WebAlfirk star system properties Alfirk is a visual double star which can be observed with the help of small or medium telescopes. The table below shows key information about the Alfirk double sysyem: Main star magnitude 3.23 Secondary star magnitude 7.83 Magnitude difference 4.6 Separation 13.4 arcsec Alternative designations of Alfirk WebStars. Stars are the most widely recognized astronomical objects, and represent the most fundamental building blocks of galaxies. The age, distribution, and composition of the stars in a galaxy trace the history, dynamics, and evolution of that galaxy. Moreover, stars are responsible for the manufacture and distribution of heavy elements such ...
Alfirk - Deep Sky Workflows: Astrophotography, Space, and …
WebAlfirk, roughly translated ‘the flock,’ is the name of a triple star system that is classified as β Cephei (Beta Cephei). It is a part of the outline of the Cepheus constellation. The main … WebIn December 2024, the names of 112 stars with confirmed exoplanets were announced at a press conference in Paris. The names come from 112 countries and are rooted in their cultures and histories. They were proposed during the IAU100 NameExoWorlds campaigns, launched as part of the International Astronomical Union’s 100th anniversary … south lake tahoe snowshoe trails
Neutron Stars and White Dwarfs Center for Astrophysics
Web4 de feb. de 2024 · The star has a surface gravity of around 3.83 cgs, and it is also a fast spinner. Merak spins with an estimated rotational velocity of around 46 km / 28.5 mi per second. Merak’s radial velocity has been estimated to be at around -12.0 km / -7.4 mi per second. Merak is part of the loose open cluster named Ursa Major moving group. Eta Cephei is a subgiant star with a stellar classification of K0 IV, which indicates it is exhausting the supply of hydrogen at its core and is in the process of evolving into a giant star. With 1.6 times the Sun's mass, at an age of 2.5 billion years it has reached a radius four times larger than the Sun and a luminosity ten times greater. It is radiating this energy from its outer atmosphere at an effective temperature of 4,950 K, giving it the orange-hued glow of a K-type star. Eta Cephei has … WebThe initial mass of Mu Cephei has been estimated from its position relative to theoretical stellar evolutionary tracks to be between 15 M☉ and 25 M☉. [13] [14] The star currently has a mass loss rate of (4.9 ± 1.0) × 10−7 M☉ per year. [13] Supernova [ … south lake tahoe snow storm