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Credit & Copyright: Bob Franke
Explanation:
Now known to be a globular star cluster at the tender
age of 10 billion years,
M71 is
a mere 13,000 light-years
away within the narrow boundaries of the faint constellation Sagitta.
Close to the plane of the Milky Way galaxy in
planet Earth's sky, its 10,000 or so member stars are
gathered into a region about 27 light-years across near the center of
this color composite view.
In fact, the line-of-sight to M71 passes along
the galactic plane through much intervening
diffuse interstellar dust.
The dust dims starlight and scatters blue light more efficiently,
masking the brightness
of M71's stars
and shifting true star colors toward the red.
How much are the star colors shifted?
Slide your cursor over the image (or follow
this link)
to use an estimate of the dust reddening or
galactic extinction
to correct the star colors in M71.
Corrections to the brightness and colors of M71 member stars are needed
to measure the cluster's distance and age using a
Color-Magnitude diagram.
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NASA Web Site Statements, Warnings, and Disclaimers
NASA Official: Jay Norris. Specific rights apply.
A service of: LHEA at NASA / GSFC
& Michigan Tech. U.
Based on Astronomy Picture
Of the Day
Publications with keywords: globular cluster - extinction - dust
Publications with words: globular cluster - extinction - dust
See also:
- APOD: 2026 July 31 Á NGC 4372 and the Dark Doodad
- APOD: 2026 July 22 Á The Corona Australis Cloud and the Chandelier Cluster
- APOD: 2026 July 9 Á The Red Glow of the Cosmic Bat Nebula
- APOD: 2026 May 23 Á Messier 2
- LDN 1622: Dark Nebula in Orion
- NGC 7023: The Iris Nebula
- APOD: 2025 December 28 Á NGC 1898: Globular Cluster in the Large Magellanic Cloud