Inizio Registrati Login

Elenco album Ultimi arrivi Ultimi commenti Più viste Più votate Preferiti Cerca

Inizio > SOLAR SYSTEM > Asteroids and Comets
Ritorna alla pagina delle miniature FILE 239/282 Torna all'inizio Guarda foto precedente Guarda foto successiva Salta alla fine
Comet McNaught (10)
Caption NASA:"By January 19/20, 2007, Comet McNaught's magnificent dust tail stretched for about 150 MKM (~1 AU), requiring images from both Southern and Northern Hemispheres of planet Earth to take it all in. Two such views - from Cerro Paranal in Chile (left) and the Carnic Alps in Italy - are combined in this unique graphic that also outlines a perspective view of the Comet's orbit (dotted line) and relative position of the Sun. Driven by solar radiation pressure the dust tail initially points away from the Sun, but also trails outside the comet's orbit. Astronomers try to account for the complex structure along the tail, including the pronounced striations, by considering forces acting on the dust (e.g. gravity, solar wind and radiation) as well as the release time and size of the dust grains. In the diagram, the modeled location of dust grains released at approximately the same time relative to perihelion passage, synchrones, are shown as dashed lines. The location of grains of similar size, syndynes, are shown as solid lines".
Parole chiave: Comet McNaught

Comet McNaught (10)

Caption NASA:"By January 19/20, 2007, Comet McNaught's magnificent dust tail stretched for about 150 MKM (~1 AU), requiring images from both Southern and Northern Hemispheres of planet Earth to take it all in. Two such views - from Cerro Paranal in Chile (left) and the Carnic Alps in Italy - are combined in this unique graphic that also outlines a perspective view of the Comet's orbit (dotted line) and relative position of the Sun. Driven by solar radiation pressure the dust tail initially points away from the Sun, but also trails outside the comet's orbit. Astronomers try to account for the complex structure along the tail, including the pronounced striations, by considering forces acting on the dust (e.g. gravity, solar wind and radiation) as well as the release time and size of the dust grains. In the diagram, the modeled location of dust grains released at approximately the same time relative to perihelion passage, synchrones, are shown as dashed lines. The location of grains of similar size, syndynes, are shown as solid lines".

McNaught-09.jpg McNaught-13.jpg McNaught-9.jpg Meteor-Wiggle.jpg Orcus-GIF.gif
Informazioni sul file
Nome del file:McNaught-9.jpg
Nome album:Asteroids and Comets
Valutazione (5 voti):55555(Mostra dettagli)
Parole chiave:Comet / McNaught
Copyright:S. Deiries (ESO), M. Fulle (INAF)
Dimensione del file:127 KiB
Data di inserimento:Feb 01, 2007
Dimensioni:1024 x 717 pixels
Visualizzato:55 volte
URL:https://www.lunexit.it/gallery/displayimage.php?pid=15754
Preferiti:Aggiungi ai preferiti
 
 

Powered by Coppermine Photo Gallery