Climate Change on Mars - By Peter J. Sherman Astrobiology, Harvard Summer School August 2011

Page created by Nicole Silva
 
CONTINUE READING
Climate Change on Mars - By Peter J. Sherman Astrobiology, Harvard Summer School August 2011
Climate Change
    on Mars

By Peter J. Sherman
Astrobiology, Harvard Summer School
            August 2011
Climate Change on Mars - By Peter J. Sherman Astrobiology, Harvard Summer School August 2011
Mars is the sole planet whose surface can be observed from Earth using a

telescope. Due to the clear view of the Martian surface from Earth, humans have

long been intrigued by the possibility of life in outer space. While the human

interest in extraterrestrial life has been existent for many centuries, viewing the

universe from Mars’ perspective had not been feasible until a few decades ago.

On July 14, 1965, NASA sent Mariner 4 to Mars. Mariner 4 was the first probe

sent by any space organization to successfully orbit Mars. From Mariner 4, we

learned about what we were dealing with on Mars; the images showed a

seemingly lifeless planet with craters that greatly ranged in size. Important to

note from the results was the low atmospheric pressure (4.1 to 7.0 mb) and

temperatures (-100 C) and the lack of a magnetic field on the surface of Mars

(http://www.astronautix.com/project/mariner.htm). Although Mariner 4’s planetary expedition occurred

just over 45 years ago, we have discovered much more about Mars through

more expeditions.

        We have recently sent more probes to Mars to provide us with information

about the potentiality of life outside of Earth. These space missions have helped

to determine the characteristics of Mars and whether life could be sustainable.

Probes have found signs of erosion and liquid water on the surface of Mars.

With well-designed probes like these, we should be able to find even more

information about Mars.

        Aside from NASA’s most recent discovery of craters forming salty, liquid

water just a few days ago, NASA was also recently baffled by the fact that parts

of Planum Australe, the Martian south pole, was evaporating into the
atmosphere. Fenton 2007 compared two images taken by the Mars Global

Surveyor, one in 1977 and 1999 (http://www.skepticalscience.com/Climate-Change-on-Mars.html). It is known

Planum Australe is primarily composed of water ice and dry ice, with some parts

being permafrost and others being seasonal. Based on the two images 23 years

apart, NASA noted that not only the seasonal ice caps disappeared, but also

parts of the permafrost. The disappearance of parts of the permafrost ice caps

can best be attributed to the rapidly growing average surface temperature which,

in fact, has increased by an astonishing .5 C since 1970

(http://www.timesonline.co.uk/tol/news/uk/article1720024.ece), a rapid average climate change which is very

similar to that of ours on Earth due to global warming. If Mars’ atmosphere were

being blasted away by solar winds (due to its lack of a magnetic field), large

asteroids, and Mars’ own internal workings, Mars would deal with a significantly

weaker greenhouse effect; there would be less of an atmosphere to insulate the

rays from the sun on Mars. This would lead to a much colder Mars. The

stripping of the Martian atmosphere begs the question as to how it would be

possible for the average temperature to rise (at a fast rate) when all of its

insulation is rapidly disappearing.

         Scientists have tried to determine possible reasons as to why the average

Martian temperature would rapidly increase despite a shrinking atmosphere.

People have attempted to explain this phenomenon through many different

theories, based off of the many characteristics of Mars and its history. These

theories run the gamut from solar irradiance on Mars to large global dust storms

which change the composition of Mars’ atmosphere. This research paper will go
over possible theories for the increased average surface temperature and

determine the validity of each one. It will start by investigating dust storms and

strong winds due to Mars’ low thermal inertia and the Martian wobble (caused by

its tilt and rotation) as possible catalysts for the large climate change that

scientists have witnessed over the past 40 years. Then, it will look at how these

small changes in the Martian environment could have led to a lower albedo and

how that could have affected the Martian climate change. This researcher will

then determine the validity of these theories or whether Mars is heating up simply

because of solar irradiance, solar cycle variations which affect the average

temperature of all planets in the sun’s orbit. Solar cycles could be used to

explain Mars’ as well as Earth’s global warming as a natural occurrence – not

completely man-made. This paper will then proceed to determine the final

location of the evaporated Martian water from the polar ice caps, as we know

that, because of probes, water vapor is an extremely small component of the

Martian atmosphere. If the Martian atmosphere is composed of only a small

amount of water vapor, where is all the water vapor going if the polar ice caps

are evaporating? Finally, this paper will conclude with a discussion as to which

theory has the most validity to its claim. A variety of factors could have

potentially influenced the current climate change on Mars, but do some hold

more validity than others?

