2014. Kaler, James B. "Epsilon Ursae Minoris". Stars. University of Illinois. Retrieved 21 June 2014. "Epsilon Ursae Minoris – Variable of RS CVn type"...

Epsilon Ursae Minoris (ε Ursae Minoris) is a binary star system in the northern circumpolar constellation of Ursa Minor. It is visible to the naked eye...

arrives at the North Celestial Pole and the star Polaris (α UMi/Alpha Ursae Minoris), the North Star. Rigil Kentaurus (α Centauri) and Hadar (β Centauri)...

Epsilon Indi, Latinized from ε Indi, is a star system located at a distance of approximately 12 light-years from Earth in the southern constellation of...

الجَوْن Epsilon Ursae Majoris Alkaid al-Qā'id (banāt naʽash) the Leader (of the mourning maidens) القائد بنات نعش القائِد بَنات نَعْش Eta Ursae Majoris...

IC 2602 Open Cluster. HD 206610 (Bosona) 482 ± 2 1 K0III 8.34 Gamma Ursae Minoris (Pherkad) 487 ± 8 1 A2 III 3.05 XO-2S 489 ± 1 2 K0V + K0V 11.12±0.03...

Kepler-42 (KOI-961) 130.8 ± 0.1 1 M5V +16.12 Has 3 exoplanets. Beta Ursae Minoris (Kochab) 130.9 ± 0.6 1 K4 III +2.08 Tau Centauri 131 ± 3 1 A0 V or A1...

traditional star names, there were some coined in modern times, e.g. "Avior" for Epsilon Carinae (1930), and a number of stars named after people (mostly in the...

Sigma Sagittarii Star 2.07 Alpha Ophiuchi Binary star system 2.08 Beta Ursae Minoris Star 2.10 Gamma Andromedae Quadruple star system 2.11 2.0 Beta Gruis...

Trianguli 171.8 ± 0.2 2 M2+? 13.366±0.006 Has one known exoplanet. Delta Ursae Minoris (Yildun) 172 ± 1 1 A1 Van 4.36 39 Arietis (Lilii Borea) 172 ± 2 1 K1...

Bibliography - Image. HD 4391 at SIMBAD - Ids - Bibliography - Image. 20 Leonis Minoris at SIMBAD - Ids - Bibliography - Image. Nu Phoenicis at SIMBAD - Ids -...

1 B9V HD 77946 322.7±1 1 F5 Has one known exoplanet. Polaris (Alpha Ursae Minoris/North Star/Pole Star) 323–433 3 F7Ib + F6 + F3V The closest star to...

brightness too close. The previous pole star was Kochab (Beta Ursae Minoris, β UMi, β Ursae Minoris), the brightest star in the bowl of the "Little Dipper"...

Milky Way galaxy. The secondary is a flare star that is referred to as WX Ursae Majoris. It is characterized as a UV Ceti-type variable star that displays...

21h 06m 53.94s +38° 44′ 57.9″ 11.4 B K7.0V 6.05 8.33 Procyon (α Canis Minoris) A F5IV-V 0.40 2.68 07h 39m 18.12s +05° 13′ 30.0″ 11.5 ε Indi K5Ve 4.69...

"Preliminary results of the spectral analysis of Suzaku data of SW Ursae Majoris and BZ Ursae Majoris", New Astronomy, 25: 1–6, Bibcode:2013NewA...25....1I...

(2007-01-01). "MOST Detects g-Modes in the Late-Type Be Star β Canis Minoris (B8 Ve)". The Astrophysical Journal. 654 (1): 544–550. arXiv:astro-ph/0609460...

004 MJ or 3.1 M🜨. The longest period of any confirmed exoplanet is 47 Ursae Majoris d, which takes 14002 days or 38.33 years to make one trip around...

stars B M? 0.11 13.27 15.58 C M? 0.10 14.03 16.34 Procyon (Alpha Canis Minoris) A$ 11.402 ±0.032 CMi* 07h 39m 18.1s +05° 13′ 30″ F5IV–V 1.499 0.38# 2...

Moon, including Antares and 119 Tauri. Examples of eclipsing binaries are Epsilon Aurigae (Almaaz), VV Cephei, and V766 Centauri (HR 5171). Angular diameter...

have its existence confirmed. It is a hot Jupiter with a 4.2-day orbit. 47 Ursae Majoris b: In 1996 this Jupiter-like planet was the first long-period planet...

Comae Berenices b 19.4 326.03 1.29 radial vel. 2007 304.54 2.7 4742 11 Ursae Minoris b 14.74 516.21997 1.53 radial vel. 2009 410.06 2.78 4213 14 Andromedae...