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Created by Jon K. Olson (WT5L)

M101 Spiral Galaxy (LRGB)

Messier 101 is a prominent face-on spiral galaxy in the constellation Ursa Major. One of the last entries in Messier's list of comet "imposters", M101 is estimated to lie at a distance of around 24 million light years from Earth. M101 is most conspicuous for its luminous star forming regions (HII) lying in its outer spiral arms. Many of these regions are so large they have been given their own NGC number. M101 is also famous for its marked asymmetrical appearance that is believed to have been caused by a near collision with another galaxy in its recent (speaking in galactic terms) past. The tidal waves from this near-collision may also be responsible for triggering the strong star formation activity in the spiral arms.

M101 Spiral Galaxy (LRGB)

Image Details


Target: M101, NGC 5457
Coordinates (Center - J2000): RA 14h 03m 26s ; Dec +54d 19m 42s
Date: 13 & 14 April 2007
Constellation: Ursa Major
Imaging Location: Chiefland, Florida
Camera: SBIG ST-8XME & CFW-10 Color Filter Wheel
Filters: Astrodon Series E Tru-Balance LRGB
Telescope: Takahashi TSA-102S 4" APO Triplet f/8 (FL = 814mm)
Mount: Takahashi EM-200 Temma II GEM (12 VDC)
Image Scale: 2.28 arcseconds per pixel
CCD Temperature: -15 C
L:R:G:B Exposures: 90:50:50:50 minutes (10 min. sub-exposures)
Mount Control Software: The Sky 6.0.0.52
Camera Control Software: CCDSoft 5.00.182
Focus Control Software: FocusMax 3.3.15
Executive Control Software: CCD Commander 1.4.5
Sub-frame Registration Software: Registar
Calibration and Combining Software: CCDStack
Final Processing Software: Photoshop CS

CCD Commander Info

Additional Information

Description of M101 (By Rob Gendler):    http://www.robgendlerastropics.com/M101text.html