HR2677 is a multiple main-sequence star in the constellation of Puppis.
HR2677 visual magnitude is 6.14. Because of its reltive faintness, HR2677 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 HR2677:
Celestial coordinates and finder chart of HR2677
HR2677 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 HR2677 are provided in the following table:
The simplified sky map below shows the position of HR2677 in the sky:
Visibility of HR2677 from your location
Location: Greenwich, United Kingdom
Latitude: 51° 28’ 47” N
Longitude: 0° 00’ 00” E
Today's HR2677 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 HR2677
The image below is a photograph of HR2677 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 HR2677 is -0.043 arcsec per year in Right Ascension and 0.041 arcsec per year in Declination and the associated displacement for the next 10000 years is represented with the red arrow.
Distance of HR2677 from the Sun and relative movement
HR2677 is distant 181.51 light years from the Sun and it is moving far from the Sun at the speed of 19 kilometers per second.
Spectral properties of HR2677
HR2677 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 HR2677 is situated in the Hertzsprung–Russell diagram.
HR2677 star system properties
HR2677 is a visual double star which can be observed with the help of small or medium telescopes. The table below shows key information about the HR2677 double sysyem: