The North America Nebula (NGC 7000)

Posted by ayiomamitis
on Monday, July 26, 2010
by Anthony Ayiomamitis

The expansive emission nebula NGC 7000, more commonly referred to as the North America Nebula owing to its characteristic shape, is a large area of nebulosity lying to the immediate southeast of Deneb (α-Cyg) and is equivalent to about twelve full moons in apparent area. NGC 7000 is active in star formation and includes three clusters, namely NGC 6989 to the northwest, NGC 6996 to the north and NGC 6997 to the west. NGC 7000 lies at a distance of 2,200 light-years away and is estimated to span 100 light-years across. To its right and separated by a dark absorption cloud is the also expansive Pelican emission nebula (IC 5067 and IC 5070). Similarly, to its bottom right is the smaller emission nebula IC 5068. The North America nebula is best observed using low magnifications (50-100x) during mid-summer preferably under dark skies as it approaches zenith around midnight and using either a UHC or O-III filter. NGC 7000 was discovered by William Herschel in 1786.

The section depicted by the "Gulf of Mexico" in the image below is more commonly referred to as "The Great Cygnus Rift" and represents the starting point of dust clouds which continue onto Aquila and Ophiuchus and bisect our Milky Way in half when viewed edge-on, for the dust obscures starlight and yields the observer darkened lanes or nebulae stretching for one thousand light-years across. These dark nebulae expand in size as one moves away from Cygnus and progresses southwards towards Aquila and Ophiuchus. The Great Cygnus Rift, also known as the Northern Coalsack, is also an area of very active star formation and only two thousand light-years away from the two other major star formation areas in the general vicinity, namely NGC 7000 (North America Nebula) and IC 5070 (Pelican Nebula).

Technical Details:
Date: July 17-18, 2010 @ 22:35 - 01:50 UT+3 and July 18-19, 2010 @ 23:30 - 01:35 UT+3
Location: Athens, Greece (38.2997° N, 23.7430° E)
Equipment: Takahashi FSQ-106/f5, AP 1200GTO GEM, SBIG ST-10XME, SBIG CFW10, SBIG LRGB filters
Integrations: HaRGB @ 160:40:40:40 using 10-/20-min subs, 1x1 binning, 2.65"/pixel, -10.0d C

Further details are available here.

Comments
To leave a comment you must be a member of our community.
Login to your account now, or register for an account to start participating.
No one has commented yet.
Join our Community!

Our community is FREE to join. To participate you must either login or register for an account.

ADVERTISEMENT
FREE EMAIL NEWSLETTER

Receive news, sky-event information, observing tips, and more from Astronomy's weekly email newsletter. View our Privacy Policy.

ADVERTISEMENT
ADVERTISEMENT
Find us on Facebook