TU Ursae Majoris is a variable star in the northern circumpolar constellation of Ursa Major. It is classified as a Bailey-type 'ab' RR Lyrae variable with a period of 0.557648 days that ranges in brightness from apparent visual magnitude of 9.26 down to 10.24. The distance to this star is approximately 2,090 light years based on parallax measurements. It is located near the north galactic pole at a distance that indicates this is a member of the galactic halo.
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| - TU Ursae Majoris (en)
- TU Большой Медведицы (ru)
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| - TU Большой Медведицы (лат. TU Ursae Majoris) — одиночная переменная звезда в созвездии Большой Медведицы на расстоянии приблизительно 2086 световых лет (около 640 парсеков) от Солнца. Видимая звёздная величина звезды — от +10,24m до +9,26m. (ru)
- TU Ursae Majoris is a variable star in the northern circumpolar constellation of Ursa Major. It is classified as a Bailey-type 'ab' RR Lyrae variable with a period of 0.557648 days that ranges in brightness from apparent visual magnitude of 9.26 down to 10.24. The distance to this star is approximately 2,090 light years based on parallax measurements. It is located near the north galactic pole at a distance that indicates this is a member of the galactic halo. (en)
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| - (en)
- kA2hA9.5 (en)
- kF0hF7.5 (en)
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| - TU Ursae Majoris is a variable star in the northern circumpolar constellation of Ursa Major. It is classified as a Bailey-type 'ab' RR Lyrae variable with a period of 0.557648 days that ranges in brightness from apparent visual magnitude of 9.26 down to 10.24. The distance to this star is approximately 2,090 light years based on parallax measurements. It is located near the north galactic pole at a distance that indicates this is a member of the galactic halo. The periodic variability of this star was discovered by P. Guthnick and R. Prager in 1929. Its relative brightness has made this star the subject of regular observation since its discovery, both photographically and then photoelectrically starting in 1957. It was initially classed as a Bailey-type "a" RR Lyrae variable. The variations were found to be somewhat similar to RR Lyrae, with the periodicity of TU UMa differing by less than 1% of a day. However, no evidence of a long-period modulation, known as the Blazhko effect, was found in this star. In 1990, and found variations in radial velocity over time that suggested this is a binary system. However, confirmation of this proved difficult because of the distance and the pulsational behavior of the variable. The system shows significant evidence of proper motion acceleration from a binary interaction. Analysis of long-term oscillatory variations suggests an orbital period of 23.3 years and an eccentricity of 0.79, with the secondary having at least 33% of the mass of the Sun. (en)
- TU Большой Медведицы (лат. TU Ursae Majoris) — одиночная переменная звезда в созвездии Большой Медведицы на расстоянии приблизительно 2086 световых лет (около 640 парсеков) от Солнца. Видимая звёздная величина звезды — от +10,24m до +9,26m. (ru)
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