The author shares about seeing the dwarf planet Pluto from Tampa, Florida using a Seestar S50. Photos of the planet are included.
Xi Serpentis (Nehushtan): A Triple Star in Serpens
Nehushtan, or Xi Serpentis, is a triple star system in the Serpens constellation, 105 light-years away. It will approach within 27 light-years in about 700,000 years. Named after a biblical idol, it showcases the intertwining of astronomy and faith. Observations highlight its brightness and challenging visibility of companions. Also known as 55 Ser, Xi Ser, SAO 160700, HD 159876, HIP 86263, HR 6561, GC 23881
Beta Serpentis: Binary Star and Traveler in the Ursa Major Group
Beta Serpentis is a binary star in the summer constellation Serpens. Of note, the pair also belong to the Ursa Major Moving Group.
La Superba: One of the Reddest Stars in the Sky
One night, La Superba appeared randomly on my astronomy app while I navigated the springtime sky. I stared at the map for a moment, scratched my head, and believed the name to be a mistake. I pressed the information icon by the reddish pixel to reveal a summary of La Superba, including the fact thatContinue reading "La Superba: One of the Reddest Stars in the Sky"
95 Herculis: A Summertime Binary Star of Ruby and Emerald
95 Herculis is a colorful binary star, looking like ruby and emerald gems placed together on black velvet. The binary lies in the constellation Hercules and is enjoyed on summer nights. Also known as 95 Her, SAO 85648, STF 2264, HD 164669.
Iota Cancri: A Beautiful Double Star of Gold and Blue
Iota Cancri is a beautiful double star in the constellation Cancer. It's best viewed in the spring with its gold and blue color. It's a great object in small scopes.
Mu Cephei: The Beautiful Garnet Star in Cepheus
Mu Cephei, also known as the Garnet Star, is a red supergiant star in the constellation Cepheus. It's best viewed in autumn.
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