1. Mission to Titan
KELSEY
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Natalia Alvarez • Kelsey Bertamus • Michael Morgan • Talia Strait • Natalie Taylor

2. KELSEY
Our mission will bring us to Saturn, 9.5 astronomical units from the Sun and varying between 7 and 11 astronomical units from earth.
Titan is one of 62 moons that orbit Saturn and the second largest moon in the solar system (point out titan in lower left corner)
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3. Photo source: http://thegreatamericandesert. files. wordpress

4. Bulk Characteristics of Titan
Diameter: 5,150 km
Average Density: g/cm3
Surface Temperature: 97K
Surface Pressure: 1.5 bars
Theorized to have an interior liquid layer composed of ammonia and water ice
KELSEY
*Titan is 5,150 km in diameter, larger than Earth’s moon. Titan is also LARGER than the planet mercury but only 40% as massive because it is made primarily of ice and rock whereas mercury contains an iron core.
Interestingly, the Cassini mission as will be discussed later found that there may be a liquid layer composed of water and ammonia between the ice crust and deeper high-pressure ice layers. Theoretically, the presence of ammonia may allows the water to remain liquid.
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5. Guide to Titan Titan parallels early Earth
Lakes, Atmosphere, Clouds, Rain, Volcanoes, Plate Tectonics.
Only other body in solar system known to harbor stable liquids on its surface.
Weather cycle
Good indications for life or at the very least, pre-earth conditions.
MICHAEL
Titan’s surface
Why are we interested?
Titan is the only body in the solar system other than Earth to have lakes, rivers, clouds, and a cycle of evaporation and mist or rainfall connecting them all. But on Titan, where temperatures hover around minus 300 degrees Fahrenheit, the flowing liquids are hydrocarbons like methane and ethane, not water.
Titan is the only world beyond Earth known to harbor stable liquids on its surface.
The moon has a weather cycle just like our planet does, although Titan’s is based on hydrocarbons rather than water.
These liquids cycle between the atmosphere, surface and subsurface, and the huge moon’s lakes are an integral part of this process.
“some of the things we see happening in our own backyard are right there on Titan to study and learn from” – Cassini team member.
Between volcanism, methane found in all three points, cycles, these are good indications of microbial life – like we talked about earlier.
Our goal through this mission is to study some of these geographic features more intimately.
Our focus being a lake in the south pole.
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6. Atmosphere Only known moon with an atmosphere.
1.45 Denser than Earth’s
1.19 times as massive.
Result of volcanism or microbial life.
Like a young planet Earth.
Research simulated atmospheric conditions and were given the building blocks of life.
MICHAEL
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What is replenishing the atmosphere? Believed to be volcanoes. Could be microbial life.
Also contains: hydrocarbons, ethane, diacetylene, methylacetylene, acetylene and propane, cyanoacetylene, hydogren cyanide, carbon dioxide, carbon monoxide, cyanogen, argon, and helium. Less ethane / methane in the winter season since it precipitates?
In October of 2010 in the American Astronomical Society's Division for Planetary Sciences meeting in Pasadena, California, researchers described how they used radio-frequency radiation—a more convenient substitute for ultraviolet sunlight—to turn methane, nitrogen, and carbon monoxide (the main constituents of Titan's atmosphere) into glycine and alanine, the two smallest amino acids. The experiments also produced cytosine, adenine, thymine, and guanine, the four most basic components of DNA. And they created uracil, a precursor of RNA.
It should be also noted that they accomplished this without using water, and an implication of this is that Earth’s life could have evolved in the atmosphere.
Obviously there are more things about the geological features of saturn’s moon to study so that we may not only search for extraterrestrial microbial life (or evidence), but also for understanding how life may have started on our planet

7. Rain on Titan
Recorded evidence of methane rainstorms on Titan in 2010.
Occurred over equator, rather than at poles.
Replenishes methane lakes and river systems.
Skepticism on whether this is any indication of life.
MICHAEL
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Another quality Titan shares with Earth is its ability to rain.
When photos showed a large patch near the equator of Titan mysteriously darken and then grow lighter within a couple of weeks, scientists knew something big was happening on Saturn's largest moon. But what they found was something they didn't expect: a methane rainstorm in a region of Titan thought to be covered by vast, arid dunes.
While the large moon is known to have methane lakes at its north and south poles, scientists thought Titan's equatorial region was mostly dry, but the likely cause of the darkness was determined to be an outburst of clouds and methane rain — which suggests Titan's equator has a rainy season. [Photos: The Rings and Moons of Saturn]
Rain rarely occurs along poles.
Scientists are skeptic as to what degree the rain cycle would be condusive for life / is not a suggestion for habitability. But again, this could be anthropomophizing expectations of the conditions of life, and this cycling of nutrients could affect methane based life or other forms of life that we have yet to fathom.
cycling of nutrients / triple point could be important for extraterrestrial life forms.
This photo was taken on October 18th, 2010 shows the clouds hovering over Titan’s equator.
Unanswered questions: What are the effects of the rain cycle on the desert?

8. MICHAEL
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Titan has weather patterns! The transition between seasons brings along a change in weather patterns. As you can see, these can be very dramatic in comparison to the earth: the rain follows the change in Summer.
seasonal change of ITCS (intertropical convergence zone) is more dramatic.

9. Methane Lakes
Thanks to Triple Point and rain, Methane Lakes exist on Titan’s surface
Only known terrestrial body other than Earth to have stable liquids on its surface.
Not difficult to land.
An enormous lake on Saturn’s moon.
Updates from this spring have shifted how we view this lake.
We know certain parts behave like a mudflat on our planet.
What is a mudflat? How does this shift our mission?
Liquid methane flows in and out.
Will be doing an incredibly close fly by on May 21st. 955 km away from Titan.
Cassini spacecraft finds evidence for long-standing channels etched into the southern end of the bed.
So it wouldn’t be difficult to land there, especially in the winter.

10. Cryovolcano Winter, S Hemisphere. Sotra Facula is a cryovolcano
Emits water with ammonium, or polyethylene, paraffin waxes, or asphalt. Possibly replenishes methane in atmosphere.
Located at 12degrees S / degrees W
235 km wide
Since, radiation should constantly be depleting the atmosphere, something on Titan’s surface need to be replenishing the source of methane in its atmosphere. As we mentioned earlier, one of those sources could be mathogenic life. Another source, however, could be active volcanoes on its surface.
Other evidence for volcanic activity comes from the great variety in geographic landscape. The mountains rise more than 3,000 feet in the air, and the hole sinks 5,000 feet below. Geophysicist Randolph kirk of the U.S. Geological Survey concludes that these physical qualities indicate volcanic activity (whether dormant or active is question).
Ammonia water lava.

11. Habitability of Titan Titan’s PHI is 0.64 Solid Surface Atmosphere
Evidence of tectonics
Atmosphere
Nitrogen and Hydrocarbons
Believed to be similar to Earth’s atmosphere before oxygen was introduced
Surface Liquid
Titan’s 93K surface temperature is directly above the triple point for methane (90.68K)
KELSEY
So why send a mission to Titan? Titan has a 0.64 on the planetary habitability index. A high ranking.
Some of the factors that Michael just discussed play into this high PHI ranking- the presence of a solid surface and plate tectonics (results from the Cassini mission show regular spacing of ridges on Titan’s surface, evidence of compression or extension of the crust over large areas). Also, the atmosphere of nitrogen and hydrocarbons, and the presence of surface liquid- in Titan’s case, methane and ethane.

