1. Large moons of the solar system: Titan
This next slide compares the terrestrial planets with the Earth’s Moon, the four Galilean moons of Jupiter, and Titan, the largest moon of Saturn.
Titan is the only moon in the solar system which has an atmosphere.
The atmosphere is mostly nitrogen and thicker than even Earth’s atmosphere.

3. Titan, as seen before the visit of the Cassini spacecraft

4. Titan, as seen by the Cassini spacecraft false color on the left, infrared on the right

5. Titan’s atmosphere has a high altitude haze, seen by the Cassini spacecraft on the left is a purplish haze, on the right is a view near the terminator between day and night (Sun to the right)

6. Another view of the haze above Titan’s atmosphere, as seen by the Cassini spacecraft from a different angle than the previous slide.

7. Titan’s surface features are difficult to see in visible light from the Cassini spacecraft.

8. Infrared pictures of Titan are not much clearer, but emphasize different details.

9. A Titan crater, as seen by the Cassini spacecraft with visible light on the left, infrared on the right, and radar images in the middle. A radar shows the details of the topographic (altitude-related) features.

10. The surface of Titan was imaged by the probe “Huygens” This is taken from about 8 km altitude as it was descending.

11. Rivers are seen on the surface of Titan as the probe “Huygens” descended to the surface. It landed and took pictures (right).

12. Rivers and channels on the surface of Titan as seen by the probe “Huygens” as it descended to the surface.

13. Photo of the surface of Titan as seen by the probe “Huygens”, compared with images from another Moon !

14. A possible lake of methane on Titan, and some
moving clouds, were seen by the Cassini spacecraft.
This is near the south pole on Titan.

16. A possible volcano (a cryovolcano) on Titan,
seen by the Cassini spacecraft. This may be
a major source of methane for Titan’s atmosphere.

17. Titan “sand” dunes (top), seen by the Cassini spacecraft,
compared with dunes in Namibia, Africa (on bottom).

18. Radar sweeps of the
North pole of Titan,
taken by the
Cassini spacecraft,
showing lakes of
methane and ethane.
Flat areas in radar
images are probably
liquid surfaces, and
are colored blue to
resemble features
on Earth. The radar
image has no color
in reality. (late 2007)

19. A lake (or sea) near the North pole of Titan, taken by
Cassini, compared to Lake Superior on Earth.

21. This sweep of the South pole of Titan was
taken by Cassini, and some small lakes are seen.

23. The task of mapping Titan continues with
each pass of the Cassini spacecraft by Titan.

24. Titan’s Atmosphere is mostly nitrogen, with simple organic compounds like methane and ethane.

25. The haze high in
the atmosphere
of Titan is due to
complex chemistry
combining organics
and nitrogen to form
aerosols. We have
little knowledge of
this low-temperature
photochemistry.

26. The structure of
Titan is possibly
A rocky core
A layer of ice
A layer of water
Surface lakes
A complex atmosphere

27. A selection of online videos about Titan
A new version of imagery during the Huygens descent:
4:41
Another video shows a zoom to the landing site: Approaching Titan a Billion Times Closer
3:23
Soaring Over Titan: Extraterrestrial Land of Lakes 1:27
The Canyon Country (fly-thru of some karst topography) 1:17
Cassini: Four Years of Discovery (Aug 2008 tribute video) 2:18
Cassini: 15 Years of Exploration (Nov tribute video) 2:29
Titan Touchdown (overview of Huygens landing with big titles) 2:27

28. Triton, the
large moon of Neptune,
may be a
captured
Kuiper-belt
Object (KBO).