Why has Cassini detected no waves on the lakes of Titan?
Why has Cassini detected no waves on the lakes of Titan?
Why has Cassini detected no waves on the lakes of Titan?
Tag: Saturn
Why has Cassini detected no waves on the lakes of Titan?
Cassini has found hints of activity coming from the Saturn moon Dione.
Cassini has found hints of activity coming from the Saturn moon Dione.
The spacecraft’s magnetometer has detected a faint particle stream coming from the moon, and images showed evidence for a possible liquid or slushy layer under its rock-hard ice crust. Other Cassini images have also revealed ancient, inactive fractures at Dione similar to those seen at Enceladus that currently spray water ice and organic particles.
Cassini has found hints of activity coming from the Saturn moon Dione.
The spacecraft’s magnetometer has detected a faint particle stream coming from the moon, and images showed evidence for a possible liquid or slushy layer under its rock-hard ice crust. Other Cassini images have also revealed ancient, inactive fractures at Dione similar to those seen at Enceladus that currently spray water ice and organic particles.
Scientists have released the first topo map of Titan.
Scientists have released the first topo map of Titan.
Whereas Earth’s tallest mountain towers nearly 9 kilometers above sea level, Titan’s topographic variations are mild: Its highest point is just half a kilometer above the mean and its lowest just 1.7 kilometers below.
Overall the detail here is not very great. None of the instruments on Cassini can see anything smaller than a half kilometer, about 1,500 feet, so the data doesn’t really show us the rough details. Moreover, the best data is spotty, as it has been accumulated by about a hundred Cassini fly-bys, rather than systematically by an orbiting spacecraft.
Scientists have released the first topo map of Titan.
Whereas Earth’s tallest mountain towers nearly 9 kilometers above sea level, Titan’s topographic variations are mild: Its highest point is just half a kilometer above the mean and its lowest just 1.7 kilometers below.
Overall the detail here is not very great. None of the instruments on Cassini can see anything smaller than a half kilometer, about 1,500 feet, so the data doesn’t really show us the rough details. Moreover, the best data is spotty, as it has been accumulated by about a hundred Cassini fly-bys, rather than systematically by an orbiting spacecraft.
Cassini snaps an amazing image of Saturn’s north pole vortex.
Cassini snaps an amazing image of Saturn’s north pole vortex.
Cassini snaps an amazing image of Saturn’s north pole vortex.
Cassini has imaged meteorites as they crash into Saturn’s rings.
Cassini has imaged meteorites as they crash into Saturn’s rings.
Cassini has imaged meteorites as they crash into Saturn’s rings.
The seasons change on Titan as winter clouds begin for form over its south pole.
The seasons change on Titan as winter clouds begin to form over its south pole.
The seasons change on Titan as winter clouds begin to form over its south pole.
The science team for Cassini has released a spectacular mosiac of Saturn and its rings, backlit by the Sun.
The science team for Cassini has released a spectacular mosiac of Saturn and its rings, backlit by the Sun.
The science team for Cassini has released a spectacular mosiac of Saturn and its rings, backlit by the Sun.
New data suggests that the icy crust of Titan is twice as thick as previously estimated.
New data suggests that the icy crust of Titan is twice as thick as previously estimated.
“The picture of Titan that we get has an icy, rocky core with a radius of a little over 2,000 kilometers, an ocean somewhere in the range of 225 to 300 kilometers thick and an ice layer that is 200 kilometers thick,” [said Howard Zebker of Stanford University]. Previous models of Titan’s structure estimated the icy crust to be approximately 100 kilometers thick.
This means that the methane lakes and rivers of Titan are flowing across a bedrock of ice, which at the cold temperatures there would be as solid as rock is here on Earth.
New data suggests that the icy crust of Titan is twice as thick as previously estimated.
“The picture of Titan that we get has an icy, rocky core with a radius of a little over 2,000 kilometers, an ocean somewhere in the range of 225 to 300 kilometers thick and an ice layer that is 200 kilometers thick,” [said Howard Zebker of Stanford University]. Previous models of Titan’s structure estimated the icy crust to be approximately 100 kilometers thick.
This means that the methane lakes and rivers of Titan are flowing across a bedrock of ice, which at the cold temperatures there would be as solid as rock is here on Earth.
Cassini has taken some spectacular new images of the gigantic hexagonal vortex on Saturn’s north pole.
Cassini has taken some spectacular new images of the gigantic hexagon-shaped vortex on Saturn’s north pole.
Cassini has taken some spectacular new images of the gigantic hexagon-shaped vortex on Saturn’s north pole.
Pac Man in orbit around Saturn.
The after effects of the giant storm on Saturn.
The after effects of the giant storm on Saturn.
The after effects of the giant storm on Saturn.
Bouncing on Titan
How Huygens bounced on Titan. With animation.
How Huygens bounced on Titan. With animation.
The landslides of Iapetus: longer and more frequent than anywhere else in the solar system.
The landslides of Iapetus: longer and more frequent than anywhere else in the solar system.
The landslides of Iapetus: longer and more frequent than anywhere else in the solar system.
Cassini has photographed daytime lightning on Saturn.
Cassini has photographed daytime lightning on Saturn.
Cassini has photographed daytime lightning on Saturn.
Cassini has now seen the beginnings of a vortex over Titan’s south pole, the first sign that winter is coming to the planet’s southern hemisphere.
Turn, turn, turn: Cassini has now seen the beginnings of a vortex over Titan’s south pole, the first sign that winter is coming to the planet’s southern hemisphere.
Turn, turn, turn: Cassini has now seen the beginnings of a vortex over Titan’s south pole, the first sign that winter is coming to the planet’s southern hemisphere.
Cassini has shifted its orbit so that it can look down on Saturn and its rings.
Saturn from above: Cassini has shifted its orbit so that it can look down on Saturn and its rings.
Saturn from above: Cassini has shifted its orbit so that it can look down on Saturn and its rings.
Data of the tidal fluxes on Titan by the Cassini spacecraft now suggest that there is a liquid ocean below Titan’s icy crust.
Data of the tidal fluxes on Titan by the Cassini spacecraft now suggest that there is a liquid ocean below Titan’s icy crust.
The team’s analyses suggest that the surface of the moon can rise and fall by up to 10 metres during each orbit, says Iess. That degree of warpage suggests that Titan’s interior is relatively deformable, the team reports today in Science1. Several models of the moon’s internal structure suggest such flexibility — including a model in which the moon is solid but soft and squishy throughout. But the researchers contend that the most likely model of Titan is one in which an icy shell dozens of kilometres thick floats atop a global ocean. The team’s findings, together with the results of previous studies, hint that Titan’s ocean may lie no more than 100 km below the moon’s surface.
Data of the tidal fluxes on Titan by the Cassini spacecraft now suggest that there is a liquid ocean below Titan’s icy crust.
The team’s analyses suggest that the surface of the moon can rise and fall by up to 10 metres during each orbit, says Iess. That degree of warpage suggests that Titan’s interior is relatively deformable, the team reports today in Science1. Several models of the moon’s internal structure suggest such flexibility — including a model in which the moon is solid but soft and squishy throughout. But the researchers contend that the most likely model of Titan is one in which an icy shell dozens of kilometres thick floats atop a global ocean. The team’s findings, together with the results of previous studies, hint that Titan’s ocean may lie no more than 100 km below the moon’s surface.
More lakes on Titan
Watching the transit of Venus – from Saturn
Watching the transit of Venus – from Saturn.
Watching the transit of Venus – from Saturn.
Scientists studying Cassini images have spotted the trails of objects as they punch through one of Saturn’s rings.
Scientists studying Cassini images have spotted the trails of objects as they punch through one of Saturn’s rings.
Scientists studying Cassini images have spotted the trails of objects as they punch through one of Saturn’s rings.
Is it snowing microbes on Enceladus?
Is it snowing microbes on Enceladus?
“More than 90 jets of all sizes near Enceladus’s south pole are spraying water vapor, icy particles, and organic compounds all over the place,” says Carolyn Porco, an award-winning planetary scientist and leader of the Imaging Science team for NASA’s Cassini spacecraft. “Cassini has flown several times now through this spray and has tasted it. And we have found that aside from water and organic material, there is salt in the icy particles. The salinity is the same as that of Earth’s oceans.”
Is it snowing microbes on Enceladus?
“More than 90 jets of all sizes near Enceladus’s south pole are spraying water vapor, icy particles, and organic compounds all over the place,” says Carolyn Porco, an award-winning planetary scientist and leader of the Imaging Science team for NASA’s Cassini spacecraft. “Cassini has flown several times now through this spray and has tasted it. And we have found that aside from water and organic material, there is salt in the icy particles. The salinity is the same as that of Earth’s oceans.”
Enceladus’s gushing geysers, as seen by Cassini.
Enceladus’s gushing geysers, as seen by Cassini.
Enceladus’s gushing geysers, as seen by Cassini.
The many moods of Titan
The dunes of Titan
Engineers have gone to a back up radio system on Cassini after a primary unit did not respond as expected in late December.
Engineers have gone to a back up radio system on Cassini after a primary unit did not respond as expected in late December.
The cause is still under investigation, but age may be a factor. The spacecraft launched in 1997 and has orbited Saturn since 2004. Cassini completed its prime mission in 2008 and has had two additional mission extensions. This is the first time its ultra-stable oscillator has had an issue.
Engineers have gone to a back up radio system on Cassini after a primary unit did not respond as expected in late December.
The cause is still under investigation, but age may be a factor. The spacecraft launched in 1997 and has orbited Saturn since 2004. Cassini completed its prime mission in 2008 and has had two additional mission extensions. This is the first time its ultra-stable oscillator has had an issue.