Your guide to the Solar System and the night sky
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🌎  Observing from: Greenwich, United Kingdom [change]

ο Aquilae (omicron Aquilae)

ο Aquilae is a multiple main-sequence star in the constellation of Aquila.

ο Aquilae visual magnitude is 5.11. Because of its reltive faintness, ο Aquilae 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 ο Aquilae:

5.11
Main-sequence
ο Aquilae (omicron Aquilae) is above the horizon from Greenwich, United Kingdom [change]. Altitude: 31°.

Celestial coordinates and finder chart of ο Aquilae

ο Aquilae 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 ο Aquilae are provided in the following table:

19h 51m 01s
+10° 24’ 56”
49.14°
-8.19°
Aquila

The simplified sky map below shows the position of ο Aquilae in the sky:

Finder chart ο Aquilae (omicron Aquilae) star
Simplified finder chart for ο Aquilae (omicron Aquilae).

Visibility of ο Aquilae from your location

Location: Greenwich, United Kingdom [change]
Latitude: 51° 28’ 47” N
Longitude: 0° 00’ 00” E
Timezone: Europe/London

Today's ο Aquilae (omicron Aquilae) rise, transit and set times from Greenwich, United Kingdom [change] are the following (all times relative to the local timezone Europe/London):

Azimuth: 79.6°
Max altitude: 48.9°
Azimuth: 280.4°
ο Aquilae (omicron Aquilae) is above the horizon from Greenwich, United Kingdom

Digitized Sky Survey image of ο Aquilae

The image below is a photograph of ο Aquilae 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 ο Aquilae is 0.242 arcsec per year in Right Ascension and -0.139 arcsec per year in Declination and the associated displacement for the next 1000 years is represented with the red arrow.

Image of ο Aquilae (omicron Aquilae) star
DSS2 image of ο Aquilae. The red arrow shows the motion of ο Aquilae during the next 1000 years (4.03 arcmin in Right Ascension and -2.32 arcmin in declination);

Distance of ο Aquilae from the Sun and relative movement

ο Aquilae is distant 63.22 light years from the Sun

19.39 pc
63.22 ly
0.242 arcsec/year
-0.139 arcsec/year

Spectral properties of ο Aquilae

ο Aquilae belongs to spectral class F8 and has a luminosity class of V corresponding to a main-sequence star.

3.67
F8V
6170K

The red dot in the diagram below shows where ο Aquilae is situated in the Hertzsprung–Russell diagram.

HR Diagram
H-R diagram showing the position of ο Aquilae. Attribution: Richard Powell / CC BY-SA

ο Aquilae star system properties

ο Aquilae 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 ο Aquilae double sysyem:

5.11
13.41
8.3
14.4 arcsec

Alternative designations of ο Aquilae

ο Aquilae
(omicron Aquilae)
SAO105338
SAO105338
Gl 768.1A