Jupiter and Io
This is a thermal-infrared image of Jupiter, obtained by the ISAAC multi-mode instrument at the 8.2-m VLT ANTU telescope on Paranal on November 14, 2000; the Universal Time (UT) of exposure is indicated. It is part of a series of images showing the dramatically different appearance of Jupiter''s disk and the aurorae when viewed through different thermal-IR imaging filters. Note also the motion of the moon Io (left). The contrast has been enhanced to better show the faint details in the aurorae.
Technical information: This image is based on on-target exposures lasting a total of 30 sec (L-band), 44 sec (4.07 µm), 58 sec (3.28 µm) and 58 sec (3.21 µm), respectively. The real observing time is twice as much, with half of the time spent in the off-target chop position. The fields shown measure 72 x 72 arcsec 2 ; 1 pixel = 0.07 arcsec. North is up and East is left.
ESO
Om billedet
Id: | eso0123b |
Type: | Observation |
Udgivelsesdato: | 7. juni 2001 |
Relaterede pressemeddelelser: | eso0123 |
Størrelse: | 778 x 775 px |
Om objektet
Navn: | Io, Jupiter |
Type: | Solar System : Planet : Satellite Solar System : Planet : Type : Gas Giant |
Kategori: | Solar System |
Baggrundsbilleder
Farver & filtre
Bånd | Bølgelængde | Teleskop |
---|---|---|
Infrarød Near-IR | 3.28 μm | Very Large Telescope ISAAC |
Infrarød Near-IR | 4.07 μm | Very Large Telescope ISAAC |
Infrarød L | Very Large Telescope ISAAC |