12. This image illustrates a new way to rank planet habitability that just came out this year. Rather than basing it on a planet’s similarity to earth, astronomers are expanding this to focus on conditions considered necessary or beneficial for life (which would take into consideration methane-based life forms). As you see in this image, Earth does not have a perfect score with this index because it lacks tidal flexing (though tidal flexing did happen in the past when the Moon was very near the Earth). Titan comes in second place behind Earth in the Solar System, beating Mars by a margin. Titan loses points because it does not contain the elements Sulfur and Phosphorus as far as we can tell, and lacks in redox reactions and tidal flexing.
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13. Triple Point
The temperature and pressure at which the three phases (gas, liquid, and solid) of that substance coexist in equilibrium.
Different changes in temp and pressure transform substance to ice, liquid, vapor.
EARTH’S SURFACE: temps and pressures similar to the triple pt of WATER.
TITAN’S SURFACE: temps and pressures similar to the triple pt of METHANE.
NATALIE
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A little chem review that goes along with our presentation:
The triple point of a substance is the temperature and pressure at which the three phases (gas, liquid, and solid) of that substance coexist in equilibrium.
For ex, the triple point of water on earth occurs at K and 6.04 x10-3 atm
At that point, it is possible to change all of the substance to ice, liquid, vapor by making changes in temperature and pressure.
Water can exist in all three states of matter on Earth.
The temperature and pressure at Titan’s surface are very close to the triple point of methane.
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14. Possibility for Methanogenic Life
2005 – Chris McKay suggested that methane-based (rather than water-based) life on Titan could consume hydrogen, acetylene, and ethane – i.e. organisms called methanogens.
EARTH = O2 metabolism
NATALIE
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In 2005 – Chris McKay suggested that methane-based life on Titan could consume hydrogen, acetylene, and ethane – i.e. organisms called methanogens.
In a way that is analogous to water-based life on Earth
This is an equation of Earth’s O2 metabolic life processes  basically the eqns for photosynthesis and cellular respiration
Life’s metabolic processes on earth function with this eqn.
C6H12O6 (glucose) + O2 -> CO2 + H2O
Photo show is of Earth-based methanogens. We do not know if Titan’s methanogens would look like this.
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C6H12O6 (glucose) + O2 -> CO2 + H2O

15. C2H2 (acetylene) + 3H2 -> 2CH4
Methanogenic Life (continued)
Titan’s organisms would:
Inhale H2 
instead of O2
React it with acetylene (or CO2) 
instead of glucose
Exhale methane 
instead of carbon dioxide
Water is widespread on Earth, therefore life is widespread on Earth because it uses water.
Analogous to Earth = Liquid methane lakes are widespread on the surface of Titan.
NATALIE
Image: this is an image of methanogenic life found on earth.
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Titan’s organisms would:
Inhale H2 instead of O2
React it with acetylene (or CO2) instead of glucose
Exhale methane instead of carbon dioxide.
Liquid methane lakes are widespread on the surface of Titan.
Analogous to Earth: Life is widespread on Earth because it uses water and water is widespread on Earth.
TITAN= H2 metabolism
C2H2 (acetylene) + 3H2 -> 2CH4
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16. The Miller-Urey Experiment
The Experiment (1953):
INORGANIC components  ORGANIC components in conditions similar to pre-biotic Earth.
Warm water + four gases [H2O, CH4, NH3, and H2] + electrical discharges
Formed simple organic molecules, including amino acids and RNA nucleotides.
Formed the idea that on pre-biotic Earth there existed an abundance of RNA life produced through chemical reactions.
In the search for extraterrestrial life? Helps to understand the conditions required for life to form.
Titan’s atmosphere lacks oxygen, but complex organic molecules are present.
 Could form biological materials in a pre-biotic habitat resembling that of early Earth.
NATALIE
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1953 – Urey and Miller produced organic molecules from the inorganic components thought to have been present on pre-biotic Earth.
Warm water combined with four gases:
H2O, CH4, NH3, and H2
Pulsed with electrical discharges.
One week later, they found simple organic molecules, including amino acids and RNA nucleotides, had formed.
There was the idea that on Earth there existed an abundance of RNA life produced through pre-biotic chemical reactions.
Relates to the search for extraterrestrial life to understand the conditions required for life to form.
Titan’s atmosphere lacks oxygen, but complex organic molecules are present there. Could form biological materials in a pre-biotic habitat resembling that of early Earth.
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17. Titan as a Prebiotic Environment?
Possible host for microbial extraterrestrial life because of its pre-biotic-like environment rich in complex organic chemistry.
Possibly subsurface liquid ocean serving as a biotic environment.
Implications of a possible ammonia-water ocean inside Titan.
NATALIE
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Yellow = hazy surface of Titan
Light gray = ice layer starting near the surface
Blue = internal ocean
Light gray = another layer of ice
Dark gray = mixture of rock and ice in the interior

18. Past Mission: Cassini-Huygens
NASA / ESA / ASI Spacecraft to study Saturn and its satellites.
Launched in 1997, reached system in 2004
Cassini: first to enter Saturn’s orbit.
To study structure and history of the rings and satellite surfaces.
Studies Titan’s cloud, hazes, and regional surfaces.
(Talia)
“This world is built by organic activities which still operate and Cassini/Huygens findings suggest a world with a balance of geologic and atmospheruic processes that is the solar system’s best analogue to Earth” (Wikipedia)
Mission related to Titan:
To study the time variability of Titan’s clouds and hazes
Characterize Titan’s surface on a regional scale
Instruments on Cassini: radar to penetrate the haze, signals bounce of Titan’s surface and times return to map surface
-Instrument to receive and measure radio signals—would determine electron density and temperature
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19. Huygens Probe Reached Titan Jan 14th, 2005
Sent data for 90 minutes after touchdown.
Designed to brake in atmosphere and parachute a robotic lab to the surface.
Sent signals to Cassini to relay back to Earth.
(Talia)
*separated from orbiter on Dec 25, 2004 and landed on Jan 14, 2005
-coasted in free space for 22 days with the only active system being the wake-up timer
*remains most distant landing
*landed near Xanadu Region
*Designed to gather data for a few hours in the atmosphere, and a short time at the surface…sent data for about 90 minutes after touchdown
*Design: to enter and brake in atmosphere and parachute a fully instrumented robotic lab to surface
*Was designed to survive impact and splash-down on a liquid surface or solid
*After ~3 2.5 hours, Cassini turned away, but other radio telescopes on Earth continued to listen
*Picture is of approximate landing area
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20. Photo source: http://www. visionsofthecosmos. co

21. Huygens Design Heat shield and parachute.
6 Types of Instrumentation to study:
Physical and electrical props of atmosphere
Radiation balance in Titan’s atmosphere
Chemicals in Titan’s atmosphere
Volatiles and decompose complex organic materials
Physical properties at point of impact.
(Talia)
Designed to be able to handle a liquid or surface landing, as not that sure about surface of Titan at that point in time
Instrumentation:
Atmospheric Structure Instrument: measured physical and electrical props of atmosphere…could get density, wind gusts, wave motion in case of liquid landing
Also contained a microphone
Doppler Wind Experiment—data lost because of failure of ground controllers to turn on receiver in Cassini orbiter
Vertical wind shear
Descent Imager/Spectral Radiometer—study radiation balance in Titan’s atmosphere
Gas Chromatograph Mass Spectrometer—to identify and measure chemicals in Titan’s atmosphere
Aerosol Collector and Pyrolyser—to vaporize volatiles and decompose complex organic materials
Surface-Science Package—to determine physical properties at point of impact
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22. Huygens Findings Landed in “Titanian Mud”
Rounded pebbles imply possible fluid motion.
Dense cloud or thick haze ~ 18 – 20 km from surface.
(Talia)
Landed in “Titanian Mud”
Rounded pebbles imply possible fluid motion.
-early imaging showed large drainage channels crossing mainland into a dark sea
-At landing site, indications of chunks of water ice scattered over an orange surface, majority of which is covered by a thin haze of methane
-Later analysis suggested more of a “sand” made of ice grains
Dense cloud or thick haze ~ 18 – 20 km from surface.
-Thermometers showed such fast heat wicking that ground must have been damp; one image shows light relfected by a dewdrop
-feeble sunlight allows only 1cm of evaporation/year (1 meter on Earth), but atmosphere can hold equivalent of about 10 meters of liquid before rain forms
Huygens landed in “Titanian mud”…indications of chunks of water ice scattered over an orange surface, covered by haze of methane
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23. Two New Proposals: TSSM and TiME
Titan Saturn System Mission
Consists of an orbiter and 2 probes.
More features than Huygens.
Titan Mare Explorer
Land in and travel around a methane lake.
To sample and analyze organics for 3 – 6 months.
New power source: Advanced Stirling Radioisotope Generator.
(Talia)
TSSM: Proposed to launch in 2020, arrive in 2029 with 20-month orbit phase
2 probes: one hot air balloon to measure atmosphere, one lander to splashdown in methane seas
Equipped to study features with instruments for imaging, radar profiling, surface and atmospheric sampling (more complete than C-H mission)
TiME: proposed as its own mission, but could be combined with TSSM as the lander
Expected to travel around the lake by wind, no self-propulsion
Target a northern polar sea, descend by parachute
Principle function is to sample and analyze organics for 3-6 months
Cannot be powered by solar panels due to haze and distance from sun, so would rely on Advanced Stirling Radioisotope Generator (14 year liftetime)
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24. Goals of TSSM & TiME Explore Titan as a system.
Study Titan’s organic inventory and astrobiological potential
Constrain Titan’s origin and evolution models.
Recover information on Enceladus and Saturn’s magnetosphere.
(Talia)
Explore Titan as a system
Composition, geographic distribution; methane cycle info; ages of surface features; season changes
Study Titan’s organic inventory and astrobiological potential
TiME would directly discern methane cycle and help understand relation to hydrologic cycle on Earth
Constrain Titan’s origin and evolution models
Recover information on Enceladus and Saturn’s magnetosphere
“This world is built by organic activities which still operate and Cassini/Huygens findings suggest a world with a balance of geologic and atmosphereic processes that is the solar system’s best analogue to Earth”
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25. Mission: PLOT Landing on Titan Probe for Life and Organics on Titan
Land in Lake Ontario Lacus
Possibly explore nearby cryovolcano
Look for Evidence of Life: CO2, acetylene, amino acids, enzymes, isotopic fingerprints
Use Cassini to relay back data
NATALIA
I would like some information about the volcano and location of the landing

