March Targets
These are deep sky targets seen from Caltech 7-10PM Local in March.
Object |
Alternative Names |
Type |
Brightness |
Surface Brightness |
Size |
Suggested Telescope/Eyepiece |
Notes |
Links for More Information |
Pleiades |
M45, Subaru |
open cluster |
1.6 |
11.1 |
110' |
>= 8" with 32mm+ eyepiece |
100 Myr-old star cluster, 440 lyr away, containing ~500 members total. |
Astropixels SEDS Wikipedia |
Orion Nebula |
M42 |
emission nebula |
4.0 |
13.1 |
85' x 60' |
>= 8" with 32mm+ eyepiece |
Bright emission nebula inside the nearest star-forming region. The four 1 Myr-old "Trapezium" stars at the heart are responsible for ionizing the surrounding gas and making it glow. 1.3 klyr away. |
Astropixels SEDS Wikipedia |
Beehive Cluster |
M44 |
Open Cluster |
3.1 |
12.1 |
90' |
>= 10" |
750 Myr old, 600 lyr away |
Astropixels SEDS Wikipedia |
Double Cluster |
NGC869 + NGC884 Caldwell 14 |
Open Cluster |
3.8 |
10.9 |
60' |
>= 10" |
Two bright, resolved star clusters side by side. Need wide FOV. Both are young clusters, 7 klyr away, ~14 Myr old, containing luminous B stars |
Astropixels SEDS Wikipedia |
Owl Cluster |
NGC457, Dragonfly Cluster, ET Cluster |
Open Cluster |
6.4 |
12.6 |
13' |
>= 8" |
10 klyr distant cluster shaped like a bird with wings, with two bright stars for eyes. Brightest of "eyes" is foreground star, dimmer is a cluster member |
Starchart Wikipedia |
Christmas Tree Cluster |
NGC2264, Cone Nebula |
Open Cluster |
3.9 |
8.25 |
20' |
>= 8" |
Young star cluster embedded in faint emission nebula; 2.6 klyr away, ~3 Myr old; brightest member is a binary O star |
SEDS Wikipedia |
Alcor & Mizar |
Horse and Rider, Handle of Big Dipper |
Double Star |
0.33 |
- |
14" apart |
>= 6" |
Historically used by many cultures as a test of vision to identify the two stars separately; 85 lyr away. |
Space.com Wikipedia |