α τ α - translation to
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α τ α - translation to

STAR
Α Volantis; Α Vol

North Star         
  • access-date=8 December 2021}}</ref>
  • Polaris pictured in the flag of [[Nunavut]]
  • integrated flux nebula.]]
  • Polaris components as seen by the [[Hubble Space Telescope]]
BRIGHTEST STAR IN THE CONSTELLATION URSA MINOR
North Star; North star; Alpha Ursae Minoris; Polaris Borealis; Α UMi; Α Ursae Minoris; Stella Polaris; 1 Ursae Minoris; Polarus; HIP 11767; Polaris (star); Α Ursae Minoris,; Hōkūpa‘a; Alruccabah; Ruccabah; Taiyi (Chinese astronomy); Star Polaris; Polaris B; 10.51847; Polaris star; Alpha UMi; Polaris AB; 1 UMi
πολικός αστέρι
alpha particle         
  • alpha spectrum]].
  • Alpha radiation detected in an isopropanol [[cloud chamber]] (after injection of an artificial source radon-220).
  • Energy-loss ([[Bragg curve]]) in air for typical alpha particle emitted through radioactive decay.
  • A physicist observes alpha particles from the decay of a polonium source in a [[cloud chamber]]
  • The trace of a single alpha particle obtained by nuclear physicist Wolfhart Willimczik with his spark chamber specially made for alpha particles.
  • Dispersing of alpha particles on a thin metal sheet
HELIUM-4 NUCLEUS; PARTICLE OF TWO PROTONS AND TWO NEUTRONS
Alpha ray; Alpha-particles; Alpha radication; Alpha Particle; Helium nucleus; Alpha Radiation; Alpha Ray; Alpha emitter; Helium Nucleus; Α particle; Α-particles; Α-particle; A-particles; A-particle; Alpha particles; Alpha-particle; Alpha rays; Anti-alpha particle; Alpha-Particle Emission; Helium nuclei; Α particles; Helium-4 nucleus; He2+
σωματίδιο άλφα
alpha radiation         
  • alpha spectrum]].
  • Alpha radiation detected in an isopropanol [[cloud chamber]] (after injection of an artificial source radon-220).
  • Energy-loss ([[Bragg curve]]) in air for typical alpha particle emitted through radioactive decay.
  • A physicist observes alpha particles from the decay of a polonium source in a [[cloud chamber]]
  • The trace of a single alpha particle obtained by nuclear physicist Wolfhart Willimczik with his spark chamber specially made for alpha particles.
  • Dispersing of alpha particles on a thin metal sheet
HELIUM-4 NUCLEUS; PARTICLE OF TWO PROTONS AND TWO NEUTRONS
Alpha ray; Alpha-particles; Alpha radication; Alpha Particle; Helium nucleus; Alpha Radiation; Alpha Ray; Alpha emitter; Helium Nucleus; Α particle; Α-particles; Α-particle; A-particles; A-particle; Alpha particles; Alpha-particle; Alpha rays; Anti-alpha particle; Alpha-Particle Emission; Helium nuclei; Α particles; Helium-4 nucleus; He2+
ακτινοβολία άλφα

Ορισμός

ALPHA
<language> (Or "Input") An extension of ALGOL 60 for the M-20 computer developed by A.P. Ershov at Novosibirsk in 1961. ALPHA includes matrix operations, slices, and complex arithmetic. ["The Alpha Automatic Programming System", A.P. Ershov ed., A-P 1971]. (1995-05-10)

Βικιπαίδεια

Alpha Volantis

Alpha Volantis (Alpha Vol), Latinized from α Volantis, is a binary star system located in the southern constellation Volans. It has an apparent visual magnitude of +4.00, which is bright enough to be seen with the naked eye. Based upon parallax measurements made with the Hipparcos spacecraft, it is located at a distance of 125 light years from the Sun. As of 2010, the two components of this system had an angular separation of 0.0318″ along a position angle of 286.9°. The magnitude difference between the two components is 0.1. It is considered a member of the Sirius supercluster.

The primary component is an Am star with a stellar classification of kA3hA5mA5 V. This notation indicates the star has the weak calcium II K-line of an A3 star, and the hydrogen and metallic lines of an A5 star. It has an estimated age of 427 million years. In 1992, it was found to be emitting an infrared excess, suggesting the presence of a circumstellar disk of dust. However, subsequent observations have not confirmed this.