26. Landing on Titan Advanced Stirling Radioisotope Generator
Powerful generator currently being developed by NASA.
≥14 year lifetime
Mass ~ 20 kg
Uses 0.8 kg plutonium-238
January 2015
NATALIA
I would like some information about the volcano and location of the landing
Source: NASA

27. Testing Testing Mass Spectrometer Composite Infrared Spectrometer
Test for hotspots in lake
MOD III
Seismometer
Camera
NATALIA
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Image Source: NASA

28. Mission Target- Ontario Lacus
Located at 72° S & 183°W
Composed of methane, ethane, and propane.
Volume: 7-50 km3
KELSEY
Cassini took a detailed radar-image of Ontario Lacus that showed some remarkable features. The northern shoreline features hills about 1 kilometer in altitude, and flooded river valleys. A smooth, wave-sculpted shoreline in the northeastern part of the lake. Waves driven by winds sweeping in from the west or southwest. The southeast shore features a round-headed bay intruding into the shore.
The middle part of the western shoreline shows the first well-developed river delta observed on Titan.
Average depth thought to be 0.4 – 3.2 m, and a maximum depth of 2.9 – 7.4 m.[5] This gives the lake an estimated volume of 7 to 50 km3, less than one thirtieth the volume of Earth's Lake Ontario.

29. Ontario Lacus
KELSEY
Diagram of lacation of Ontario lacus

30. Tour of Ontario Lacus http://www.youtube.com/watch?v=kK4n5l7bHSw
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31. 2017: Launch 2024: Land Timeline Timeline
The goal is to land and test during winter in the Southern Hemisphere.
Talia
We want winter because lake is full and life more likely to thrive in wet conditions
3 year transition to winter in S Hemisphere started in Winter in S. Hemisphere until 2025.
Or 2045 in middle of next winter.

32. Talia
2017
2024

33. Cost of Mission Cost of Mission Proposed Cost: 1 billion
Includes cost of designing and launching a new probe.
Use of the orbiter from the Cassini mission will cut costs
Cassini-Huygens mission (launched 1997) cost NASA 3.2 billion!
NATALIA

34. … is expensive but IMPORTANT!
The Search for Life
Bibliography
… is expensive but IMPORTANT!
It’s important because Titan is in many ways a young Earth. This could provide insight into the origins of life, or at the veryleast, provide a grounds for researching an early earth.