Overview:
Messier
51 (M51) is probably the best known and one of the most often
observed galaxy in the northern hemisphere. It lies in the
direction of the constellation
Canes
Venatici. This constellation is Latin for the "hunting dogs" and often
associated as the dogs of
Bootes, the Herdsman, a bordering constellation. M51 is also
called the Whirlpool Galaxy due to its resemblance to a
whirlpool of liquid. It is one of the brightest and most
beautiful of spiral galaxies. Also cataloged as NGC 5194 (center
galaxy) and NGC 5195 (galaxy just to upper right of center) in the
New General Catalogue (abbreviated NGC). M51 is another
example of colliding galaxies where the larger galaxy on the
left, NGC 5194, may absorb the smaller right side galaxy, NGC
5195.
Details: . The M51 pair of galaxies is about 30 million
light years away, therefore with a visual diameter of about 10
minutes of arc (1/6 of a degree), simple trigonometry calculates
a size of about 75 thousand light years or about 70% the size of
our Milky Way galaxy. Its mass is only about 10% of our galaxy
at about 150 million suns, compared to the 1.5 trillion suns of
our galaxy. While these two massive galaxies
may be passing each other and just shaking hands, most likely
NGC 5195 has passed through the galactic plane of NGC 5194
multiple times, caused increased star formation along the arms,
and currently lies behind the larger galaxy. Even through small
telescopes the pair of galaxies is visible; through a 6-8"
telescope you can start to resolve the wonderful galaxy arms.
Note how the arms of NGC 5194 are slightly bent, likely due to
the gravitational distortion of NGC 5195.
M51 is also a
Seyfert galaxy, which accounts for about 10% of all
galaxies. Seyferts have very active central cores powered
similarly to those of quasars, but much closer by and less
luminous. We now know that supermassive black holes surrounded
by accretion disks of doomed material dominate the centers of
these galaxies. Visible on the left side of NGC 5194 is a group
of red colored emission nebula, contrasted over the blue spiral star
arms. The red color indicates gas and dust being excited by
nearby stars. The blue color shows areas of active star
formation, where young hot stars glow blue-white. Finally the
ghostly white areas around the galaxy are 100s of millions of
stars, like our sun, so far away that they appear as faint
cloudy puffs of smoke.
Annotations. In the image
above, hover a mouse or curser over the image to show
annotations of the galaxy with several enlarged insets
identifying interesting features! Beginning at the top, 12
o’clock position, clearly visible are two visually smaller
galaxies IC 4278 and IC 4279 in the
Index Catalogue, or IC Catalogue, the first major update to
the NGC Catalogue mentioned above. Continuing clockwise, next
are two very exciting phenomena.
First, is the detection
of a very distant
quasar at 11.1 billion light years away, meaning it’s light
left it when the universe was only 2-3 billion years old and way
before our earth and sun even existed!. Today the universe is
about 13.7 billion years old. Quasar is short for quasi-stellar
object or QSO. They are extremely bright active galaxies powered
by
supermassive black holes of tens of billions of solar
masses. This means 10,000,000,000 suns have been squeezed into
an infinitesimally small point. Their brightness can exceed
thousands of times the brightness of our whole Milky Way galaxy
of 200 billion suns. Because they are so far away, they are
likely the cores of very young, very active galaxies and since
our universe is expanding faster the further an object is away
from us, they have highly
red shifted spectrums.
This Quasar,
designated J133004.71+472301.0 is a galaxy with a redshift near
3.0, meaning it is moving away from us at nearly 90% the speed
of light, is 11 billion years old, and was 11 billion light
years away at the time its light left it. Today however it is
nearly 18 billion light years away from us and therefore outside
of our visible universe. Light leaving it today will never reach
us.
Continuing clockwise in the above image, a second exciting phenomena is an apparent jet of
blue material that can be seen just to the right of the core of
NGC 5195 as annotated. This is likely a jet of newly formed
stars being disrupted, perhaps even expelled into intergalactic
space by the merging galaxies. There are trillions of stars in
intergalactic space not associated with a parent galaxy.
Civilizations inhabiting these star systems would never know the
beauty of the Milky Way like we do. Continuing clockwise are
insets showing the neculei of both NGC 5195 and NGC 5195, as
well as nebulae within the M51 galaxy. Some of these nebulae may
be as large and bright as our own
Orion
Nebula, and someday space telescopes may resolve as much
detail.
Below Images: In the first image below,
the same image has been processed to remove all foreground stars
as these stars are all within our own Galaxy. This is what the
view would appear like if no stars existed along our line of
sight and what we would see outside of our own galaxy. Using a
mouse to hover over the image, brings all the stars back.
The second image below shows an enlarged and cropped version of
M51 and this time hovering a mouse makes the stars disappear.
Finally, the third image below is the same image, same data with
my previous pre- and post- processing workflow. Hovering over
the third below image shows a direct comparison to the current
processing workflow using PixInsight software for the majority
of stacking and sharpening, with Photoshop use for final touch-up.
Note the improved color throughout the image from object to
stars, as well as the visibilty and more natural look of very
faint stars and object details.
Object Statistics:
Constellation: Canes Venatici, Right Ascension: 13h 29m 53.3s,
Declination: +47° 11' 48, Magnitude: 9.0 (B), Size: 10.3'x8.1',
Class: SA(s)bc pec.