- Archive ID
- hubblesite-images-2015-15-3538-image
This diagram shows how scientists determined the size of the halo of the Andromeda galaxy. Because the gas in the halo is dark, the team measured it by using the light from quasars, the very distant bright cores of active galaxies powered by black holes. They observed the quasars' light as it traveled through the intervening gas. The halo's gas absorbed some of that light and made the quasar appear darker in a very small wavelength range. By measuring the tiny dip in brightness at that specific range, scientists could tell how much gas is between us and each quasar. Some quasars showed no dip in brightness, and this helped define the size of the halo.
Credits
Illustration: NASA, ESA, and A. Feild (STScI);Science: NASA, ESA, N. Lehner and J.C. Howk (University of Notre Dame), and B. Wakker (University of Wisconsin, Madison)
Image Details
| About The Object | |
|---|---|
| Object Name | M31, Andromeda Galaxy, Messier 31, NGC 224 |
| Object Description | Spiral Galaxy, halo |
| R.A. Position | 00h 42m |
| Dec. Position | +41° 15' |
| Constellation | Andromeda |
| Distance | Redshift: 2.5 million light-years (0.8 megaparsecs) |
| About The Data | |
| Data Description | Ultraviolet observations of multiple quasi-stellar objects (QSOs) seen through the extended circumgalactic medium around M31 were obtained from various HST proposals. Studies of these archival data led to the results found. The science team comprises: N. Lehner and J.C. Howk (University of Notre Dame), and B. Wakker (University of Wisconsin, Madison). |
| Instrument | HST>COS/FUV |
| Filters | Gratings: G130M, G160M |
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Image and source material are credited to the official mission archive linked below.
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