HR4313 is a main-sequence star in the constellation of Antlia.
HR4313 visual magnitude is 5.43. Because of its reltive faintness, HR4313 should be visible only from locations with dark skyes, while it is not visible at all from skyes affected by light pollution.
The table below summarizes the key facts about HR4313:
Celestial coordinates and finder chart of HR4313
HR4313 is situated south of the celestial equator, as such, it is more easily visible from the southern emisphere. Celestial coordinates for the J2000 equinox as well as galactic coordinates of HR4313 are provided in the following table:
The simplified sky map below shows the position of HR4313 in the sky:
Visibility of HR4313 from your location
Digitized Sky Survey image of HR4313
The image below is a photograph of HR4313 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 HR4313 is -0.017 arcsec per year in Right Ascension and 0.004 arcsec per year in Declination and the associated displacement for the next 10000 years is represented with the red arrow.
Distance of HR4313 from the Sun and relative movement
HR4313 is distant 530.08 light years from the Sun and it is moving far from the Sun at the speed of 11 kilometers per second.
Spectral properties of HR4313
HR4313 belongs to spectral class A2 and has a luminosity class of V corresponding to a main-sequence star.
The red dot in the diagram below shows where HR4313 is situated in the Hertzsprung–Russell diagram.