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Credit & Copyright: Phil Keyser
Explanation:
Big, bright, beautiful
spiral, Messier 106 dominates this cosmic
vista.
The nearly two degree wide
telescopic
field of view looks toward the well-trained constellation
Canes Venatici, near the handle of the Big Dipper.
Also known as NGC 4258, M106 is about 80,000 light-years across and
23.5 million light-years away, the largest member of the
Canes
II galaxy group.
For a far away galaxy, the distance to M106 is well-known
in part because it can be
directly measured
by tracking this galaxy's remarkable maser, or microwave laser emission.
Very rare but naturally occurring, the
maser
emission is produced
by water molecules in molecular clouds orbiting its
active
galactic nucleus.
Another prominent spiral galaxy on the scene, viewed nearly
edge-on,
is NGC 4217 below and right of M106.
The distance to NGC 4217 is much less well-known, estimated
to be about 60 million light-years.
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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: M 106 - spiral galaxy
Publications with words: M 106 - spiral galaxy
See also:
- APOD: 2025 September 4 Á NGC 4565: Galaxy on Edge
- APOD: 2025 August 22 Á A Tale of Two Nebulae
- APOD: 2025 August 19 Á Giant Galaxies in Pavo
- APOD: 2025 August 18 Á NGC 1309: A Useful Spiral Galaxy
- APOD: 2025 July 4 Á NGC 6946 and NGC 6939
- APOD: 2025 June 30 Á NGC 4651: The Umbrella Galaxy
- APOD: 2025 June 19 Á NGC 3521: Galaxy in a Bubble