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Theta Aquarii

A yellow subgiant-giant star in Aquarius, named Ancha.

Theta Aquarii is a star in the equatorial constellation of Aquarius, designated by the Bayer name θ Aquarii. It is visible to the naked eye with an apparent visual magnitude of 4.175 and lies approximately 191 light-years from the Sun. The star bears the official name Ancha, approved by the International Astronomical Union's Working Group on Star Names in 2016.

Quick Facts

Bayer designation
θ Aquarii
Apparent visual magnitude
4.175
Distance from sun
191 ly
Radial velocity
−14 km/s
Spectral class
G8 III–IV
Age
437 million years
Effective temperature
4,864 K

Facts from the source article.

Lore & Background

The star's traditional name Ancha derives from Medieval Latin for 'the haunch'. In 2016, the International Astronomical Union organized a Working Group on Star Names (WGSN) to catalogue and standardize proper names for stars; the WGSN approved the name Ancha for this star on 12 September 2016, and it is now included in the List of IAU-approved Star Names. In Chinese, the asterism known as Weeping consists of Theta Aquarii and Rho Aquarii; consequently, the Chinese name for Theta Aquarii itself is derived from that asterism. Possibly, the name Lei, meaning 'tears (weeping)' in Chinese, derives from the Chinese name for this star.

Ancha belongs to the spectral class G8 with a luminosity class of III–IV, suggesting that at an age of 437 million years, this star is part way between the subgiant and giant stages of its evolution. Estimates of the star's mass range from 2.39 to 2.78 times the Sun's mass, with a radius of about 12 times that of the Sun. It radiates from 72 to 83 times as much luminosity as the Sun from its enlarged outer envelope at an effective temperature of 4,864 K. At this heat, the star glows with the yellow hue of a G-type star.

Reader's Guide

Theta Aquarii, known as Ancha, holds significance as a named star in the equatorial constellation of Aquarius, with its Bayer designation and traditional name formally recognized by the International Astronomical Union. Its position near the ecliptic makes it subject to occultation by the Moon and, very rarely, by planets, a characteristic that has drawn observational interest. The star's spectral classification of G8 III–IV places it in a transitional evolutionary stage between a subgiant and a giant, offering insight into stellar evolution for stars of roughly 2.4 to 2.8 solar masses. Its measured radial velocity of −14 km/s indicates it is drifting closer to the Sun, a kinematic detail that contributes to understanding its motion through the galaxy. The Chinese asterism Weeping, which includes Theta Aquarii and Rho Aquarii, connects the star to cultural astronomy, with the possible derivation of the name Lei from this context. As a naked-eye object at magnitude 4.175, Ancha remains accessible to amateur observers and serves as a reference point in the constellation. Its legacy is anchored in both modern astronomical cataloging and historical naming traditions, bridging ancient Chinese asterisms and medieval Latin nomenclature with contemporary IAU standards.

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