Spiral Galaxy M101 - Hubble Space Telescope
Ssc2009 03b2

Credit: NASA, ESA, K. Kuntz (JHU), F. Bresolin (University of Hawaii), J. Trauger (Jet Propulsion Lab), J. Mould (NOAO), Y.-H. Chu (University of Illinois, Urbana), and STScI

Observation • February 10th, 2009 • ssc2009-03b2

ssc2009-03b2

Messier 101 has a pancake-like shape that we view face-on. This perspective shows off the spiral structure that gives it the nickname the Pinwheel Galaxy. In this Hubble image, taken in visible light, the bright blue clumps are regions where new stars have formed. The yellowish core consists mainly of old stars. The dark brown dust lanes are colder and denser regions where interstellar clouds may collapse to form new stars. All of these features are shaped into a beautiful spiral pattern by a combination of gravity and rotation. Astronomers use visible light to study where and how stars form in spiral galaxies.

About the Object

Name
Pinwheel GalaxyMessier 101M101
Type
Galaxy > Type > Spiral
Galaxy > Activity > Normal
Distance
27,000,000 Light Years
Redshift
0.0008

Color Mapping

Band Wavelength Telescope
Optical 435 nm Hubble ACS
Optical 555 nm Hubble ACS
Infrared 814 nm Hubble ACS