γ Crateris (gamma Crateris)

γ Crateris is a double main-sequence star in the constellation of Crater.

γ Crateris visual magnitude is 4.08. Because of its moderate brightness, γ Crateris 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 γ Crateris is -0.098 arcsec per year in Right Ascension and 0.004 arcsec per year in Declination and the associated displacement for the next 1000 years is represented with the red arrow.

Key facts about γ Crateris

Celestial coordinates and finder chart of γ Crateris

γ Crateris 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 γ Crateris are provided in the following table:

The simplified sky map below shows the position of γ Crateris in the sky:

Visibility of γ Crateris from your location

Today's γ Crateris (gamma Crateris) rise, transit and set times from Greenwich, United Kingdom are the following (all times relative to the local timezone Europe/London):

Distance of γ Crateris from the Sun and relative movement

γ Crateris is distant 83.80 light years from the Sun and it is moving far from the Sun at the speed of 1 kilometers per second.

Spectral properties of γ Crateris

γ Crateris belongs to spectral class A5 and has a luminosity class of V corresponding to a main-sequence star.

The red dot in the diagram below shows where γ Crateris is situated in the Hertzsprung–Russell diagram.

γ Crateris star system properties

γ Crateris 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 γ Crateris double sysyem:

Alternative designations of γ Crateris