- NGC 2362 (Wikipedia)
NGC 2362, also known as Caldwell 64, is an open cluster of stars in the southern constellation of Canis Major. It was discovered by the Italian court astronomer Giovanni Batista Hodierna, who published his finding in 1654. William Herschel called it a “beautiful cluster”, while William Henry Smyth said it “has a beautiful appearance, the bright white star being surrounded by a rich gathering of minute companions, in a slightly elongated form, and nearly vertical position”. In the past it has also been listed as a nebula, but in 1930 Robert J. Trumpler found no evidence of nebulosity. The brightest member star system is Tau Canis Majoris, and therefore it is sometimes called the Tau Canis Majoris Cluster.
- Gamma Hydrae (stars.astro.illinois.edu)
Skipping over obscure (at least in brightness) fourth magnitude Beta Hydrae (the southernmost of Hydra’s outlining stars), exact third magnitude Gamma Hydrae (3.00) comes in at number two, just beating out a host of slightly lesser stars (such as Nu, Zeta, Pi, and Epsilon).
- Gamma Hydrae (Wikipedia)
Gamma Hydrae (γ Hya, γ Hydrae) is a binary star in the equatorial constellation of Hydra. It has an apparent visual magnitude of 3.0, placing it second in brightness among the members of this generally faint constellation. Based upon parallax measurements made during the Hipparcos mission, this star is at a distance of around 133.8 light-years (41.0 parsecs) from Earth.
