15 Aquarii
15 Aquarii is a main-sequence star in the constellation of Aquarius.
15 Aquarii visual magnitude is 5.82. Because of its reltive faintness, 15 Aquarii 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 15 Aquarii:
15 Aquarii is below the horizon from Greenwich, United Kingdom .
Altitude: -25.5°
Azimuth: 297.4°
Direction: West-North-West
Celestial coordinates and finder chart of 15 Aquarii
15 Aquarii 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 15 Aquarii are provided in the following table:
The simplified sky map below shows the position of 15 Aquarii in the sky:

Visibility of 15 Aquarii from your location
Location: Greenwich, United Kingdom
Latitude: 51° 28’ 47” N
Longitude: 0° 00’ 00” E
Timezone: Europe/London
Today's 15 Aquarii 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 15 Aquarii
The image below is a photograph of 15 Aquarii 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 15 Aquarii is 0.011 arcsec per year in Right Ascension and 0.015 arcsec per year in Declination and the associated displacement for the next 10000 years is represented with the red arrow.

Distance of 15 Aquarii from the Sun and relative movement
15 Aquarii is distant 978.98 light years from the Sun and it is moving towards the Sun at the speed of 9 kilometers per second.
Spectral properties of 15 Aquarii
15 Aquarii 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 15 Aquarii is situated in the Hertzsprung–Russell diagram.
