HR6435 is a multiple main-sequence star in the constellation of Ophiuchus.
HR6435 visual magnitude is 6.02. Because of its reltive faintness, HR6435 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 HR6435:
Celestial coordinates and finder chart of HR6435
HR6435 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 HR6435 are provided in the following table:
The simplified sky map below shows the position of HR6435 in the sky:
Visibility of HR6435 from your location
Digitized Sky Survey image of HR6435
The image below is a photograph of HR6435 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 HR6435 is -0.01 arcsec per year in Right Ascension and -0.021 arcsec per year in Declination and the associated displacement for the next 10000 years is represented with the red arrow.
Distance of HR6435 from the Sun and relative movement
HR6435 is distant 373.00 light years from the Sun and it is moving towards the Sun at the speed of 4 kilometers per second.
Spectral properties of HR6435
HR6435 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 HR6435 is situated in the Hertzsprung–Russell diagram.
HR6435 star system properties
HR6435 is a visual double star which can be observed with the help of medium or large telescopes. The table below shows key information about the HR6435 double sysyem: