The Hyades, Melotte 25
Open Cluster Melotte 25
(= Collinder 50 = Caldwell 41)
in Taurus
The Hyades
Right Ascension | 4 : 27 (h:m) |
---|---|
Declination | +16 : (deg:m) |
Distance | 0.150 (kly) |
Visual Brightness | 0.5 (mag) |
Apparent Dimension | 330 (arc min) |
At a distance of only about 150 light years, the Hyades form the nearest open
cluster to us, disregarding the Ursa Major cluster
which appears as spread individual stars. Their distance is quite wellknown
from their motion along a common direction: All member stars move toward a point
slightly east of Betelgeuse (alpha in Orion), about at RA=6:08, Dec=+9.1 degrees.
From their radial velocity, which is about 43 km/sec in recession, and from
their proper motion the distance is not difficult to be derived.
The distance has also been well confirmed by data obtained by ESA’s astrometric
satellite Hipparcos, which found a distance of 151 light years.
The central group is roughly 10 light years in diameter, while outlying members
seem to be spread over a volume of at least 80 light years diameter. The cluster’s
Hertzsprung-Russell diagram corresponds to the HRD of a theoretical cluster of
660 million years age, therefore it is concluded that this cluster is 660 million
years old. This age, as well as the stellar contents of this cluster, and its
proper spatial motion suggests that probably the Hyades have a common origin with
the Praesepe star cluster M44.
In John Caldwell’s observing list.
Last Modification: 8 Mar 1998, 19:55 MET