w e a re n ot a lone b ecause of e nceladus red co-investigators on team jeewon jeon dongwook kim...
TRANSCRIPT
We Are Not Alone Because of Enceladus
RED
Co-investigators on teamJeeWon Jeon
DongWook KimSungbeum Bae
MinJae Kim
Team
Mission Principle Investigator (Spokesperson)KunWook Lee
Contents
I. Information About Enceladus
II. Preparing
III. Launching and Investigation
IV. Other investigations
I. Information about
Enceladus
About Enceladus
Cycle of revolution 1.37 days
Diameter 500km
Surface Covered with ice
Temperature -210℃
Acceleration of gravity 0.114m/s2
Composition of Atmostphere H2O(91%), N(4%), CO2(3.2%), CH4 (1.7%)
Mass 1.082 X 1020
Mission Objective
Mission Statement: 1. Searching for life in Enceladus 2. Investigating the environment of Enceladus
Science Goals 1. Clarifying whether Enceladus has lives or not. 2. Investigating the structure of Enceladus.
Why is Enceladus important?
- Organic chemicals (Cassini found it)
- Magnetic field (from Saturn, protect solar wind)
- Energy
- Water
Previous research
Voyagers- Measured its diameter about
500km long- Enceladus was located in the
densest part of Saturn's diffuse E-ring
Cassini- Found water geysers in the south
pole- Investigated the composition of
water (found organic chemicals.)
II. Preparing
1. Conditions of water (composition, temperature, etc)
2. Isotope of carbon, hydrogen, oxygen, nitrogen, sulfur
3. Periodical changes of composition
4. Physical conditions inside of the Ocean
5. Structure of Enceladus
6. Configuration of the ocean floor
What we want to investigate?
What we want to find?
1. RNA
2. DNA
3. Amino Acid
4. H2S
5. CH4 , NH3
-Camera
-Sonar
-Laser spectrometer
-GC-MS
-Seismography
Instruments
Instruments - Camera
-At least, two kinds of lens one for visible, other for infrared
-Take pictures
-Make videos
-Investigate temperature
-Find out the most thin layer
Instruments - Sonar
Principle of Sonar
- The principle : Reflection of supersonic waves.
Mapping
- Map the geographical features.
Instruments - Laser Spectrometer
- Composition of the gas
- Whether there are some particles or not.
?
Instruments – GC/MS(Gas Chromatography/Mass
Spectrometry)
Gas Chromatograph
MassSpectrometry
Inner Structure of GC/MS
- identify unknown samples that we collected.
Using GC/MS
- Observe unknown samples’ Periodical changes of composition
Instruments - Seismography
- Investigating the inner structure of Enceladus
- Using 3 Seismography forming an equilateral triangle shape.
III. Launching and investigation
Where is the most interesting place?
-The south pole
And why??
-geysers-Biomarkers
Timeline
Feb, 2027 Lander completes dissolving ice. Separate submarine(probe) and start probing.
Jan, 2020 Lift off. Aug, 2021 Swing by at Venus. Oct, 2021 Swing by at Earth.
Apr, 2023 Swing by at Jupiter.
Sep, 2026 Go into the Saturn's orbit
Nov, 2026 Go into the Enceladus' orbit, start mapping.
Dec, 2026 Dropping lander and three seismographs Lander starts dissolving ice
seismography
lander
spacecraft
Find appropriate area by using Thermal/visible camera
The Front Of Submarine
Thermal/visible
Camera
Thermal/visible
Camera
Thermal/visible
Camera
Thermal/visible
Camera
1. Find small particles easily
2. Increase the probability that we find biomarkers
3. Measure changes of composition
The Side Of Submarine
Sonar
LaserSpectromete
r
Antenna
GC/MS
Computer
RTG
Mapping configuration of the ocean floor
!
Small particles
Searching for samples to collect
Collectparticles
Submarine
SpacecraftCommunication
Why is Our Mission Special?
1. Find small particles easily
2. Increase the probability that we find biomarkers
3. Measure changes of composition
Other Investigations that we can Offer
1. Ocean current
2. Magnetite
3. Environment inside the crust
Question?!
Thank you!