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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 |