HR7048 is a multiple main-sequence star in the constellation of Serpens.
HR7048 visual magnitude is 5.83. Because of its reltive faintness, HR7048 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 HR7048:
Celestial coordinates and finder chart of HR7048
HR7048 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 HR7048 are provided in the following table:
The simplified sky map below shows the position of HR7048 in the sky:
Visibility of HR7048 from your location
Digitized Sky Survey image of HR7048
The image below is a photograph of HR7048 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 HR7048 is 0.015 arcsec per year in Right Ascension and -0.011 arcsec per year in Declination and the associated displacement for the next 10000 years is represented with the red arrow.
Distance of HR7048 from the Sun and relative movement
HR7048 is distant 708.70 light years from the Sun and it is moving towards the Sun at the speed of 11 kilometers per second.
Spectral properties of HR7048
HR7048 belongs to spectral class A1 and has a luminosity class of V corresponding to a main-sequence star.
The red dot in the diagram below shows where HR7048 is situated in the Hertzsprung–Russell diagram.
HR7048 star system properties
HR7048 is a visual double star which can be observed with the help of large telescopes. The table below shows key information about the HR7048 double sysyem: