Curiosity - columbusastronomy
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Transcript Curiosity - columbusastronomy
CURIOSITY
Antoine Henderson
Fiona Ward
Launch and Landing
Launched:
Landed: August 6, 2012
November 26, 2011
August 6, 2012
Cape Canaveral, Florida
Aeolis Palus, Gale Crater
Objectives
Biological
Determine the nature and inventory of organic carbon compounds.
Inventory the chemical building blocks of life.
Carbon, Hydrogen, Nitrogen, Oxygen, Phosphorous, Sulfur
Identify features that may represent the effects of biological processes.
Geological and Geochemical
Investigate the chemical, isotopic, and mineralogical composition of the Martian
surface and near-surface geological materials.
Interpret the processes that have formed and modified rocks and soils.
Objectives
Planetary Processes
Assess long-timescale atmospheric evolution processes.
Determine present state, distribution, and cycling of water and carbon dioxide.
Surface Radiation
Characterize the broad spectrum of surface radiation, including galactic cosmic
radiation, solar proton events, and secondary neutrons.
Goals
Determine Possibility of Ancient Life on Mars
Conditions Needed for Life to Thrive
Looking for Life Signs
Characterize the Climate of Mars
What's the Martian Climate Like Today?
What Can the Current Climate on Mars Reveal about the Past?
Characterize the Geology of Mars
The Magnetism of Mars Gives Clues to the Planet's Interior and More
Rocks on Mars Can Tell Us About the Planet's History and Its Potential for Harboring Life
Prepare for Human Exploration
Astronaut Safety in the Hostile Martian Environment
Robotic Spacecraft Will Pave the Way for Human Exploration of Mars
Technology
Mars Science Laboratory (MSL)
Mass: 899kg
2.9m x 2.7m x 2.2m
Power Source: Radioisotope
Thermoelectric Generator
(RTG)
Computers: Rover Computer
Element (RCE)
Robotic arm
Communications: X band
transmitter and receiver, UHF
Electra-Lite software-defined
radio
Mobility: Rocker-Bogie system
17 cameras:
HazCams (8), NavCams (4),
MastCams (2), MAHLI (1),
MARDI (1), and ChemCam
(1).
Accomplishments
Atmospheric Composition
Mars has no traces of
Methane.
Rock Samples
Discovery of Streambed Gravel
Evidence of Flowing Water
Curiosity Identifies Traces of:
Sulfur
Nitrogen
Hydrogen
Oxygen
Phosphorous
Carbon
Ancient Streambed