The small constellation Triangulum [
http://www.hawastso
] in the northern sky harbors this magnificent face-on spiral galaxy, M33. Its popular names include the Pinwheel Galaxy or just the Triangulum Galaxy [
http://www.seds.org
]. M33's diameter spans over 50,000 light-years, making it third largest in the Local Group [
http://www.anzwers.
] of galaxies after the Andromeda Galaxy (M31), and our own Milky Way. About 3 million light-years from the Milky Way, M33 lies very close to the Andromeda Galaxy [
http://antwrp.gsfc.
] and observers [
http://www.astr.ua.
] in these two galaxies would likely have spectacular views of each other's grand spiral star systems. As for the view from planet Earth, this sharp 27 frame mosaic [
http://www.robgendl
] of M33 nicely shows off blue star clusters and pinkish star forming regions which trace the galaxy's loosely wound spiral arms. In fact, the cavernous NGC 604 [
http://antwrp.gsfc.
] is the brightest star forming region seen here, visible along an arm arcing above and to the right of the galaxy center. Like M31, M33's population of well-measured variable stars have helped make this nearby spiral a cosmic yardstick [
http://cfa-www.harv
] for establishing [
http://adsabs.harva
bib_query?1926ApJ....63..236H ] the distance scale [
http://antwrp.gsfc.
debate96.html ] of the Universe.
explanation
The small constellation Triangulum [ http://www.hawastsoc.org/deepsky/tri/index.html ] in the northern sky harbors this magnificent face-on spiral galaxy, M33. Its popular names include the Pinwheel Galaxy or just the Triangulum Galaxy [ http://www.seds.org/messier/m/m033.html ]. M33's diameter spans over 50,000 light-years, making it third largest in the Local Group [ http://www.anzwers.org/free/universe/localgr.html ] of galaxies after the Andromeda Galaxy (M31), and our own Milky Way. About 3 million light-years from the Milky Way, M33 lies very close to the Andromeda Galaxy [ http://antwrp.gsfc.nasa.gov/apod/ap021021.html ] and observers [ http://www.astr.ua.edu/gifimages/m33.html ] in these two galaxies would likely have spectacular views of each other's grand spiral star systems. As for the view from planet Earth, this sharp 27 frame mosaic [ http://www.robgendlerastropics.com/M33ColorPage.html ] of M33 nicely shows off blue star clusters and pinkish star forming regions which trace the galaxy's loosely wound spiral arms. In fact, the cavernous NGC 604 [ http://antwrp.gsfc.nasa.gov/apod/ap021102.html ] is the brightest star forming region seen here, visible along an arm arcing above and to the right of the galaxy center. Like M31, M33's population of well-measured variable stars have helped make this nearby spiral a cosmic yardstick [ http://cfa-www.harvard.edu/~kstanek/DIRECT/ ] for establishing [ http://adsabs.harvard.edu/cgi-bin/ bib_query?1926ApJ....63..236H ] the distance scale [ http://antwrp.gsfc.nasa.gov/diamond_jubilee/ debate96.html ] of the Universe.
Explanation
false