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🌎  Greenwich, United Kingdom [change]

ι Microscopii (iota Microscopii)

ι Microscopii is a double sub-giant star in the constellation of Microscopium.

ι Microscopii visual magnitude is 5.11. Because of its reltive faintness, ι Microscopii 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 ι Microscopii:

5.11
Sub-giant
ι Microscopii (iota Microscopii) is below the horizon from Greenwich, United Kingdom [change].

Celestial coordinates and finder chart of ι Microscopii

ι Microscopii is situated south of the celestial equator, as such, it is more easily visible from the southern emisphere. Celestial coordinates for the J2000 equinox as well as galactic coordinates of ι Microscopii are provided in the following table:

20h 48m 29s
-43° 59’ 18”
356.83°
-39.02°
Microscopium

The simplified sky map below shows the position of ι Microscopii in the sky:

Finder chart ι Microscopii (iota Microscopii) star
Simplified finder chart for ι Microscopii (iota Microscopii).

Visibility of ι Microscopii from your location

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

ι Microscopii (iota Microscopii) is currently not visible from Greenwich, United Kingdom [change]

Digitized Sky Survey image of ι Microscopii

The image below is a photograph of ι Microscopii 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 ι Microscopii is 0.185 arcsec per year in Right Ascension and -0.106 arcsec per year in Declination and the associated displacement for the next 1000 years is represented with the red arrow.

Image of ι Microscopii (iota Microscopii) star
DSS2 image of ι Microscopii. The red arrow shows the motion of ι Microscopii during the next 1000 years (3.08 arcmin in Right Ascension and -1.77 arcmin in declination);

Distance of ι Microscopii from the Sun and relative movement

ι Microscopii is distant 133.88 light years from the Sun and it is moving towards the Sun at the speed of 15 kilometers per second.

41.07 pc
133.88 ly
-15 km/s
0.185 arcsec/year
-0.106 arcsec/year

Spectral properties of ι Microscopii

ι Microscopii belongs to spectral class F1 and has a luminosity class of IV corresponding to a sub-giant star.

2.04
F1IV
7158K

The red dot in the diagram below shows where ι Microscopii is situated in the Hertzsprung–Russell diagram.

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

ι Microscopii star system properties

ι Microscopii 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 ι Microscopii double sysyem:

5.11
15.51
10.4
4.3 arcsec

Alternative designations of ι Microscopii

ι Microscopii
(iota Microscopii)
SAO230379
SAO230379
Gl 808.1