Close to the Great Bear (Ursa Major) and surrounded by the stars [
http://www.enchante
constellations.shtml ] of the Hunting Dogs (Canes Venatici), this celestial nebula was discovered [
http://www.seds.org
] in 1781 by the metric [
http://www.britanni
] French astronomer Pierre Mechain [
http://www.seds.org
pmechain.html ]. Later, it was added to the catalog of his friend and colleague Charles Messier as M106 [
http://www.seds.org
]. Modern deep telescopic views reveal it to be an island universe [
http://antwrp.gsfc.
] -- a spiral galaxy around 30 thousand light-years across located only about 21 million light-years beyond the stars of the Milky Way. Youthful blue star clusters and reddish stellar nurseries trace the striking spiral arms of M106. Seen so clearly in this beautiful image [
http://www.noao.edu
], the galaxy's bright core is also visible across the spectrum [
http://coolcosmos.i
multiwavelength_astr onomy/multiwavelengt h_astronomy/ ] from radio to x-rays, making M106 a nearby example of the Seyfert class [
http://antwrp.gsfc.
] of active galaxies. The bright core of a Seyfert galaxy is believed to be powered by matter falling into a massive central black hole [
http://csep10.phys.
smblack.html ].
Explanation
Close to the Great Bear (Ursa Major) and surrounded by the stars [
http://www.enchante
constellations.shtml ] of the Hunting Dogs (Canes Venatici), this celestial nebula was discovered [
http://www.seds.org
] in 1781 by the metric [
http://www.britanni
] French astronomer Pierre Mechain [
http://www.seds.org
pmechain.html ]. Later, it was added to the catalog of his friend and colleague Charles Messier as M106 [
http://www.seds.org
]. Modern deep telescopic views reveal it to be an island universe [
http://antwrp.gsfc.
] -- a spiral galaxy around 30 thousand light-years across located only about 21 million light-years beyond the stars of the Milky Way. Youthful blue star clusters and reddish stellar nurseries trace the striking spiral arms of M106. Seen so clearly in this beautiful image [
http://www.noao.edu
], the galaxy's bright core is also visible across the spectrum [
http://coolcosmos.i
multiwavelength_astr onomy/multiwavelengt h_astronomy/ ] from radio to x-rays, making M106 a nearby example of the Seyfert class [
http://antwrp.gsfc.
] of active galaxies. The bright core of a Seyfert galaxy is believed to be powered by matter falling into a massive central black hole [
http://csep10.phys.
smblack.html ].
Explanation