Category Archives: Double/Multiple Stars

Zeta Aquarii (Struve 2909): A Tight Binary Near the Water Bearer’s Shoulder

Zeta Aquarii, a binary star system in Aquarius, is about 92 light-years away. First identified by William Herschel in 1777, it appears as a single point to the naked eye. Both stars are similar F-type main-sequence stars, orbiting each other every 587 years, exhibiting complexity beneath their apparent simplicity. This post explores the star and illustrates what it looks like in the telescope. Also known as: STF 2909, SAO 146108, HIP 110960, GC 31398, HR 8558, Zet1 Aqr, 55 Aquarii, HD 213052, 55 Aqr

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.

Epsilon Arietis: A Rewarding, Tight Binary in Aries

Learn about Epsilon Arietis, a close binary white pair of stars in the constellation Aries, best viewed on autumn and winter nights. The two stars only lie 1.3 arcseconds apart, so a telescope will be needed to see both stars also known as Struve 333, STF 333, Eps Ari, SAO 75673, HD 18519, HR 887, HIP 13914, 48 Ari.

Struve 1850: A Wide Binary Star in Boötes

Struve 1850, a binary star system in the Boötes constellation, consists of two nearly identical A1V stars, easily observable with binoculars or small telescopes. Discovered by Friedrich Struve in 1823, they are over 800 light-years away. Their similar luminosity and proximity make them delightful targets for amateur astronomers. Also known as: STF 1850, HD 127067, SAO 83374, HIP 70786, HR 5414

Beta Draconis (Rastaban): The Dragon’s Eye

Beta Draconis, or Rastaban, is a prominent star in the constellation Draco, with an apparent magnitude of 2.8. This golden giant, situated 380 light-years away, is part of a binary system. Despite its brilliance, its companion is a dimmer star, visible only under optimal conditions. Also known as Bet Dra, Rastaben, Alwaid, Asuia, SAO 30429, HD 159181, 23 Dra, β Dra, 23 Draconis, HIP 85670, HR 6536, BU 1090

Mu Scorpii: A Pleasant Blue Visual Pair of Stars in Scorpius

Mu Scorpii, located in the tail of the Scorpion constellation, comprises two stars, Mu1 and Mu2, which appear close but are at different distances. Mu1 is a binary star system, while Mu2 is less luminous. Observations reveal the beauty of this pair, easily visible with binoculars, reminding us of the wonders of stargazing.

Zeta Sagittae (Struve 2585): A Subtle Triple Star System in the Arrow Sagitta

Sagitta, a small constellation between Aquila and Vulpecula, features Zeta Sagittae, a fascinating triple star system. The brighter component, Zeta Sagittae A, shines at magnitude 5, while its companion, Zeta Sagittae B, is fainter at magnitude 9. Located near Altair, this hidden treasure is worth observing with a telescope. Also known as STF 2585, SAO 105298, 8 Sagittae, HR 7546, HIP 97496, HD 187362