| u-b =
}}{{Starbox astrometry
| radial_v = {{val|-5.48|0.20}}[1]
| prop_mo_ra = {{val|-1.454|0.217}}[1]
| prop_mo_dec = {{val|-13.822|0.177}}[1]
| parallax = 4.4409
| p_error = 0.1180
| parallax_footnote = [1]
}}{{Starbox detail
| source = [10]
| mass =
| radius =
| luminosity = 299.05
| gravity =
| temperature = 4,371
| metal =
| metal_fe =
| rotation =
| rotational_velocity =
| age =
| age_myr =
| age_gyr =
}}{{Starbox catalog
| names = BD+36° 519, SAO 55684, HIP 12072, HR 748.
}}{{Starbox reference
| Simbad = HD+16028
}}{{Starbox end}}HD 16028 is a star in the constellation Andromeda. Its apparent magnitude is 5.71.[ Located approximately {{convert|225|pc|ly}} distant,[1] it is an orange giant of spectral type K3III,[4] a star that has used up its core hydrogen and has expanded.]
Double star catalogues list two stars as optical companions. One has a magnitude of 10.9 and is separated by 16.9 arcseconds. It has been suggested it is related to the primary,[4] but parallax measured by Gaia yields a much greater distance for this star in comparison to HD 16028.[2] The other is even fainter and is separated 45 arcseconds from the primary.[3]
References
1. ^1 2 3 4 5 6 {{cite DR2|333614200354086656}}
2. ^{{cite DR2|333614200354086272}}
3. ^{{cite simbad | title=UCAC4 637-009202 | access-date=January 3, 2019}}
4. ^1 2 3 {{Cite journal | doi = 10.1111/j.1365-2966.2008.13596.x | title = A catalogue of multiplicity among bright stellar systems | date = 2008 | last1 = Eggleton | first1 = P. P. | last2 = Tokovinin | first2 = A. A. | journal = Monthly Notices of the Royal Astronomical Society | volume = 389 | issue = 2 | pages = 869 | bibcode = 2008MNRAS.389..869E |arxiv = 0806.2878 }}
5. ^1 {{citation | display-authors=2 | last1=McDonald | first1=I. | last2=Zijlstra | first2=A. A. | last3=Boyer | first3=M. L. | title=Fundamental parameters and infrared excesses of Hipparcos stars | journal=Monthly Notices of the Royal Astronomical Society | volume=427 | pages=343 | year=2012 | postscript=. | bibcode=2012MNRAS.427..343M | arxiv=1208.2037 | doi=10.1111/j.1365-2966.2012.21873.x }}