Mann$46741$ - definizione. Che cos'è Mann$46741$
Diclib.com
Dizionario ChatGPT
Inserisci una parola o una frase in qualsiasi lingua 👆
Lingua:

Traduzione e analisi delle parole tramite l'intelligenza artificiale ChatGPT

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 Mann$46741$ - definizione

STAR IN THE CONSTELLATION CARINA
HD83095; HIP 46741

Mann (surname)         
FAMILY NAME
Mann (scientist); Representative Mann
Mann () may refer to a South Asian surname of Punjabi Jatt origin or a European surname of Germanic origin.
Austin Mann         
AMERICAN POLITICIAN
Draft:Austin Mann; Austin Shuey Mann; Austin S. Mann
Austin Shuey Mann (January 14, 1847 – September 19, 1912) was a lawyer, orange grove owner, and politician who served in the Florida Senate and Florida House of Representatives. He represented Hernando County.
James Mann (curator)         
BRITISH CURATOR (1897-1962)
James Gow Mann; J G Mann; J. G. Mann
Sir James Gow Mann (23 September 1897 – 5 December 1962) was an eminent figure in the art world in the mid twentieth century, specialising in the study of armour.Amongst others he wrote "The Armoury of the Castle of Churburg", 1929; "Spanish Armour of the Xth–XVth Centuries", and "The Etched Decoration of Armour", British Library web site accessed 15:27 GMT Wednesday 15 February 2012

Wikipedia

HD 83095

HD 83095 is a single star in the southern constellation of Carina. It has the Bayer designation H Carinae; HD 83095 is the identifier from the Henry Draper Catalogue. This object has an orange hue and is dimly visible to the naked eye with an apparent visual magnitude of 5.46. The star is located at a distance of approximately 710 light years from the Sun based on parallax, and is drifting further away with a radial velocity of +14 km/s. It has an absolute magnitude of −1.45.

This is an aging K-type giant star with a stellar classification of K4III, having exhausted the supply of hydrogen at its core then cooled and expanded off the main sequence. At present it has about 60 times the radius of the Sun and is radiating 769 times the Sun's luminosity from its swollen photosphere at an effective temperature of 3,940 K.