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  2. Betelgeuse - Wikipedia

    en.wikipedia.org/wiki/Betelgeuse

    Betelgeuse's color may have changed from yellow (or possibly orange; i.e. a yellow supergiant) to red in the last few thousand years, based on a 2022 review of historical records. This color change combined with the CMD suggest a mass of 14 M ☉ and age of 14 Myr, and a distance from 125 to 150 parsecs (~400 to 500 light years). [12]

  3. Yellow supergiant - Wikipedia

    en.wikipedia.org/wiki/Yellow_supergiant

    Yellow supergiants generally have spectral types of F and G, although sometimes late A or early K stars are included. [1] [2] [3] These spectral types are characterised by hydrogen lines that are very strong in class A, weakening through F and G until they are very weak or absent in class K. Calcium H and K lines are present in late A spectra, but stronger in class F, and strongest in class G ...

  4. Delta Canis Majoris - Wikipedia

    en.wikipedia.org/wiki/Delta_Canis_Majoris

    Artist's illustration of Wezen, a yellow supergiant 1,600 light-years away in the Canis Major constellation. Delta Canis Majoris is a supergiant of class F8. Its surface temperature is around 5,818 K, [12] and it is 14 to 15 times more massive than the Sun. Its absolute magnitude is −6.77, [8] and it lies around 1,600 light-years away. It is ...

  5. Almaany - Wikipedia

    en.wikipedia.org/wiki/Almaany

    It has Arabic to English translations and English to Arabic, as well as a significant quantity of technical terminology. It is useful to translators as its search results are given in context. [ 6 ] Almaany offers correspondent meanings for Arabic terms with semantically similar words and is widely used in Arabic language research. [ 7 ]

  6. Canis Major - Wikipedia

    en.wikipedia.org/wiki/Canis_Major

    It is a yellow-white supergiant of spectral type F8Iab and magnitude 1.84, around 1605 light-years from Earth. [42] With a traditional name meaning "the weight", Wezen is 17 times as massive and 50,000 times as luminous as the Sun.

  7. HD 271182 - Wikipedia

    en.wikipedia.org/wiki/HD_271182

    In 1983, Olin J. Eggen reported that HD 271182 was a pseudo-Cepheid variable, [17] a supergiant in the Hertzsprung gap with less periodic light variations than true Cepheids. [18] This star in particular showed an amplitude of 0.25 mag in the V band. Similarities were noted between it and two other pseudo-Cepheids, namely R Puppis and HD 269879 ...

  8. Savings interest rates today: Ring in the new year with APYs ...

    www.aol.com/finance/savings-interest-rates-today...

    The FDIC is an independent government agency charged with maintaining stability and public confidence in the U.S. financial system and providing insurance on consumer deposit accounts.

  9. Alpha Persei Cluster - Wikipedia

    en.wikipedia.org/wiki/Alpha_Persei_Cluster

    The most luminous member is the ~2nd magnitude yellow supergiant Mirfak, also known as Alpha Persei. Bright members also include Delta, Sigma, Psi, 29, 30, 34, and 48 Persei. The Hipparcos satellite and infrared color-magnitude diagram fitting have been used to establish a distance to the cluster of ~560 light-years (172 pc).