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Details of the meteor spectrum (FORS1/VLT)
Details of a VLT meteor spectrum (solid line): the intensity (in arbitrary units) is shown as a function of the wavelength. The dashed line is a theoretical model of the spectrum of air heated to a temperature of 4600 degrees at an altitude of 95 km.
Kredit:ESO
O snímku
Id: | eso0424c |
Typ: | Mapa |
Datum zveřejnění: | 30. července 2004 |
Související články: | eso0424 |
Velikost: | 3414 x 963 px |
O objektu
Jméno: | Meteor |
Typ: | Solar System : Interplanetary Body |
Kategorie: | Solar System |
Barvy & filtry
Pásmo | Vlnová délka | Dalekohled |
---|---|---|
Infračervený I | 850 nm | Very Large Telescope FORS1 |
Optický R | 750 nm | Very Large Telescope FORS1 |
Optický R | 650 nm | Very Large Telescope FORS1 |