Rasalgethi - α1 Herculis (alpha1 Herculis)
Rasalgethi, also designated as α1 Herculis (alpha1 Herculis), is a variable and multiple supergiant star in the constellation of Hercules.
Rasalgethi visual magnitude is 3.48. Because of its moderate brightness, Rasalgethi should be easily visible from locations with dark skies, while it can be barely visible, or not visible at all, from skies affected by light pollution.
The proper motion of Rasalgethi is -0.006 arcsec per year in Right Ascension and 0.036 arcsec per year in Declination and the associated displacement for the next 10000 years is represented with the red arrow.
Key facts about Rasalgethi
Rasalgethi - α1 Herculis (alpha1 Herculis) is below the horizon from Greenwich, United Kingdom.
Altitude: -18.3°
Azimuth: 326.6°
Direction: North-North-West
Celestial coordinates and finder chart of Rasalgethi
Rasalgethi is situated close to the celestial equator, as such, it is at least partly visible from both hemispheres in certain times of the year. Celestial coordinates for the J2000 equinox as well as galactic coordinates of Rasalgethi are provided in the following table:
The simplified sky map below shows the position of Rasalgethi in the sky:
Visibility of Rasalgethi from your location
Location: Greenwich, United Kingdom
Latitude: 51° 28’ 47” N
Longitude: 0° 00’ 00” E
Timezone: Europe/London
Today's Rasalgethi - α1 Herculis (alpha1 Herculis) rise, transit and set times from Greenwich, United Kingdom are the following (all times relative to the local timezone Europe/London):
Distance of Rasalgethi from the Sun and relative movement
Rasalgethi is distant 382.18 light years from the Sun and it is moving towards the Sun at the speed of 33 kilometers per second.
Spectral properties of Rasalgethi
Rasalgethi belongs to spectral class M5 and has a luminosity class of I corresponding to a supergiant star.
The red dot in the diagram below shows where Rasalgethi is situated in the Hertzsprung–Russell diagram.
Rasalgethi star system properties
Rasalgethi is a visual double star which can be observed with the help of small or medium telescopes. The table below shows key information about the Rasalgethi double sysyem: