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Running head: THE MARS CURIOSITY ROVER
The Mars Curiosity Rover
Li Yan (Lee)
University of New Hampshire
1
THE MARS CURIOSITY ROVER
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The Mars Curiosity rover
Introductory statement
The exploration of the planet for signs of life has been a major endeavor scientist. The
great story of the massive exploration captures the interest of the scientists after what was a
general exploration of the solar system captured the images of Mars. This picture created a
point of interest among the scientists in the field of astronomy. NASA has been on the
frontline in this voyage, creating and sending spaceships to carry out the expenditure. Various
missions have been launched to Mars with some hit unsuccessful ends. There is about five
orbiters spaceship going around the orbit of Mars and gathering data from the planet that only
seems to qualify as the earth’s distant cousin.
The picture, images, and the data collected from the spaceships could not provide
sufficient evidence to determine whether Mars ever supported or can support life. For this
reason, the scientist saw the need to send an explorer and land it at the surface of the red
planet. Through this way more detailed data on the capabilities of the planet to support life
especially on the aspects of water and air qualities. The two successful landers and rovers are
Mars exploration rover (Opportunity) and the Curiosity of the Mars Science Laboratory.
This paper will be developed to describe the mission of the Curiosity Mars rover. It
will analyze in details the capability of this ship that makes it well suited for the exploration
mission. The primary functions that Curiosity was launched to perform. The paper will also
report on the progress on the NASA main purpose on the attempts to determine ad gather
evidence that Mars habitat supports life or once supported life.
Mission
The Curiosity rover was launched from the Cape Canaveral Air Force base on 26th
November 2011. The rover was destined to land at the Gale Crater on the surface of Mars.
The primary mission was destined to take 23 months. (NASA). The main goals of the
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Curiosity were to gather evidence to help establish whether Mars had the ability to support
life, to analyzes the role of water, and to explore the climatic and geological conditions of the
planet. All this was seen as paving the way for future human exploration. To achieve these
goals, the mission of Curiosity was subdivided into categories each representing objectives.
These are biological, geological and the planetary process. The biological objective seeks to
address the issues of organic carbon compounds, chemicals regarded as a basic block of life
and the biological processes. In the geological objective, Curiosity was charged with to
research on the rocks and mineral composition. The planetary process was meant to address
the evolution process and the possible water and carbon dioxide cycles (Trebi, 2013).
Major Curiosity Rover’s technological components
Curiosity Rover developed by the Mars science laboratory was comprised of 77% of
its total mass as gears destined to ensure its safe transfer from the earth and to ensure a soft
landing on the surface of the earth. Only 23% of the total mass of the spacecraft was to be
used for carrying out the exploration mission. The active weight of Curiosity Rover including
the technological and scientific apparatus is 80kgs.
The powering of the Curiosity is conducted through radioisotope thermoelectric
generator (Trepi, 2013). These systems generate electricity to power the rover ad is systems
from the decomposition of radioactive isotopes mostly used being plutonium. The systems
were developed by Rocket dyne and Teledyne energy systems. The electricity is used to
recharge batteries to supply power. The stored energy facilitate to fulfill high peak power
demands of the systems when the same can be attained through the operation of the
generators optimal functionality and output level (Serafim, 2012).
The Curiosity Rover has advanced communications devices. According to Serafim
(2012) describes these communication devices. The Rovers bear’s three antennas; the X-band
transmitter with an ability of 400 megahertz. It also has a UHF electro-life controlled radio.
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These communications systems facilitate sending of signals back to earth with a delay of only
13 minutes and 46 seconds.
The computer component of the curiosity is one that is slow, with little storage
capabilities even less than that of a smartphone but well adapted for the rugged terrain on the
surface of the Mars (Harwood, 2012). The computer described as the PowerPC RAD750 is
built to withstand extremely high temperature and to deal with a large amount of radiations
that would cripple other computers. This computer is also built with chips that are long
lasting thereby not demanding intervention from earth which may sabotage the mission.
