HR4692 is a main-sequence star in the constellation of Musca.
HR4692 visual magnitude is 6.21. Because of its reltive faintness, HR4692 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 HR4692:
Celestial coordinates and finder chart of HR4692
HR4692 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 HR4692 are provided in the following table:
The simplified sky map below shows the position of HR4692 in the sky:
Visibility of HR4692 from your location
HR4692 is currently not visible from Greenwich, United Kingdom [change]
Digitized Sky Survey image of HR4692
The image below is a photograph of HR4692 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 HR4692 is -0.056 arcsec per year in Right Ascension and -0.015 arcsec per year in Declination and the associated displacement for the next 10000 years is represented with the red arrow.
Distance of HR4692 from the Sun and relative movement
HR4692 is distant 322.77 light years from the Sun and it is moving towards the Sun at the speed of 8 kilometers per second.
Spectral properties of HR4692
HR4692 belongs to spectral class B9 and has a luminosity class of V corresponding to a main-sequence star.
The red dot in the diagram below shows where HR4692 is situated in the Hertzsprung–Russell diagram.