1 Aquarii
{{short description|Binary star in the constellation Aquarius}}
{{Starbox begin
| name = 1 Aquarii
}}
{{Starbox image
| image =
{{Location mark
|image=Aquarius constellation map.svg
|float=center
|alt=
|label=
|position=right
|width=280
|mark=Red circle.svg
|mark_width=12
|mark_link=1 Aquarii
|x=958|y=295
}}
| caption = Location of 1 Aqr (circled)
}}
{{Starbox observe
| epoch = J2000
| constell = Aquarius
}}
{{Starbox character
| variable =
}}
{{Starbox astrometry
| radial_v = {{val|−40.93|(3)}}
| prop_mo_ra = {{val|96.805|(120)}}
| prop_mo_dec = {{val|−10.140|(94)}}
| parallax = 12.3852
| p_error = 0.1134
}}
{{Starbox orbit
| primary = 1 Aquarii A
| name = 1 Aquarii B
| period_unitless = {{val|1966.7|2.9}} days
| eccentricity = {{val|0.368|0.009}}
| node =
| periastron = {{val|54740|7}}
| periarg = {{val|150.7|1.6}}
| k1 = {{val|3.24|0.04}}
| k2 =
}}
{{Starbox detail
| temperature = {{val|4715|15}}
}}
{{Starbox catalog
| names = {{odlist | F=1 Aqr | BD=−00°4064 | FK5=3651 | HD=196758 | HIP=101936 | HR=7897 | SAO=126062 | WDS=J20394+0029 | CCDM=J20394+0029 }}{{cite simbad | title=11 Per | access-date=2019-03-28 }}
}}
{{Starbox reference
| Simbad = 1+Aqr
}}
{{Starbox end}}
1 Aquarii is a binary star system in the zodiac constellation of Aquarius, about 263 light years away from the Sun. 1 Aquarii is the Flamsteed designation. It is visible to the naked eye as a faint, orange-hued star with an apparent visual magnitude of 5.151, located a degree north of the celestial equator. The system is moving closer to the Earth with a heliocentric radial velocity of −41 km/s.
Systematic observation for determining the orbit of this system began in 2002, some eighty years following the first radial velocity measurements. It is a single-lined spectroscopic binary with an orbital period of {{Convert|1966.7|days|years|disp=out}} and an eccentricity of 0.368. The visible component is an aging giant star with a stellar classification of K1III. At the age of 1.26 billion years old it is a red clump giant, which indicates it is on the horizontal branch and is generating energy through helium fusion at its core. The star has 1.5 times the mass of the Sun and has expanded to 11 times the Sun's radius. It is radiating 53.7 times the Sun's luminosity from its enlarged photosphere at an effective temperature of 4,715 K.
The mass of the companion appears small, suggesting a red dwarf no higher than class M5. In addition to the spectroscopic companion there are two faint optical companions that have no physical relation to 1 Aqr.
Etymology
1 Aquarii was known to the ancients as al-sa'd al-malik, or "the lucky star of the king." Interpreting the unexpressed Arabic vowels, al-sa'd al-mulk, gives an alternate translation of "the lucky star of the kingdom." In English, the name is Sadalmelik (or Sadalmelek), although rarely used today.[https://academic.oup.com/astrogeo/article/49/5/5.27/422591 A Llnguist's Angle on the Star of Bethlehem — i.e. α Aquarii]; Coates, Richard; Astronomy & Geophysics, Volume 49, Issue 5; (01 October 2008); Pp. 5.27–5.32; https://doi.org/10.1111/j.1468-4004.2008.49527.x[https://www.naic.edu/~gibson/starnames/starnames.html Star Names]; Arecibo Observatory website; mod.: Steve Gibson; accessed March 2019
References
{{Reflist|refs=
{{Cite Gaia DR3|4231171058672649856}}
}}
{{Stars of Aquarius}}
{{DEFAULTSORT:1 Aquarii}}
Category:Horizontal-branch stars
Category:Spectroscopic binaries