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How big is Jupiter's moon Io? The most volcanic body in the Solar System, Io (usually pronounced "EYE-oh") is 3,600 kilometers in diameter, about the size of planet Earth's single large natural satellite. Gliding past Jupiter at the turn of the millennium, the Cassini spacecraft captured this awe inspiring view of active Io with the largest gas giant as a backdrop, offering a stunning demonstration of the ruling planet's relative size. Although in the above picture Io appears to be located just in front of the swirling Jovian clouds, Io hurtles around its orbit once every 42 hours at a distance of 420,000 kilometers or so from the center of Jupiter. That puts Io nearly 350,000 kilometers above Jupiter's cloud tops, roughly equivalent to the distance between Earth and Moon. The Cassini spacecraft itself was about 10 million kilometers from Jupiter when recording the image data.
This picture makes me wonder why so many of the "new" space photos appear to be computer graphics.
Your talking about the basic principle of a flatbed scanner CCD(the scanners most of us use). Those satellites don't take scans. And using a singlepass or 3pass that wouldn't alter the real image.
I always laugh when I see such detailed Hi res pictures of planets and moons in our sloar system.
Because we still can't get Nasa to give us a high resolution close up shot of the lunar surface and the landing site of Apollo. All we get is a pic of a real tiny tiny thing in the distance of what they say is the lunar module.
Originally posted by elevenaugust
This Cassini photo gives an idea on how big Jupiter is: Io is slightly bigger than our Moon: 420 000 km for Io and 384 399 km semi-major axis for the moon.
Originally posted by jra
Some corrections need to be made here. Firstly, it was Galileo that went to Jupiter. Cassini is at Saturn. Unless this is an image from Cassini when it did a flyby past Jupiter on its way to Saturn.
Gliding past Jupiter at the turn of the millennium, the Cassini spacecraft captured this awe inspiring view of active Io with the largest gas giant as a backdrop, offering a stunning demonstration of the ruling planet's relative size
How big is Jupiter's moon Io? The most volcanic body in the Solar System, Io (usually pronounced "EYE-oh") is 3,600 kilometers in diameter, about the size of planet Earth's single large natural satellite. Gliding past Jupiter at the turn of the millennium, the Cassini spacecraft captured this awe inspiring view of active Io with the largest gas giant as a backdrop, offering a stunning demonstration of the ruling planet's relative size. Although in the above picture Io appears to be located just in front of the swirling Jovian clouds, Io hurtles around its orbit once every 42 hours at a distance of 420,000 kilometers or so from the center of Jupiter. That puts Io nearly 350,000 kilometers above Jupiter's cloud tops, roughly equivalent to the distance between Earth and Moon. The Cassini spacecraft itself was about 10 million kilometers from Jupiter when recording the image data.
Wide Angle Camera [WAC](20 cm f/3.5 refractor; 380-1100 nm; 18 filters; 3.5ox3.5o) Narrow Angle Camera [NAC](2 m f/10.5 reflector; 200-1100 nm; 24 filters; 0.35ox0.35o)
At the heart of each camera is a charged coupled device (CCD) detector consisting of a 1024 square array of pixels, each 12 microns on a side. The data system allows many options for data collection, including choices for on-chip summing and data compression. The narrow-angle camera packs plenty of power too, and could see a quarter -- 2.4 centimeters (0.9 inches) across -- from a distance of nearly 4 kilometers (2.5 miles).
To increase the images' scientific value, each camera on Cassini has two filter wheels designed to take images at specific wavelengths of light. The narrow-angle camera has 12 filters in each wheel for a total of 24 filters; the wide-angle has 9 in each wheel for a total of 18. Some filters only allow light of a certain color to reach the sensor. Combining three such images can produce a color image. The most scientifically interesting images are calibrated in order to turn the electrical signals that emerge from the CCDs into an absolute measure of brightness.