τέτ α τέτ - definizione. Che cos'è τέτ α τέτ
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In questa pagina puoi ottenere un'analisi dettagliata di una parola o frase, prodotta utilizzando la migliore tecnologia di intelligenza artificiale fino ad oggi:

  • come viene usata la parola
  • frequenza di utilizzo
  • è usato più spesso nel discorso orale o scritto
  • opzioni di traduzione delle parole
  • esempi di utilizzo (varie frasi con traduzione)
  • etimologia

Cosa (chi) è τέτ α τέτ - definizione

STAR
Α Volantis; Α Vol

Alpha         
FIRST LETTER OF THE GREEK ALPHABET
Α; ALPHA; Α (letter); Alpha (letter); \alpha; Άλφα; Alpha (Greek); Αα; Alpha (Greek letter); A (Greek)
Alpha (uppercase , lowercase ; , álpha, or ) is the first letter of the Greek alphabet. In the system of Greek numerals, it has a value of one.
ALPHA         
FIRST LETTER OF THE GREEK ALPHABET
Α; ALPHA; Α (letter); Alpha (letter); \alpha; Άλφα; Alpha (Greek); Αα; Alpha (Greek letter); A (Greek)
<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)
Alpha         
FIRST LETTER OF THE GREEK ALPHABET
Α; ALPHA; Α (letter); Alpha (letter); \alpha; Άλφα; Alpha (Greek); Αα; Alpha (Greek letter); A (Greek)
·noun The first letter in the Greek alphabet, answering to A, and hence used to denote the beginning.

Wikipedia

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.