Haggart Observatory

Obects & Observing Tips:

Nebulae

Diffuse Nebulae   Planetary Nebulae    Supernova Remnants

Orion Nebula, NASA photo
[NASA photo, APOD]

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Diffuse (star-forming) Nebulae:
These are areas of hot, glowing gas in which new stars are condensing; they are very dramatic objects, though the stunning colors seen in photographs are not visible to the human eye, even through a telescope. (Our eyes "refresh" too frequently to pick up the colors, except for possibly a bit of pinkish glow in large amateur telescopes. Computer imaging and photographic plates can collect light over long periods.) Because they are so young - only a few million years old, with ongoing star formation - they still contain extremely massive, bright but short-lived, O and B type stars.
( Check out the SEDS explanation of diffuse nebula.)

Observing Diffuse Nebulae:

Best Bets:
There are only a few of these fine objects available. (Links are to the SEDS website description.)

Nebula Constellation Availability by month Mag. Dist.
(ly)
Diam
(ly)
J F M A M J J A S O N D
M8: Lagoon
Sagittarius
- - - - - - X X X - - -
6
5,200
136
M17: Omega, Swan
Sagittarius
- - - - - - X X X - - -
6
5,000
75
M20: Trifid
Sagittarius
- - - - - - X X X - - -
8
5,200
44
M42 / M43: Orion Orion X X X - - - - - - - X X
4
1,600
30
M78 Orion X X X - - - - - - - X X
8.3
1,600
4

 


"Planetary" (dying star) Nebulae:
star in final stages of life cycle has "blown off" much of its surface layers, or "atmosphere" into an expanding ring or dumb-bell shaped cloud
the remnant of the central star is a "white dwarf"

binoculars: dim, hard to spot with any light pollution
telescopes: spot with low power, use high power to view (24mm or less)

  Constellation J F M A M J J A S O N D Mag Dist (ly) Diam (ly) Age (yrs)
 M27: Dumbbell Vulpecula - - - - - X X X X X X -
7.4
1,250
2
?
 M57: Ring Lyra - - - - X X X X X X X -
8.8
2,300
2.4
8,000
M76: Little Dumbbell Perseus X X X - - - - - - X X X
10.1
3,400
2.6
?
M97: Owl Ursa Major - X X X X X X X X - - -
9.9
2,600
?
6,000

[It is apparently very hard to determine distances to planetary nebulae, and diameter and age estimates depend on the distance; different authors report wildly varying distances. SEDS gives age estimates on the Dumbbell of 4,000 years from one study and 48,000 years on another]


Supernova Remnants:

  Constellation J F M A M J J A S O N D Mag Dist (ly)
 M1: Crab Nebula
Taurus
X X X - - - - - - - X X
8.4
6,300

The Crab Nebula is the remnant of a supernova that appeared in 1054 AD.


Data sources:

SEDS "Diffuse Nebulae" website: www.seds.org/messier/diffuse.html
(note on ages: if several given, I've used the one attributed to Sky Catalog 2000)

Sky and Telescope Messier Card, 1997

Watson, Brent. Finder Charts of the Messier Objects, 1993

(Monthly availability determined from star charts in Rey, The Stars: a New Way to See Them and at Heavens-Above.com)