Gomeisa: The Shining Blue Jewel of Canis Minor

Gomeisa, or Beta Canis Minoris, is a striking blue-white B-type star located 170 light-years from Earth in Canis Minor. With a surface temperature over 11,000 Kelvin and a brightness of magnitude 2.9, it stands out near Procyon. Its rapid rotation and classification as a variable star add to its intrigue for astronomers.

HD 39881 (S 503): A Wide Double Star in Orion

Orion is a prominent winter constellation known for its bright stars, including Betelgeuse and the Orion Nebula, as well as double stars like S 503. This system, consisting of components A and B, offers viewing opportunities with binoculars and telescopes. Recent observations highlighted their visibility despite fading dawn light. Also known as SAO 95004, HD 39881, HR 2067, HIP 28066, BD+13 1036, GC 7469, 0728-03142-1

The Horsehead Nebula (IC 434): A Shadow in the Stars

The Horsehead Nebula, located in Orion, is recognized for its iconic silhouette but is faint and challenging to observe. First discovered in 1888 by Williamina Fleming, it is a stellar nursery contributing to star formation. Ideal viewing occurs between December and March, away from city lights using larger telescopes.

Struve 700 (V1804 Orionis): Double Blue in Orion’s Winter Cool

Learn about the double star in Orion called Struve 700 and V1804 Orionis. The pretty set of blue-white stars shine around 7.8 magnitude and are a tight pair in telescope. My sketch shows what the binary looks like through a backyard telescope. They are a great pair to seek out when observing through Orion, the hunter, on winter days.