ψ Persei (psi Persei)

ψ Persei is a variable main-sequence star in the constellation of Perseus.

ψ Persei visual magnitude is 4.23. Because of its moderate brightness, ψ Persei should be easily visible from locations with dark skyes, while it can be barely visible, or not visible at all, from skyes affected by light pollution.

The table below summarizes the key facts about ψ Persei:

Color of ψ Persei ⬤

Magnitude of ψ Persei 4.23

Class Main-sequence

VISIBILITY RIGHT NOW ψ Persei (psi Persei) is above the horizon from Greenwich, United Kingdom [change]. Altitude: 60°.

Celestial coordinates and finder chart of ψ Persei

ψ Persei 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 ψ Persei are provided in the following table:

Right Ascension J2000 03h 36m 29s

Declination J2000 +48° 11’ 34”

Galactic Longitude 149.17°

Galactic Latitude -6.09°

Constellation Perseus

The simplified sky map below shows the position of ψ Persei in the sky:

Simplified finder chart for ψ Persei (psi Persei).

Visibility of ψ Persei from your location

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

ψ Persei (psi Persei) is circumpolar and transits at 15:44 UTC (altitude: 86.7°)

Digitized Sky Survey image of ψ Persei

The image below is a photograph of ψ Persei 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 ψ Persei is 0.024 arcsec per year in Right Ascension and -0.026 arcsec per year in Declination and the associated displacement for the next 10000 years is represented with the red arrow.

DSS2 image of ψ Persei. The red arrow shows the motion of ψ Persei during the next 10000 years (4.00 arcmin in Right Ascension and -4.33 arcmin in declination);

Distance of ψ Persei from the Sun and relative movement

ψ Persei is distant 699.57 light years from the Sun and it is moving towards the Sun at the speed of 1 kilometers per second.

Distance (parsec) 214.59 pc

Distance (light year) 699.57 ly

Heliocentric radial velocity -1 km/s

Proper Motion RA 0.024 arcsec/year

Proper Motion Dec -0.026 arcsec/year

Spectral properties of ψ Persei

ψ Persei belongs to spectral class B5 and has a luminosity class of V corresponding to a main-sequence star.

Absolute magnitude -2.43

Spectral Type B5V

Color Index (B-V) -0.06

Temperature of ψ Persei 10941K

The red dot in the diagram below shows where ψ Persei is situated in the Hertzsprung–Russell diagram.

H-R diagram showing the position of ψ Persei. Attribution: Richard Powell / CC BY-SA

Alternative designations of ψ Persei

Bayer designation ψ Persei
(psi Persei)

Flamsteed designation 37 Persei

Henry Draper Catalogue HD22192

SAO Catalogue SAO38980

Hipparcos Catalogue HIP16826

Durchmusterung Catalogue BD+47 857

General Catalogue of Variable Stars Psi Per

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Other stars in Perseus