Cassiopeia
2655 OBJECTSCassiopeia is the W of five bright stars on the far side of the pole from the Plough, which makes it the other reliable way of finding north. It never sets from most of the northern hemisphere, so the W turns through the year and is as often an M. It lies along the plane of the Milky Way and is crowded with star clusters, and it holds the site of Tycho's supernova of 1572, one of the handful ever recorded in this galaxy.
Cassiopeia holds 2655 catalogued objects: 2375 stars, 130 galaxies, 50 neutron stars, 50 exoplanets, 33 star clusters, 13 nebulae, 4 unclassified.
STARS · 2375GALAXIES · 130NEUTRON STARS · 50EXOPLANETS · 50STAR CLUSTERS · 33NEBULAE · 13UNCLASSIFIED · 4
[
BRIGHTEST OBJECTS
] 12 SHOWNNAME
CLASS
MASS
DISTANCE
MAG
CONSTELLATION
Cih
B0.5IVpe blue-white subgiant
—
549.1 ly
2.15 V
Cassiopeia
Schedar
K0-IIIa orange giant
—
228.2 ly
2.24 V
Cassiopeia
Caph
F2III yellow-white giant
—
54.74 ly
2.28 V
Cassiopeia
Ruchbah
A5IV white subgiant
—
99.41 ly
2.66 V
Cassiopeia
Segin
B3Vp_sh blue-white main-sequence star
—
411.8 ly
3.35 V
Cassiopeia
Achird
F9V yellow-white main-sequence star
—
19.42 ly
3.46 V
Cassiopeia
Fulu
B2IV blue-white subgiant
—
593.0 ly
3.69 V
Cassiopeia
50 Cas
A2V white main-sequence star
—
157.1 ly
3.95 V
Cassiopeia
NGC 771
Star
—
—
3.95 V
Cassiopeia
15 κ Cas
BC0.7Ia blue-white star
—
—
4.17 V
Cassiopeia
33 θ Cas
A7V white main-sequence star
—
133.6 ly
4.34 V
Cassiopeia
ι Cas
A3IIIpSr+F5V white giant
—
132.9 ly
4.46 V
Cassiopeia
[
COMMON QUESTIONS
] 8 ANSWERED- Where in the sky is Cassiopeia?
- Its boundary is centred near right ascension 0h 49m, declination +59.6°. It stands at its highest around midnight in earlyOctober, which puts it in the evening sky for the two months after that and behind the Sun half a year later.
- Can I see it from where I live?
- Every part of Cassiopeia clears the horizon from latitudes between 8° S and the north pole. Outside that band some or all of the region never rises at all, whatever the time of year — a constellation is fixed on the sky, and it is your latitude that decides how much of the sky you get.
- What is the brightest thing in it?
- The brightest catalogued object in Cassiopeia is Cih, at apparent magnitude 2.15 (V). That is apparent brightness — how it looks from Earth — so it mixes how much light a thing gives off with how far away it is, and the brightest object in a region is rarely the most interesting one.
- How are the stars in it named?
- The brightest carry Greek letters, assigned roughly in order of brightness — by Johann Bayer in 1603, and for the deep southern constellations by Nicolas-Louis de Lacaille in the 1750s — followed by the Latin genitive of the constellation's name. Fainter naked-eye stars north of about −30° take a number from John Flamsteed's catalogue, which never covered the far south, and fainter still a designation from whichever survey recorded them.
- What exactly are the boundaries?
- Lines of constant right ascension and declination, drawn by Eugène Delporte for the IAU in 1930 and referred to the sky as it stood in 1875. Precession has tilted the sky against them since, which is why the boundaries on a modern chart are very slightly askew.
- Are the stars in Cassiopeia actually near each other?
- Almost never. The stars in a constellation lie at wildly different distances and are not related to one another in any way — the pattern is a line of sight from one particular planet. Two stars that look adjacent can be a hundred times further apart than either is from the Sun.
- What is the difference between a constellation and an asterism?
- A constellation is one of the 88 regions the IAU recognises, with a fixed boundary and an official name. An asterism is any memorable pattern that is not one — the Plough inside Ursa Major, the Summer Triangle drawn across three constellations, the Great Square shared between two.
- Why are the names in Latin?
- Because the list was assembled in Latin. Fifty of the 88 descend from Ptolemy's second-century catalogue of forty-eight — his ship Argo was later cut into three — and the rest were coined between the sixteenth and eighteenth centuries to fill the southern sky and the gaps. The genitive form is what star names use: Alpha Orionis means the alpha star of Orion.