| 39 | | ||'''April'''|| || || || || || || || || || || || || || || |
| | 39 | ||'''April'''|| ||M 81 + M 82|| ||interacting galaxy pair|| ||7.9, 9.3|| ||37' separation|| ||>= 10"|| ||M 81 appears as a fuzzy white spot; M 82 is fainter and noticeably elongated. Quoth the APOD: "The gravity from each galaxy dramatically affects the other during each hundred million-year pass. Last go-round, M82's gravity likely raised density waves rippling around M81, resulting in the richness of M81's spiral arms. But M81 left M82 with violent star forming regions and colliding gas clouds so energetic the galaxy glows in X-rays. In a few billion years only one galaxy will remain."|| || ||[http://apod.nasa.gov/apod/ap080325.html 1] [http://www.seds.org/messier/m/m081.html 2] [http://www.seds.org/messier/m/m082.html 3] [http://en.wikipedia.org/wiki/Messier_81 4] [http://en.wikipedia.org/wiki/Messier_82 5]|| |
| | 40 | || || ||Beehive Cluster (M44)|| ||open star cluster|| ||3.7|| ||95'|| ||>= binoculars|| ||~100 stars fully resolved in a small telescope. 600 lyr away, 700 Myr old|| ||[http://www.seds.org/messier/m/m044.html 1]|| |
| | 41 | || || ||Mizar & Alcor|| ||Binary Star|| ||2.2 mag|| ||11.8' apart|| ||>=Binoculars|| ||Bright double star, easy to find in big dipper.|| |
| | 42 | || || || M 37 || || open cluster || || 6.2 || || 24' || || || || || ||[http://www.seds.org/messier/m/m037.html 1]|| |
| | 43 | || || || M 35 || || open cluster || || 5.3 || || 28' || || || || || ||[http://www.seds.org/messier/m/m035.html 1]|| |