110 Herculis is a variable and multiple main-sequence star in the constellation of Hercules.
110 Herculis visual magnitude is 4.19. Because of its moderate brightness, 110 Herculis should be easily visible from locations with dark skyes, while it can be barely visible, or not visible at all, from skyes affected by light pollution.
The table below summarizes the key facts about 110 Herculis:
Celestial coordinates and finder chart of 110 Herculis
110 Herculis 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 110 Herculis are provided in the following table:
The simplified sky map below shows the position of 110 Herculis in the sky:
Visibility of 110 Herculis from your location
Digitized Sky Survey image of 110 Herculis
The image below is a photograph of 110 Herculis from the Digitized Sky Survey 2 (DSS2 - see the credits section) taken in the red channel. The area of sky represented in the image is 0.5x0.5 degrees (30x30 arcmins). The proper motion of 110 Herculis is -0.008 arcsec per year in Right Ascension and -0.335 arcsec per year in Declination and the associated displacement for the next 1000 years is represented with the red arrow.
Distance of 110 Herculis from the Sun and relative movement
110 Herculis is distant 62.25 light years from the Sun and it is moving far from the Sun at the speed of 24 kilometers per second.
Spectral properties of 110 Herculis
110 Herculis belongs to spectral class F6 and has a luminosity class of V corresponding to a main-sequence star.
The red dot in the diagram below shows where 110 Herculis is situated in the Hertzsprung–Russell diagram.
110 Herculis star system properties
110 Herculis is a visual double star which can be observed only with the help of very large telescopes. The table below shows key information about the 110 Herculis double sysyem: