42 Aquilae
42 Aquilae is a sub-giant star in the constellation of Aquila.
42 Aquilae visual magnitude is 5.46. Because of its reltive faintness, 42 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 42 Aquilae:
42 Aquilae is above the horizon from Greenwich, United Kingdom .
Altitude: 33.5°
Azimuth: 189.5°
Direction: South
Celestial coordinates and finder chart of 42 Aquilae
42 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 42 Aquilae are provided in the following table:
The simplified sky map below shows the position of 42 Aquilae in the sky:

Visibility of 42 Aquilae from your location
Location: Greenwich, United Kingdom
Latitude: 51° 28’ 47” N
Longitude: 0° 00’ 00” E
Timezone: Europe/London
Today's 42 Aquilae 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 42 Aquilae
The image below is a photograph of 42 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 42 Aquilae is 0.107 arcsec per year in Right Ascension and -0.051 arcsec per year in Declination and the associated displacement for the next 1000 years is represented with the red arrow.

Distance of 42 Aquilae from the Sun and relative movement
42 Aquilae is distant 104.69 light years from the Sun and it is moving towards the Sun at the speed of 38 kilometers per second.
Spectral properties of 42 Aquilae
42 Aquilae belongs to spectral class F3 and has a luminosity class of IV corresponding to a sub-giant star.
The red dot in the diagram below shows where 42 Aquilae is situated in the Hertzsprung–Russell diagram.
