HR7035
HR7035 is a double main-sequence star in the constellation of Sagittarius.
HR7035 visual magnitude is 5.83. Because of its reltive faintness, HR7035 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 HR7035:
HR7035 is below the horizon from Greenwich, United Kingdom .
Altitude: -32.8°
Azimuth: 89.9°
Direction: East
Celestial coordinates and finder chart of HR7035
HR7035 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 HR7035 are provided in the following table:
The simplified sky map below shows the position of HR7035 in the sky:

Visibility of HR7035 from your location
Location: Greenwich, United Kingdom
Latitude: 51° 28’ 47” N
Longitude: 0° 00’ 00” E
Timezone: Europe/London
Today's HR7035 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 HR7035
The image below is a photograph of HR7035 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 HR7035 is 0.005 arcsec per year in Right Ascension and -0.022 arcsec per year in Declination and the associated displacement for the next 10000 years is represented with the red arrow.

Distance of HR7035 from the Sun and relative movement
HR7035 is distant 793.19 light years from the Sun and it is moving far from the Sun at the speed of 15 kilometers per second.
Spectral properties of HR7035
HR7035 belongs to spectral class B5 and has a luminosity class of V corresponding to a main-sequence star.
The red dot in the diagram below shows where HR7035 is situated in the Hertzsprung–Russell diagram.

HR7035 star system properties
HR7035 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 HR7035 double sysyem: