Whitby & District Astronomical Society

One of the many delights of observing the Winter night sky is noting the diverse range of Open Clusters visible to the naked eye, binoculars and telescope alike.  But what is an Open Cluster?

Open Clusters: clusters of young stars (usually no older than 500 million yrs) of roughly the same age, born from the same large cloud of gas (like the Orion Nebula) and are now only just starting to slowly move away from their stellar nursery (due to the pull of other stars in the spiral arms of our galaxy).  Open clusters sometimes, called Galactic clusters, range in size from a few tens of stars up to a few thousand stars.  Related to open clusters are Associations, very loose groupings of stars of common origin. 

Let us now take a tour of the more prominent open clusters visible in the winter sky starting with M45, the Pleiades or "Seven sisters", found to the upper right of Aldeberan, in Taurus.  This distinctive cluster is one of the jewels of the heavens, especially when viewed at low power, i.e.  with binoculars.  In a scope up to 50 stars are visible, though not in the same field.  The cluster actually contains over 350 members lying some 400 light-years away.  It is estimated that the cluster is around 100 million years old.  A good example of a loose cluster is the Hyades, the “v” shape of stars dominated by Aldeberan in Taurus.  This is an illusion as Aldeberan is half the distance of the Hyades members. 

Next find the constellation of Auriga high above Taurus and marked by the prominent star Capella.  Using binoculars sweep the area between Theta and Iota Aurigae you will notice 3 faint hazy patches, these are the open clusters M36, M37 and M38. 

M38 (top) and M36 are seen in the same binocular field, M37 is situated to the lower left.  For small scopes, M36 is probably the finest of the trio - a pretty knot of jewel like blue stars seen against the hazy light of dozens of cluster members.  It lies 4000 light-years away. 

For larger scopes M37 is the more impressive, appearing more like a loose Globular cluster than an open cluster.  It is 4,500 light-years away.  M38 is better to resolve than M37, though fainter than M36, it lies 4000 light-years away.

Most open clusters are formed in the plane of the galaxy, where the effects of gravity eventually disperse the cluster members, M67 is unusual in that it lies 1,500 light-years above the galactic plane, some 2,500 light-years away, well away from the gravitational pull of other stars and consequently the cluster has stayed and evolved together.  The estimated age of the 500 cluster members is around 7 billion years, older than our solar system.

From Cancer, head southwards to find the brightest star in the sky, Sirius, in Canis Major.  Place dazzling Sirius at the top of your binocular / finder scope field and move slightly downwards.  You should find a lumpy patch of light; this is the open cluster M41 a rather pleasing collection of 3 dozen or so stars visible in small instruments.  M41 is another distant cluster lying over 2,100 light-years away. 

Next, sight from Mirzam (the bright-ish star to the right of Sirius) through Sirius and continue for twice that distance to an area in the constellation of Puppis ( you can also sight down through Orion’s belt to this same area).  Through binoculars / finder scope, a small cloud of light should be visible, this is the open cluster M47, and under dark skies M46, another open cluster is just visible next to M47.

In small scopes M47 resolves easily into a group of stars, M46 still resembles a hazy patch of light, though in 6’’ scopes or larger M46 is the more impressive.  Even though these clusters appear next to each other in the sky, in reality M46 is over 3 times further away than M47, 5,000 light-years compared to 1,500 light-years.  A third open cluster in Puppis can be found 2-3 binocular fields to the South-East of M46/7, though M93 can be hard to pick out in the “murk” above the South horizon.        

Returning to Sirius imagine a line extended to Procyon, the bright star up to the North-East.  in Canis Major.  A third of the way along this trajectory, in the constellation of Monoceros you will find the faint open cluster M50.  a collection of 100 stars 3,000 light-years distant

Our final port of call is in Orion, or should I say it is Orion.  For apart from “ruddy” Betelguese which is closer, many of the stars situated in and around the main body of Orion are associated.  Most are hot blue stars (Rigel) formed from the same giant molecular cloud several hundred million years ago which are now drifting apart.

I have concentrated on winter open clusters visible in the South aspect of the night sky. There are many other well placed open clusters in the northern half, but these can wait for another time.  Good hunting!

Image Credits: NASA

In this month's Sky Notes:

• Planetary Skylights
• Meteor Activity
• Winter Solstice Photos
• November 2014 Sky Charts

Planetary Skylights

The Winter Solstice

The Sun reached its lowest position in the sky on December 21st this year and we asked for your Solstice photos for the website.  As it turned out, sun was particularly scarce that day, but with a day's leeway either way, here are some Solstice photos.

Crescent moon over Ravenscar taken by Paul Ming (20-Dec-2014 07:15h)	Solstice Clouds from Victoria Garden Ctr taken by Andi (21-Dec-2014)
Solstice Clouds from Whalebones taken by Andi (21-Dec-2014)	First sun after Solstice from Pannett Park taken by Andi (22-Dec-2014)

 

January 2015 Sky Charts

Click each image to see a full-size Sky Chart:

Looking South Mid January - 21:30h	Looking North Mid January - 21:30h
Looking East Mid January - 21:30h	Looking West Mid January - 21:30h
Overview Mid-January - 21:30h

Image Credits:

• Planets and Comets where not otherwise mentioned: NASA
• Sky Charts: Stellarium Software