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By analyzing methane in the skies of Jupiter and Saturn's moon Titan, scientists are now pinpointing what effects this global warming gas is having on Earth, a new study finds.
Methane, on the other hand, although found in abundance on Jupiter, Saturn, Uranus, and Neptune, was tricky to spot on exoplanets located so far away, at least by means of space-based spectroscopy.
NASA’s Juno spacecraft has once again delivered a stunning view of Jupiter’s ever-changing atmosphere. In this latest image, a trail of drifting clouds ...
Jupiter's atmosphere is mostly composed of hydrogen and helium, with small amounts of ammonia, methane, water vapor and other gases. These latter components condense at different levels to form ...
This giant planet orbits its star so closely that it completes a full orbit in just 30.5 hours. Its dayside reaches a scorching 3000°C, while the eternal nightside cools down to 1500°C. You would ...
For the first time ever, the James Webb telescope has detected methane in an exoplanet's atmosphere. Wed, 19 Feb 2025 13:36:55 GMT (1739972215991) Story Infinite Scroll ...
Now, James Webb has detected methane in an exoplanet’s atmosphere for the first time. The exoplanet in question is WASP-80 b, which is what astronomers call a “warm Jupiter.” ...
Cassini’s cameras come equipped with filters that sample three wavelengths where methane gas absorbs light. These are in the red at 619 nanometer (nm) wavelength and in the near-infrared at 727 ...
Scientists still don’t know what gives it its characteristic hue; its atmosphere is primarily hydrogen, helium and methane. How common is this event Jupiter reaches opposition every 13 months or so.
Jupiter's four best-known moons are the Galilean moons, discovered by Galileo Galilei in 1610. ... rivers and lakes — but made of hydrocarbons like methane instead of water," Cook said.
Scientists have discovered that the icy shell of Saturn's largest moon, Titan, could possess an insulated, six-mile-thick (9.7-kilometer-thick) layer of methane ice beneath its surface.
Hill used the absorption bands of methane (619 nm) and ammonia (647 nm), both well-known features in Jupiter's visible spectrum, to calculate the abundance of these gases above Jupiter’s cloud tops.