HR2895 is a double main-sequence star in the constellation of Puppis.
HR2895 visual magnitude is 6.3. Because of its reltive faintness, HR2895 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 HR2895:
HR2895 is below the horizon from Greenwich, United Kingdom .
Celestial coordinates and finder chart of HR2895
HR2895 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 HR2895 are provided in the following table:
The simplified sky map below shows the position of HR2895 in the sky:
Visibility of HR2895 from your location
Location: Greenwich, United Kingdom
Latitude: 51° 28’ 47” N
Longitude: 0° 00’ 00” E
Today's HR2895 rise, transit and set times from Greenwich, United Kingdom are the following (all times relative to the local timezone Europe/London):
Digitized Sky Survey image of HR2895
The image below is a photograph of HR2895 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 HR2895 is -0.012 arcsec per year in Right Ascension and 0.005 arcsec per year in Declination and the associated displacement for the next 10000 years is represented with the red arrow.
Distance of HR2895 from the Sun and relative movement
HR2895 is distant 739.23 light years from the Sun and it is moving far from the Sun at the speed of 23 kilometers per second.
Spectral properties of HR2895
HR2895 belongs to spectral class B9 and has a luminosity class of V corresponding to a main-sequence star.
The red dot in the diagram below shows where HR2895 is situated in the Hertzsprung–Russell diagram.
HR2895 star system properties
HR2895 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 HR2895 double sysyem: