HR7599 is a double main-sequence star in the constellation of Aquila.
HR7599 visual magnitude is 6.51. Because of its reltive faintness, HR7599 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 HR7599:
Celestial coordinates and finder chart of HR7599
HR7599 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 HR7599 are provided in the following table:
The simplified sky map below shows the position of HR7599 in the sky:
Visibility of HR7599 from your location
Digitized Sky Survey image of HR7599
The image below is a photograph of HR7599 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 HR7599 is 0.036 arcsec per year in Right Ascension and -0.046 arcsec per year in Declination and the associated displacement for the next 10000 years is represented with the red arrow.
Distance of HR7599 from the Sun and relative movement
HR7599 is distant 279.35 light years from the Sun and it is moving towards the Sun at the speed of 7 kilometers per second.
Spectral properties of HR7599
HR7599 belongs to spectral class F2 and has a luminosity class of V corresponding to a main-sequence star.
The red dot in the diagram below shows where HR7599 is situated in the Hertzsprung–Russell diagram.
HR7599 star system properties
HR7599 is a visual double star which can be observed only with the help of very large telescopes. The table below shows key information about the HR7599 double sysyem: