Error message

Deprecated function: implode(): Passing glue string after array is deprecated. Swap the parameters in drupal_get_feeds() (line 394 of /home2/dsakers/public_html/sw/includes/common.inc).

Star

Sigma Callade

Primary of Hlekkar.

Spectral type: G6

Giunchig

Primary of Gotlan.

Spectra type: G5

Oepida

Primary of Wakmarrel.

Spectral Class: G7

Delta Illyrius

Primary of Sedante.

Spectral Class: G0

 

Azana

Primary of Midway.

Spectral Class: G2

Meltan

Primary of Hafen.

Spectral class: G3

Alpha Mensae

Primary of Lu Hsing.

Spectral Class: G5

Alpha Mensae is the brightest star in the constellation Mensa. It is a main sequence dwarf star only slightly smaller and cooler in temperature than the Sun.

Alpha Mensae has a relatively high proper motion across the sky, and it is located about 33 light years distant from the Sun. It has a red dwarf companion star at a distance of 3.05 arcseconds (a projected separation of roughly 30 AU).

 

HR 5256

Primary of Gualicho.

HR 5256 is a solitary, K-type main sequence star located thirty-three light-years away in the constellation Ursa Major. It has an estimated 80% of the Sun's mass and 78% of the Sun's radius. The space velocity components of this star are (U, V, W) = (−2, −10, −25) km/s. HR 5256 will make its closest approach to the Sun in about 333,000 ± 16,000 years, when it will be at a distance of 3.9 ± 0.2 parsecs.

HR 511

Primary of Lerna.

HR 511 (also designated Gliese 75 among others) is an orange dwarf of spectral type K0V in the constellation Cassiopeia. The star is relatively close, 32.5 light years from the Sun.

This star is estimated to be about the same age as the sun. It has not been identified as a member of any moving star groups. This star has displayed unusual emissions of Ca II and is much more x-ray luminous than the Sun. It is considered a relatively active star. Based on an iron abundance of [Fe/H] = -0.02, the metallicity of this star appears to be similar to that of the Sun.

 

Pages

Subscribe to RSS - Star