HR3335 is a variable and double main-sequence star in the constellation of Pyxis.
HR3335 visual magnitude is 6.56. Because of its reltive faintness, HR3335 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 HR3335:
Celestial coordinates and finder chart of HR3335
HR3335 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 HR3335 are provided in the following table:
The simplified sky map below shows the position of HR3335 in the sky:
Visibility of HR3335 from your location
Digitized Sky Survey image of HR3335
The image below is a photograph of HR3335 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 HR3335 is 0.01 arcsec per year in Right Ascension and -0.008 arcsec per year in Declination and the associated displacement for the next 10000 years is represented with the red arrow.
Distance of HR3335 from the Sun and relative movement
HR3335 is distant 722.84 light years from the Sun and it is moving far from the Sun at the speed of 1 kilometers per second.
Spectral properties of HR3335
HR3335 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 HR3335 is situated in the Hertzsprung–Russell diagram.
HR3335 star system properties
HR3335 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 HR3335 double sysyem: