HD 112028 is an evolved star in the northern constellation of Camelopardalis. It has spectral peculiarities that have been interpreted as a shell, and also relatively weak magnesium and silicon lines. Its spectral class has been variously assigned between B9 and A2, and its luminosity class between a subgiant and bright giant. At an angular separation of 21.47″ is the slightly fainter spectroscopic binary HD 112014, consisting of a pair of A-type main sequence stars. HD 112028 and HD 112014 together are known as the binary star Struve 1694.
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| - HD 112028 (en)
- HD 112028 (sv)
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| - HD 112028 is an evolved star in the northern constellation of Camelopardalis. It has spectral peculiarities that have been interpreted as a shell, and also relatively weak magnesium and silicon lines. Its spectral class has been variously assigned between B9 and A2, and its luminosity class between a subgiant and bright giant. At an angular separation of 21.47″ is the slightly fainter spectroscopic binary HD 112014, consisting of a pair of A-type main sequence stars. HD 112028 and HD 112014 together are known as the binary star Struve 1694. (en)
- HD 112028 är en ensam stjärna i den norra delen av stjärnbilden Giraffen. Den har en skenbar magnitud av ca 5,28 och är svagt synlig för blotta ögat där ljusföroreningar ej förekommer. Baserat på parallaxmätning inom Hipparcosuppdraget på ca 5,6 mas, beräknas den befinna sig på ett avstånd på ca 600 ljusår (ca 180 parsek) från solen. Den rör sig bort från solen med en heliocentrisk radialhastighet på ca 2 km/s. (sv)
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| - HD 112028 is an evolved star in the northern constellation of Camelopardalis. It has spectral peculiarities that have been interpreted as a shell, and also relatively weak magnesium and silicon lines. Its spectral class has been variously assigned between B9 and A2, and its luminosity class between a subgiant and bright giant. At an angular separation of 21.47″ is the slightly fainter spectroscopic binary HD 112014, consisting of a pair of A-type main sequence stars. HD 112028 and HD 112014 together are known as the binary star Struve 1694. (en)
- HD 112028 är en ensam stjärna i den norra delen av stjärnbilden Giraffen. Den har en skenbar magnitud av ca 5,28 och är svagt synlig för blotta ögat där ljusföroreningar ej förekommer. Baserat på parallaxmätning inom Hipparcosuppdraget på ca 5,6 mas, beräknas den befinna sig på ett avstånd på ca 600 ljusår (ca 180 parsek) från solen. Den rör sig bort från solen med en heliocentrisk radialhastighet på ca 2 km/s. (sv)
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