HR7607
HR7607 is a multiple main-sequence star in the constellation of Cygnus.
HR7607 visual magnitude is 6.57. Because of its reltive faintness, HR7607 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 HR7607:
Celestial coordinates and finder chart of HR7607
HR7607 is situated north of the celestial equator, as such, it is more easily visible from the northern hemisphere. Celestial coordinates for the J2000 equinox as well as galactic coordinates of HR7607 are provided in the following table:
The simplified sky map below shows the position of HR7607 in the sky:

Visibility of HR7607 from your location
Location: Greenwich, United Kingdom
Latitude: 51° 28’ 47” N
Longitude: 0° 00’ 00” E
Timezone: Europe/London
Today's HR7607 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 HR7607
The image below is a photograph of HR7607 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 HR7607 is 0.011 arcsec per year in Right Ascension and 0.017 arcsec per year in Declination and the associated displacement for the next 10000 years is represented with the red arrow.

Distance of HR7607 from the Sun and relative movement
HR7607 is distant 742.60 light years from the Sun and it is moving towards the Sun at the speed of 12 kilometers per second.
Spectral properties of HR7607
HR7607 belongs to spectral class B6 and has a luminosity class of V corresponding to a main-sequence star.
The red dot in the diagram below shows where HR7607 is situated in the Hertzsprung–Russell diagram.

HR7607 star system properties
HR7607 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 HR7607 double sysyem: