Visualize in real time the position of the Cassiopeia constellation in the sky.
General presentation
Its position near the north celestial pole makes it visible for much of the year, and it never completely disappears below the horizon for many observers. Cassiopeia is widely used as a reference point in the sky because it is located opposite Ursa Major in relation to the North Star. It thus makes it easy to orient oneself, even without instruments.
Shape of the Cassiopeia constellation
The constellation of Cassiopeia has a very characteristic W or M shape, depending on its position in the sky. This form consists of five relatively bright main stars that draw a broken line easily identifiable. This zigzag-shaped visual signature is what makes Cassiopeia so easy to recognize, even for beginners. Unlike other constellations that require an effort of imagination, Cassiopeia is directly visible as a geometric figure in the sky.
Stars of the Cassiopeia constellation
Star
Magnitude
Distance
Equatorial position J2000
Current Equatorial Position
Current Horizontal Position at Marseille
Link
Alpha Cassiopeiae
2.23
228 light years
Right ascension : 0ʰ40ᵐ30.441ˢ Declination : 56°32'30.441″
Right ascension : 0ʰ42ᵐ1.6253412844ˢ Declination : 56°40′49.099629782″