HR7435
HR7435 is a double main-sequence star in the constellation of Pavo.
HR7435 visual magnitude is 6.39. Because of its reltive faintness, HR7435 should be visible only from locations with dark skies, while it is not visible at all from skies affected by light pollution.
The proper motion of HR7435 is 0.032 arcsec per year in Right Ascension and -0.043 arcsec per year in Declination and the associated displacement for the next 10000 years is represented with the red arrow.
Key facts about HR7435
HR7435 is below the horizon from Greenwich, United Kingdom.
Altitude: -44.4°
Azimuth: 146.5°
Direction: South-South-East
Celestial coordinates and finder chart of HR7435
HR7435 is situated south of the celestial equator, as such, it is more easily visible from the southern hemisphere. Celestial coordinates for the J2000 equinox as well as galactic coordinates of HR7435 are provided in the following table:
The simplified sky map below shows the position of HR7435 in the sky:
Visibility of HR7435 from your location
Location: Greenwich, United Kingdom
Latitude: 51° 28’ 47” N
Longitude: 0° 00’ 00” E
Timezone: Europe/London
HR7435 is currently not visible from Greenwich, United Kingdom
Distance of HR7435 from the Sun and relative movement
HR7435 is distant 335.39 light years from the Sun and it is moving towards the Sun at the speed of 14 kilometers per second.
Spectral properties of HR7435
HR7435 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 HR7435 is situated in the Hertzsprung–Russell diagram.
HR7435 star system properties
HR7435 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 HR7435 double sysyem: