HR4841 is a supergiant star in the constellation of Musca.
HR4841 visual magnitude is 6.16. Because of its reltive faintness, HR4841 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 HR4841:
Celestial coordinates and finder chart of HR4841
HR4841 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 HR4841 are provided in the following table:
The simplified sky map below shows the position of HR4841 in the sky:
Visibility of HR4841 from your location
HR4841 is currently not visible from Greenwich, United Kingdom [change]
Digitized Sky Survey image of HR4841
The image below is a photograph of HR4841 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 HR4841 is -0.032 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 HR4841 from the Sun and relative movement
HR4841 is distant 1,940.48 light years from the Sun and it is moving towards the Sun at the speed of 3 kilometers per second.
Spectral properties of HR4841
HR4841 belongs to spectral class F6 and has a luminosity class of I corresponding to a supergiant star.
The red dot in the diagram below shows where HR4841 is situated in the Hertzsprung–Russell diagram.