The Curiosity rover has an inbuilt heat rejection system. Mars records varied
temperature levels ranging from -127-40 degrees Celsius. Mostly the heating system will
require warming the system. Heating in the rover is achieved by strategic placing electric
heaters close to the key components and working the heat rejection systems. This system
operates by using a fluid around the essential components that absorb heat and helps maintain
their temperature at optimal.
The mobility of the Curiosity rover has six wheels with rocker-bogie suspension.
Every wheel has cleats, and gearing is done independently to ensure the movement on the
soft sand and rocky surface. The vehicle is well adapted for making arch turns with the ability
to steer each front and back wheel independently (Harwood, 2012).
Serafim (2012) describes the cameras installed in the Curiosity rover. The rover has
17 cameras. The best of them are the Mast Camera instrument that bears a 100-mm focal
length and a 34mm focal-length camera. It also carries four pairs of hazards avoidance
cameras known as Hazcam and navigation cameras.
The Curiosity rover is also fitted with a robotic that is very flexible with three joints at
the shoulder, elbow, and the wrist. The arms can extend for 7 feet. The end of the arm has a
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turret used to hold five devices; an alpha particle x-ray, a hand lens imager and on an addition
to three devices for gathering samples.
To ensure the performance of its core functions, the Curiosity rover is made to operate
many instruments. Among then include alpha-particle X-ray, chemical and mineralogy
device, sample analysis, assessment radiation tracker, the dynamic albedo of neutrons, an
environmental monitoring station equips with a meteorological package and a UV sensor.
The Curiosity Rover touchdown
The Curiosity used a guided entry for the atmospheric to improve the landing
accuracy (Trebi, 2013). The landing is initiated with the cruise separation from the spacecraft.
This is then followed by a deceleration towards the surface of the Mars leading to heating.
The guided entry has followed a path that was a horizontal flight. During the parachute
descent, there was the separation of the heat shield and the back shell from where the
spacecraft underwent a powered descent from the sky crane that designed a place for the
rover’s touchdown.
The findings of the Curiosity Rover.
The curiosity made a discovery that some years back, Mars had the right conditions to
support life. The chemical conditions were found to have been suitable for living microbes to
survive. The chemical elements included sulfur, nitrogen, oxygen, phosphorus and carbon
which are key element required to sustain life (NASA, 2015). Some samples collected some
clay particles with low levels of salt a possible indication that there once flowed fresh water
on those zones.
The Curiosity rover also discovered elements of organic carbon on the rocks from the
surface of Mars. The organic components are considered to be the building blocking of living
organisms. This sample was gathered by the sample analysis at Mars. Although this is not
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conclusive evidence of present or past life, it portrays the availability of essentials of life
(NASA, 2015).
Another key finding on this red planet by Curiosity rover was the presence of preset
and active methane in the atmosphere (NASA, 2015). This was discovered by the Tunable
laser spectrometer in the SAM, and it recorded an increase of ten-fold within a period of two
months. This was an intriguing discovery as one possible source of methane is living things
or a reaction between rock and water.
The radiation levels on Mars were rated as a big health risk for a human. The
radiation assessment detector discovered two harmful rays on the deep space which could be
hazardous to the astronaut’s health. These rays are the galactic cosmic rays and the solar
energetic particles (NASA, 2015).
Conclusion
With the continued universe exploration, voyages to planet Mars have been
considered as essentially important. The main agenda has been to evaluate the planet’s
capabilities to support life. It is for this reason that the Curiosity Rover was commissioned
and deployed to Mars. The rover was designed and built with advanced technical capabilities
to facilitate a successful mission. The instruments installed allowed for the collection of data,
and samples, testing them, capturing images and relying on the information back to earth.
The rover was built with mobility capabilities to help in navigating on Mars’ rugged terrain.
The computer in the Curiosity rover was built to withstand extreme heat and radiations.
The major discoveries provided evidence pointing to that Mars may have at one time
supported life. The discovery of organic compound and increasing the level of methane in the
atmosphere. The rover also discovered that the radiation levels would be a threat to the health
well-being of human.
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References
Harwood, W. (2012, August). Slow, but rugged, curiosity's computer was built for
Mars. Retrieved from http://www.cnet.com/news/slow-but-rugged-curiositys-computer-wasbuilt-for-mars/
NASA. (2015). Results of Curiosity Rover. Retrieved from
http://mars.nasa.gov/msl/mission/science/results/
Serafim, M. (2012, August). NASA's curiosity over- Technical specifications.
Trebi, A. (2013, March). Robotic exploration of Mars: Curiosity Rover, Phoenix Mars
Lander and Mars Exploration rovers (Spirit & Opportunity).
OMT COURSE X
1
A Modern View of the Universe 1
1.1 The scale of the Universe 2
What is our place in the universe 2
con misconceptions The Meaning of a Lightyear 2
How is the universe? 6
con misconceptions Confusing very Dent
Things
tools of science in the Man
1.2 The History of the Universe 10
How did we come to be? 10
How do our lifetimes compare to the
age of the universe? 12
THE PROCESS OF SCIENCE IN ACTION 13
1.3 Defining Planets 13
What planet? 14
3 Changes in Our Perspective 36
3.1 From Earth-Centered to Sun-Centered 37
How did the Greeks explain planetary motion 37
common misconceptions Columbus and a farth
How did the Copernican revolution change our view
the universe 3
3.2 Hallmarks of Science 43
tools of science scope 43
How can we distinguin scene from onscience? 46
content Fire 11 The Chorcanvi
common misconceptions for on the rounox
What is a scientific theory? 48
THE PROCESS OF SCIENCE IN ACTION 4
3.3 The Fact and Theory of Gravity 49
How does the fact of gravity differ from the theory of
Bravity 50
2 Understanding the sky 18
21 Understanding the Seasons 19
What causes the seasonst 19
comic context. Foare 23. Seasons 20
common misconceptions me cause of seasons 22
common misconceptions: gh Noon 23
Why do the constellations we see depend
on the time of year? 23
2.2 Understanding the Moon 26
Why do we see phases of the Moon? 26
common misconceptions: Shadows and the Moon 26
common misconceptions: Moon in the Daytime 27
common misconceptions: Me Dark Side of the Moon 28
What causes eclipses? 28
tools of science: Angular Sizes and Distances 29
THE PROCESS OF SCIENCE IN ACTION 31
2.3 The Puzzle of Planetary Motion 31
Why did the ancient Greeks reject the real explanation
for planetary motion? 32
4
Origin of the Solar System 54
4.1 Characteristics of the Solar System 55
What does the solar system look like? 55
comic context Figure 4.1 The Sole System 56
What features of our solar system provide clues
to how it formed? 61
tools of science: Conservations 2
4.2 The Birth of the Solar System 63
What theory best explains the orderly patterns of motion
in our solar system? 83
How does our theory account for the features of planets
moons and small bodies? 65
common misconceptions Solar Grity and the Density
of planets 66
THE PROCESS OF SCIENCE IN ACTION 71
4.3 The Age of the Solar System 71
How do we determine the age of Earth
and the solar system? 71
VI
7. Extrasolar Planets and the Netheory 124
PROCESSO SECTION
Do we need your of som
Somont 124
5 Terrestrial Worlds 75
5.1 Terrestrial Surfaces and Atmospheres 76
What determines a world's level of geolocal
common misconceptions For Me
Lave
How does an atmosphere we conditions for
tools of science Properties of
5.2 Histories of the Terrestrial Worlds 82
Why did the terrestrial worlds out to me
What unique features of Earth are mortato
de78
common misconceptions why the sky
e THE PROCESS OF SCIENCE IN ACHON
5.3 Global Warming 90
What is the evidence for global warming
8 The Sun and Other Stars 128
8.1 Properties of the Sun 129
Why does the sunshine 129
How does energy escape from the Sunt 130
common misconceptions The Sun Noon
ols of science: Spectroscopy 132
2 Properties of other stars 134
How do we measure the properties of stars 134
common misconceptions Photos of Stars
What patterns to we find in the properties of stars
THE PROCESS OF SCIENCE IN ACTION 140
3.3 Visualizing Patterns Among Stars 140
How did we discover the patterns into propri
comic context Figure 1.17. Reading an HR Dugan
common misconceptions The Grect
6 The Outer Solar System 95
6.1 Jovian Planets, Rings, and Moons 96
What are joven planets?
tools of science: Newton's version of pler's
Third Law 97
Why are jovian moons so geologically active? 100
6.2 Asteroids, Comets, and the impact Threat 106
Why are asteroids and comes grouped into
three distinct regions? 106
common misconceptions: Dodge Those Astenes 106
Do small boties pose an impact threat to Earth? 108
THE PROCESS OF SCIENCE IN ACTION 109
-3 Extinction of the Dinosaurs 109
Did an impact kw the dinosaurs? 109
9 stellar Lives 146
9.1 Lives in Balance 147
Why do stars shine so steadily? 147
Why do a star's properties depend on its mass?
9.2 Star Death 152
tools of science: Ouantum Laws and Astronomy
What will happen when our Sunruns out of fuel?
How to high-mass stars end their lives? 155
THE PROCESS OF SCIENCE IN ACTION 159
9.3 Testing Stellar Models with Star Clusters
What do star clusters reveal about the lives of st
cosmic context. Figure 9.25 Stellar Lives 162
10 The Bizarre Stellar Graveyard
Planets Around Other Stars 113
Detecting Planets Around Other Stars 114
How do we detect planets around other stars? 114
tools of science: The Doppler Erfect 116
What properties of extrasolar planets can we
measure? 117
cosmic context. Figure 7.6 Dicting Expo Planets 118
Characteristics of Extrasolar Planets 120
How do extrasolar planets compare with planets in our
solar system? 121
are Earth-like planets common? 123
10.1 White Dwarfs and Neutron Stars 167
What are white dwarfs? 167
What are neutron stars? 169
10.2 Black Holes 171
What are black holes? 171
tools of science: Einstein's Theories of Relath
What happens to space and time near a blac
common misconceptions: Black Holes Don't
CAUTION 1
Saching for Black Hole 176
Dar1
11 caden
11.1 Our Galaxy The Milky Way 13
What does outcally 183
tocis of science
Commons
How did the My Way Tom 187
11.2 Galaxies Beyond the Milky Way 189
What are the mor types of west 189
why does 101
THE PROCESS OF SCIENCE IN ACTION 19
11.3 Seeking Supermassive Black Holes 193
What is the evidence for supermasse black holes
at the centers of galaxies? 194
12 Galaxy Distances and Hubble's
w dobervations of the comic microwave
bacon scoort the ant theory? 219
con contre 3. The caly uvese 220
How do the abundance of elements soport
the Big Bang Theory z
THE PROCESS OF SCIENCE IN ACTION 234
13.3 Inflation 224
Did the need any episode of inition
14 Dark Matter and Dark Energy 22
14.1 Evidence for Dark Matter 231
What is the evidence for dark matter? 221
tools of science The Velocity Formula 233
What might dark matter be made of? 236
14.2 Gravity versus Expansion 237
How did structures like galaxies form? 237
Comic contexte Evolution 2
Will the universe continue expanding forever? 2
THE PROCESS OF SCIENCE IN ACTION 243
14.3 Evidence for Dark Energy 243
What is the evidence for dalk energy? 243
Cosmic context roure 12 17 Dark Matter and Da
Energy 245
15 Life in the Universe 250
15.1 The Search for Life in the Solar System
What are the necessities of tey 25t
Could there be life elsewhere in our solar syster
15.2 The Search for Life Among the Stars 2
How can we dentify habitable planets? 255
tools of science Planetary Spacecraft 255
is there intelligent life beyond Earth257
THE PROCESS OF SCIENCE IN ACTION 2
15.3 Evolution on Earth and Beyond 261
What is the evidence for evolution? 262
come context: Figure 15.11 A Universe of
CREDITS 268
Law 198
12.1 Measuring Cosmic Distances 199
How do we measure the distances to gais? 199
tools of science Measuring stances with standard
Cards 200
What is Hubble's law? 202
12.2 The implications of Hubble's Law 204
in what sense is the universe expanding? 204
How do distance measurements tell us the age of the
universe? 206
common misconceptions: Wome Universe
Expanding into 2016
THE PROCESS OF SCIENCE IN ACTION 205
12.3 Observing Galaxy Evolution 208
What do we see when we look back through time 208
common misconceptions: Beyond the Horizon 202
