Chapters
1. Introduction to Titan[below]
* Introduction
* Titan facts table
* Bibliography/Links
* Foreword: About Living Titan
website
2.
Interpreting Huygens Image Data
* artifacts, blobs, etc, versus
real image data
* What's in the view in Huygens
image scenes?
* Notes on Image Colorizations
3.
Titan Geography
* How the Tides Shape Titan's
Overall Geography
Huygens's landing Site
* Explores how all the
instrument
readings support (or don't contradict) the visually evident landing in
a few cm or inches of very clear liquid methane at a mud or silt bar,
and
how many of the Huygens images show clearly that the sea they view
could
only be liquid.
* Time lapse and still images of
tide pools and other water scenes in color and-or monochrome, regular
and
contrast expanded, showing the similarities between Huygens images and
images of water on Earth.
* Mosaics showing Huygens' point
of landing
* The correlation of features
from
HRI high altitude and SLI low altitude images.
In some ways, Titan is remarkably Earthlike, and in others, very strange to us. Owing to the methane vapor in the atmosphere, which absorbs many light wavelengths visible to human eyes, on Titan we would see sunlight and shadows dimly, and we'd miss the stars at night, and perhaps even beautiful Saturn which Titan orbits. Eyes of Titanian creatures, however, would evolve to see in the wavelengths methane is transparent to, and would be able to see these sights. Titan has both land and sea areas as does the Earth. The land areas have mountains, hills and lakes. The sea areas are sculpted by the stong tides, and have sand and mud bars, tidal flats and shoals, as well as deeper areas where huge waves crawl lazily along, stirred by gentle tidal winds and superrotational breezes in the low gravity. Where Huygens landed, it was raining a drizzely rain of liquid methane, but it is not known yet whether it rains everywhere or just some places, or whether it rains all the time or just once in a while. Occasional rain clouds form and then vanish in the antarctic, where it has been summer for several Earth years as I write.
(It seems obvious from Cassini and Huygens images and other observations that) Titan is covered with verdant vegetation. Forests with plants and trees of sizes exceeding anything ever seen on Earth poke their way upward in the low gravity and calm weather. The forests extend from the tropics into the high arctic and the vegetation changes in character with the latitude. The seas and lakes are filled with aquatic vegatation much in the nature of gigantic swamps. Gigantic vines with sessile leaves crawl for kilometers across the mud bars and over the sea. With the cold temperature, the low gravity, and the long seasons, all of this vegetation probably lives very much in slow motion compared to life on Earth. The individual forest plants may perhaps be but little changed since Columbus ventured to the Americas on Earth.
The only possible signs of animal life so far are dubious at best. However, most of the views were too distant to identify animals unless they were colossal - "Titanic".
Earth has two poles: North and South. Titan has four: North, South, Saturn and Anti-Saturn. Along the equator, tidal flows rush back and forth between the Saturn -- anti-Saturn seas and the mid-longitude seas at right angles to Saturn over the course of each Titanian day, 16 Earth days long. The time of day of the tide changes slowly over the course of the year, 30 Earth years long. Titan's 'water' is liquid methane (CH4): at Titan's 94 degree Kelvin temperatures, Earth's water (H2O ice) is just another kind of rock.
The atmosphere is just a little thicker than the Earth's (Huygens measured 1460 millibars) and composed mainly of the same gas, nitrogen. It is the only other world in the solar system with an air pressure even remotely similar to Earth's. Oxygen, however, is absent, and water vapour is replaced by methane vapour.
Titan's gravity is only about 1/7 of the Earth's. This is even less than our moon's gravity (1/6) even though Titan is over three times the size of our moon, because Titan's core contains many lighter materials such as ice, and so it is less dense. The horizon would seem strangely close to us owing to Titan's smaller size. Although Titan is just 1/15th of Earth's size by volume, it has 1/6 of its surface area.
While there is a lot more of Titan unexplored than explored, it would appear that much of tropical Titan could be likened to a vast swampy wetlands, where the question about the almost flat surface is not always "liquid or land?" but "how soggy?"
Titan Revealed!, at a
methane-transparent
wavelength (939 nm)
Center is 15º south and
156º west; Huygens landed at 10º S, 192º W.
The dark area is the Saturn
antipodal sea -- Saturn is never seen on Titan from this hemisphere,
while
from the other, it always sits at one point in the sky, lighting the
nights.
There appear to be shallows to the East of the islands, possibly silt
in
the lee of tidal flows. The bright "sinewy" region to the East of it
has
been dubbed "Xanadu". Clouds are seen near the South pole, which were
gone
on the next fly-by, probably having rained in the polar region. Some of
the darker features here and there are lakes, and what seem to be
mountains
have been seen in the southern mid latitudes.
A tropical methane
sea
as seen by the descending Huygens lander. What looked like an island
with
rivers from high altitude looks more and more like a flat mudbar, awash
in the sea and covered with huge plants, as Huygens nears its landing
on
another, very small, mudbar. The dark "rivers" are seen as being
shadows
and reflections of the leaves and stems. Aquatic vegetation appears in
and floats on the deeper area in front of the mudbar. The transparency
of the methane and the similar chemistry of air and sea may explain
Titan's
prolific aquatic vegetation, which appears in Cassini images to blanket
almost the whole of the seas, like duckweed, bullrushes, water lillies
and so on on an Earthly pond.
The area behind the
mudbar
is probably a very immense, flat beach, just submerged, with big waves
slowly rolling in over it. However, I've never been entirely certain
these
are waves and not gigantic floating plant stems -- I colored some as
such.
These are also seen by Cassini's radar and labelled "sand dunes", but
they
are not seen in the visual images.
It seems it was raining at the
time of the landing, with drops of methane almost 1/2 inch across
lazily
drizzling down from the gold-orange sky and making the view hazy. In
nearly
all the images, considerable contrast enhancement has been employed to
attempt to discern detail in what was dimly seen through the rain or
drifting
about submerged in the clear sea.
| Size | 5156
Km Diameter; somewhat larger than Mercury; almost half the size of
Mars;
1/15 the size of Earth (by volume). The total surface area is 16% of
Earth's,
or 3/5 of our Land area, or 83 million square Km.
|
| Density | 1.8
- about twice that of water. (Earth, the densest planet, is about 5.5.)
|
| Atmosphere | 1460
mBars or 21 PSI as measured by Huygens at sea level, 4.5 times as dense
as Earth's air. (from Boyle's law of boiling: gas
density=pressure/temperature,
=1.46 bars / (93K/295K). ) Extends over 1000 Km into space. (Cassini
dares
not fly much closer!) ~95% Nitrogen, 5% Methane vapour.
|
| Seas | Liquid Methane (CH4). Strong tidal flows on a once-per-Titan-day cycle. (See The Seas on Titan) |
| Daytime Surface Temperature | 93.65
+/- .25 degrees Kelvin, or -187 degrees Celsius as measured by Huygens
at the surface. This is 1/3 the thermal energy of Earth.
|
| Distance
from Saturn
|
1.2
Gm (Giga-meters), slightly elliptical causing tides; Earth's moon
is .4 Gm from Earth
|
| Length of day | 16 Earth days; Titan orbits gas-giant Saturn once in that time, and keeps the same face always towards Saturn. |
| Distance from Sun | 1400
Gm (Giga-meters); Earth is 150 Gm
|
| Year | 30 Earth Years; Titan is 9.5 times as far from the sun as Earth |
| Inclination of Equator to the Sun (Seasons) | 26-3/4 degrees (same as Saturn's rings); Earth 23-1/2 degrees |
"Bibliography": Links to other sources of Titan information, or copies of those sources:
"Official" sites associated with Cassini & Huygens Missions
* General Link to
Cassini-Huygens
mission at JPL/NASA: http://saturn.jpl.nasa.gov
* General Link to
Cassini-Huygens
at ESA: http://www.esa.int/SPECIALS/Cassini-Huygens
* Cassini Solid State Imaging
(SSI)
Laboratory site: http://www.ciclops.org
Links to Lunar and Planetary
Laboratories
sites
* Huygens Descent Imager &
Radial Spectrometer site: http://www.lpl.arizona.edu/~kholso
* Cassini Visual and Infrared
Mapping
Spectrometer site: http://wwwvims.lpl.arizona.edu
Selected independent Titan exploration sites
* This page has links to many
Titan
images and information: http://anthony.liekens.net/huygens_static.html
* Some other people's considered
thoughts on Titan: http://www.titanexploration.com/
* Here's a site concentrating on
Titan chemistry:
http://www.markelowitz.com/titan.htm
* René Pascal, Some fine
Mosaics made from the Huygens images: http://www.beugungsbild.de/huygens/huygens.html
Selected email and web groups which discuss Titan
* Jupiter List;
"Discuss
the outer solar system". Not necessarily a good place to air new or
unconventional
ideas, but a good source of quasi-official news releases form NASA,
JPL,
etc:
jupiter_list@yahoogroups.com
(around
300 subscribers)
* Cassini Huygens list.
A more open discussion list about the Saturn system and especially the
Cassini-Huygens mission to it. Be prepared to receive lovely (but
sometimes
large file size) pictures of Saturn's moons and rings, etc, as well as
text, and for limited discussion of other space topics: cassinihuygens@yahoogroups.com
(around 200 subscribers)
* Unmanned Spaceflight Web
Discussion
Group.
http://www.unmannedspaceflight.com
My Titan studies started in March (2005) with disbelief of the astonishing idea that Huygens saw no liquid methane, when it is ubiquitous in the images and also was apparently detected by the downward looking spectrometers from 21 meters altitude and by the GCMS instrument when Huygens's landed "with a splat". The Huygens images now appear to have been cast aside with little attention ever having been paid to their fascinating content.
It is tedious to discern the features of a scene and easy to read things that aren't really there into low-resolution monochrome images, degraded by "dewdrops" on the lenses and lossy image compression. However, the Huygens images and data, collected at great expense and effort from on Titan itself, are of adequate quality to reliably show Most Interesting Real scenes. Finer points of detail are often ambiguous for the very reason of what they show: a changing seascape with features in or on very shallow liquid. Many features are seen several times as Huygens descends, providing independent checks of each other to illuminate truth and separate it from illusions of light and shadow. Applicable Cassini images also very much correspond with Huygens images and support the model presented. In fact, no instrument readings or images I've been able to find actually contradict the views herein expressed: even with observations that appear to contradict each other such as the Earth-based 2003 radar versus the 2005 IR checks for reflections from liquid, this scenario appears to explain why they might.
This site to a great extent
consists of Huygens's images with my commentary. There is nothing else
to bring to the table but distant images. Huygens info Must be examined
analytically with an open mind, not a mind that has already concluded
certain
things that "must be" and is therefore unable to comprehend what it is
looking at. Colorizing (with retention of the original brightness
levels)
is my attempt to make immediately clear features that often took me
considerable
time to discern and fathom, not to embellish or - worse - create them.
While I certainly make no claim that every brush stroke and idea
presented
is correct or perfect, I firmly believe I've painted an essentially
true
and comprehensive picture of the astonishing Real Titan.
Note January 21, 2006. With the low resolution monchrome images evidently making visual recognition difficult to many, and looking into Huygens's various Surface Science Package (SSP) and other sensors further, the various data might seem to override the Gas Chromatograph and Mass Spectrometer (GCMS) finding of "...liquid methane on the surface". Without recognition that plant life could extend some sort of dry olive branch to a probe landing in the sea, I can better understand how a general belief that "Titan is dry" formed, though I don't share it. It seems to be a catch-22: one can't believe in aquatic plants without a sea, and one can't believe in the liquid sea without first recognizing that it's choked with gigantic aquatic plants that drastically change its appearance from what would otherwise be expected.
One of my illusions appears to be vanquished: on discovering the actual direction of shadows for the images in question, "giant sea creatures" I thought I saw would appear to be simply light and shadow playing tricks with seaweed. If there are sea animals on Titan, they were too small, too distant, or too strange to be recognized -- at least by me -- in the Huygens images. And that was to be expected for anything smaller than whales, except in the after landing images. Searching for animal life both undersea and above would surely be a worthy science goal for the next Titan explorer, and any balloon should have a "glass bottom boat" for a bottom. With color (methane bands) cameras, of course. We should also temper our hopes by remembering what a monumental achievement landing a craft on Titan was, and that about 1/2 of all Mars landers have failed.
But overall, Titan seems to be even more astonishing than I dreamed when I originally wrote the foreword: What seemed to be land now appears to be mud or silt flats barely level with the sea, there appear to be waves a mile wide seen by Cassini's radar rippling through vast beds of seaweed, and Huygens itself appears to have landed on a small mud or silt bar. Spectrographic data from the surface supports the visual scenes of life by finding complex organic compounds with unknown constituents, different from anywhere else in the solar system, and aerosols that are the end products of a complex organic chemistry.
Perhaps the words of an earlier space explorer, while somewhat dated by developments in robotic space travel and subsequent explorations, are worth quoting here:
"What
would the explorers bring home from Mars? No one can say--just as no
one
can say what explorers eventually may find on the moons of Jupiter, or
on Pluto.
"Such uncertainty
inevitably attends the conquest of new horizons; explorers since the
beginning
of time have been unable to envision the full impact of their
achievements.
"Often, like
Columbus,
they made confident assessments which time proved wrong. It usually
remained
for those who followed to find the real significance of the explorer's
effort, and to reap benefits far greater than were anticipated. There
is
little doubt in my mind that the benefits of space travel will emerge
in
the same way."
Dr. Thomas O. Paine,
Administrator, NASA,
(National Geographic Journal,
December
1969 - Apollo 11 Moon landing coverage issue.)
August 8th, 2005
Rev Aug 16, 2005
Rev Aug 26 (foreword)
Rev Sept 9 2005 (Index: feature
descriptions added)
Rev Nov 12 2005 (Links update)
Rev Jan 21 2006 (update note to
foreword)
Rev July 08 2006 (Link to
"unmanned
spacelflight" web discussion group; updates to chapter highlights;
rotten
HTML cleanup which may have effected some things.)
Rev Jan 23 2007 A few additions
to Introduction to Titan; Colorized Huygens scene.