Sorry! This page is not yet available in your preferred language, so we're displaying the original version instead.
NACO images of Titan's surface
An image of Titan by NACO, obtained in a waveband at 1.3 μm that does not perfectly match an atmospheric window is compared to a SDI-NACO image of the same region. The greater clarity and contrast of the latter is evident; it is due to the smaller degree of "atmospheric contamination".
Kredit:ESO
O snímku
| Id: | eso0412e |
| Typ: | Pozorování |
| Datum zveřejnění: | 14. dubna 2004 |
| Související články: | eso0412 |
| Velikost: | 1600 x 816 px |
O objektu
| Jméno: | Titan |
| Typ: | Solar System : Planet : Satellite |
| Kategorie: | Solar System |
Barvy & filtry
| Pásmo | Vlnová délka | Dalekohled |
|---|---|---|
| Infračervený Near-IR | 1.3 μm | Very Large Telescope NACO |