13 The Birth of the Universe 213
13.1 The Big Bang Theory 214
Appendixes A-1
A Useful Numbers A-2
B Useful Formulas A-3
C A Few Mathematical Skills A-4
What were conditions like in the early universe7 214
tools of science: Particle Acceleratons 215
How did the early universe change with time? 216
13.2 Evidence for the Big Bang 219
GLOSSARY G-1
INDEX 1
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Research Paper (Physics 405 only)
All 405 students, in lieu of the laboratory part of the course, will write a research paper. Th
e due date for this paper is Monday, April 16. If you miss the deadline, your grade for the p
aper will be reduced by 1 point out of a possible 15 for every day after the deadline. Ther
esearch paper should be nine double-spaced pages in 12-point font (exclusive of figures o
r references), with one-inch margins. 6 Physics 405n Spring 2018 What are legitimate topi
cs? There are many possible topics so I urge you not to anguish over it. Pick something th
at sounds interesting and go with it. Feel free to ask me or our TAs. I can offer suggestion
s if you are unsure of your choice. You will undoubtedly find plenty of material work wit
h. Here are some suggestions for general topic areas:
Discussion of some current astronomical discovery. The Mars Curiosity rover, a future orc
urrent space mission, New Horizons, Dawn, Juno, the Europa mission, the James Webb Sp
ace Telescope, are all examples of interesting topics. There are tons on the web on these
topics and many others.
MESSENGER that orbited around Mercury until April of last year, Kepler spacecraft
discoveries, extrasolar planets, future or current observatories, an observatory on the
Moon; is it a good idea?
Discussion of an astronomical system that you find particularly interesting. • The James
Webb Space Telescope JWST)
The world's largest radio telescope in China (Guizhou Province). The Hubble Space Tel
escope (HST)
The influence of astronomy on society, or the international space programs. • Historical pe
rspective on some aspect of astronomy or the space program. Biographies are always go
od. There are plenty of interesting figures in astronomy. · Politics and astronomy and/or th
e space program or US space policy or the lack of one
You should also feel free to pick a different topic of your own design. If you are having dif
ficulty doing so, ask me or one of the TAs for help. There is plenty of fertile material out th
ere, so don't stress-out or fear that someone else is covering the same topic.
After choosing your topic, gather materials and information, synthesize the material and f
ormulate what you would like to say. Don't just be a stenographer, parroting the material y
ou find, but develop and express your own ideas and opinions. As you read the researched
material carefully, your own observations and questions will arise. When drafting your pap
er, follow the format of first introducing your subject, including a brief statement of what y
ou are going to tell the reader. Then present the material that is relevant for your discussio
n and make your main points, supported by sources with citations. Discuss why your topic
and/or discussion is interesting or important, and finish with some concluding remarks. Be
careful to avoid embarrassment through the cavalier use of auto correction and spell chec
ker tools. Use your best grammar. Read the text aloud-you uncover many ghastly failings
of your composition that way, and, have someone else you trust, read your paper before y
ou turn it in.
When you first draft your paper, don't worry too much about the formatting (i.e., figures, pro
per bibliographic style, etc.). The point of your first draft is to get a coherent manuscript th
at tells a story and holds water. After completing your first draft (or even before this point)
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