|
Instrument |
Celestron
C11 @ ~f/10.48 (2930 mm fl) 1.27 arcsec / pixel, resampled to
1.91 arcsec / pixel. |
Mount |
Paramount ME |
Camera |
SBIG STL-11000 w/
internal filter wheel, AstroDon Filters |
Acquisition Data |
3/7/2008 to 4/4/2008
Chino Valley... with CCDAutoPilot3 |
Exposure |
Lum
360 min. (36 x 10 bin 2x2)
RGB 240 min. (8 x 10 bin 3x3) each |
Software |
CCDSoft,
Sigma-Clip, Photoshop CS w/ the Fits Liberator plugin, Paint Shop
Pro, and Noel
Carboni's actions |
Comment |
North is to the
top.
Spiral galaxy M94 has a ring of newly formed stars surrounding its
nucleus, giving it not only an unusual appearance but also a strong
interior glow. A leading hypothesis holds that an elongated knot of
stars known as a bar rotates in M94 and has generated a burst of
star formation in the form of an outward moving ring. M94 spans
about 30,000 light years, lies about 15 million light years away,
and can be seen with a small telescope toward the constellation of
Canes Venatici.
Source: NASA APOD |
|