NGC 457 is looser, and its brightest star, Phi Cassiopeiae, is a white-hued supergiant star of magnitude 5.0.The stars of NGC 457 are around 10,000 light-years away from us, while NGC 663 is closer, at 8,200 light-years, and larger, at 0.25 degrees in diameter.The Heart Nebula, also designated as IC 1805, is situated at around 7,500 light-years away from Earth. Caph has surface average temperatures of around 7,079 K, much hotter than our Sun.Gamma Cassiopeiae, also known as Navi, is the prototype Gamma Cassiopeiae variable star, a type of star that has a variable disc of material flung off by the high rotation rate of the star.Navi occasionally outshines the brightest star in Cassiopeia – Alpha Cassiopeiae, reaching a magnitude of 1.6, due to its variability in brightness.
Ruchbah is 99.4 light-years away from Earth.Ruchbah is a subgiant star on its way into becoming a giant star. The Soul Nebula has an absolute magnitude of 6.5.The Pacman Nebula, designated as NGC 281 – is an H II region, a large gas cloud in which star formation has recently taken place. The star would be around twice the size of our Kappa Cassiopeiae is a blue supergiant situated at around 4,000 light-years away from us. Marfak is located at around 134 light-years away from us.This star is 1.8 times more massive than our Sun, having 2.6 times its radius, and it is also considerably hotter, having average surface temperatures of around 8,202 K.6 Cassiopeiae is a hot white hypergiant star, around 25 times more massive than our Sun, and 200,000 times more luminous. Its magnetic field and wind of particles create a visible bow shock 4 light-years ahead of it, that collides with the diffuse, and usually invisible, interstellar gas and dust.The dimensions of Kappa Cassiopeiae’s bow shock are vast – around 12 light-years long and 1.8 light-years wide.V509 Cassiopeiae is an extremely rare yellow hypergiant star, which is around 400,000 times brighter than our Sun, and 14 times as massive.V509 Cassiopeiae is around 4,500 light-years away from us, and it has an apparent magnitude that has varied from below +6 in historical times to a peak of +4.6, and now around +5.3.It is visible to the naked eye, having a radius between 400 to 900 times that of our Sun. Maffei 2 is below the range of most amateur telescopes.The December Phi Cassiopeiids is a recently discovered early-December meteor shower that radiates from the constellation of Cassiopeia.Phi Cassiopeiids are quite slow, with an entry velocity of around 16.7 km / 10.3 mi per second. It has 249% of our Sun’s mass, 390% its radius, and it is 77 times brighter.Ruchbah is also hotter than our Sun, having average surface temperatures of around 7,980 K.Epsilon Cassiopeiae, also known as Segin, is a hot blue-white star with an apparent magnitude of 3.3. They are:3C 10, also known as Tycho’s Supernova Remnant, is the aftermath of the supernova called Tycho’s star.
This is variously said to represent a woman's hand dyed red with Another Arab constellation that incorporated the stars of Cassiopeia was the Camel. It is an Alpha Cygni variable star, having an apparent magnitude of +5.43.6 Cassiopeiae is situated at around 8,000 light-years away from us. NGC 147 is slightly dimmer, at magnitude 9.3, and it is even farther away, at 2.3 million light-years.Both dwarf galaxies are gravitationally bound to the IC 10 is the closest starburst galaxy to us, at around 2.2 million light-years, and the only starburst galaxy in the Local Group of galaxies. Segin is 9 times more massive than our Sun, having 6 times its radius. Caph is situated at around 54 light-years away from the Sun.Caph is a Delta Scuti variable star, and since it is rotating at around 92% of its critical speed, the star has an oblate spheroid shape with an equatorial bulge that is 24% larger than its polar radius.Caph is 1.9 times more massive than our Sun, and it has around 343% of our Sun’s radius. Its average surface temperatures have been recorded at around 10,023 K.The constellation of Cassiopeia hosts many interesting It contains several open clusters, young luminous galactic disc stars, nebulae, Both clusters have around 80 discovered stars.


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