         Mars has a low thermal inertia; when the sun shines on the surface, it

heats up quickly, and when the sun’s rays do not hit the surface, Mars cools

down almost immediately. The low thermal inertia of Mars can be seen though
its daily temperature swings, which can have a range as large as 100 K per day

(http://en.wikipedia.org/wiki/Climate_of_Mars). Like on Earth, the temperature swings on the surface of

Mars lead to large                                                                  windstorms –

significantly larger than                                                           that on Earth because

the temperature swings                                                              are much greater on

Mars. These large                                                                   Martian windstorms

contribute two things to                                                            their environment; they

trap heat on Mars and they                                                       throw everything on the
                                          Figure 1: This is an
surface of Mars around,                 image of Mars taken in                   like a Martian version of a
                                       2001. In the bottom right
                                         corner, a light patch of
tornado. The Martian                      brown can be seen,                     wind’s ability to trap heat
                                        indicating a dust storm.
could be an explanation of             http://en.wikipedia.org/wiki/File:Mars_   the beginning for Mars’
                                                     pits 1999.gif

rapid climate change. When the Mariner 9 probe first landed on Mars in 1971,

NASA noticed that all the images taken were difficult to see. The images were

unclear due to a large dust storm that encompassed a large portion of the planet.

We later found out that these dust storms are a frequent occurrence on Mars

because winds only need to be around 40-50 miles per hour to cause such

storms (http://en.wikipedia.org/wiki/Climate_of_Mars). Strong enough winds would shoot dust from

Mars’ surface into the air. This also occurs on Earth, but on Mars, the dust

becomes an important contributor to the atmosphere because there is more of it

and because of precipitation. On Earth, we are able to get rid of dust in our

atmosphere, before it can become a major contributor to the atmosphere

through, precipitation. This process of precipitation requires too warm a

temperature and too high an atmospheric pressure to currently occur on Mars.
Therefore, while the dust thrown into the wind on Earth is cleaned out of the

atmosphere by precipitation, more dust on Mars (because there are stronger

winds) is left in the atmosphere. The combination of heat trapped by the large

surface winds and no loss of heat from the atmosphere (that is neither growing

nor shrinking because the Mars’ surface dust counters the affects of the Martian

atmosphere stripping) could be an explanation for the beginning of the increased

average surface temperatures on Mars since the late 1970s. This is an

extremely plausible theory because there are many images of large windstorms

on Mars, like in Figure 1, which indicate large quantities of dust being thrown into

the air all over the Martian surface. What other scientific theories have been

taken into account as possibilities for the climate change on Mars?

       Every planet in our solar system experiences a wobble due to the

gravitational                                                                          pull from the

sun with                                                                               respect to its

tilt from the                                                                          rotational axis.

Changes in                                                                             the tilt, as

small as they                                                                          may be, can

result in                                                                              drastic climate

changes.                                                                               Milutin

Milankovitch,                                                                          a renowned

Serbian

mathematician, noticed that      Figure 2: This diagram
                                                                           Earth’s average surface
                                 indicates the relation of
                                degrees to the change in
                                    temperature in the
                                    Vostok ice core in
                                   Milankovitch cycles.
                                http://en.wikipedia.org/wiki/File:Milank
                                   ovitchCyclesOrbitandCores.png
temperature was directly related to its axial tilt from its orbital plane. As the axial

tilt decreases, the seasons have much milder temperatures because the sunlight

hits the entire surface of Earth with the same amount of power. This is the

opposite from when the axial tilt is large because the seasons will be extremely

polarized due to sunlight shining brightly on some areas of Earth and little on

others (http://www.universetoday.com/14894/mars-tilt/). Milankovitch addressed the relationship of

Earth’s axial tilt versus Earth’s average surface temperature, which had a period

of around 41,000 years (http://en.wikipedia.org/wiki/Milankovitch_cycles). This relationship is known as

Milankovitch Cycles, which are similar to a sinusoidal function. While Earth and

Mars are not entirely characteristically similar, similar cycles can be attributed to

Mars, as well. Mars’ axial tilt is currently increasing, which is making the

summers hotter and the winters colder. Martian seasons are about twice as long

as Earth’s seasons. With a hotter summer, the seasonal martian polar ice caps

on Mars evaporate into the atmosphere at a faster rate than usual. Even some

of the permafrost on Mars evaporates due to the strong effects of the axial tilt.

This could be a plausible explanation for the Martian climate change because the

summers would be hotter than usual, and the polar ice caps would evaporate into

the atmosphere.

        A few other scientists believe that a change in solar irradiation was the

catalyst for climate change on both Earth and Mars. Solar irradiance is “the

amount of solar energy that arrives at a specific area at a specific time.”

(http://www.oilgae.com/ref/glos/solar_irradiance.html). Over the past few decades, some scientists have

noted a slight distinction in the amount of solar irradiation received by Earth,
which varied by about .2% (http://en.wikipedia.org/wiki/Solar_variation#Solar_irradiance_of_Earth_and_its_surface).

Comparing solar irradiation versus time, scientists saw a sinusoidal graph, as

shown in Figure 3. In this belief of solar irradiation, the amount of power

received is not the only thing changing; ultraviolet irradiance and solar winds are

also greatly impacted. While there is a percent variation of just .2% for total

irradiance, things such as UV irradiance have greatly changed over the past few

centuries. The UV irradiance has increased by 4.3% since the Maunder

Minimum (a period from 1645-1715 where sunspots were seldom seen by solar

observers), and the sun’s magnetic flux has increased by a factor of 2.3 since

1901 (http://en.wikipedia.org/wiki/Solar_variation#Changes_in_total_irradiance). The increase of UV radiation and

the sun’s magnetic flux over the past few centuries would be an indication of

climate change, not just on Earth, but in our entire solar system. This means that

all planets in our solar system would have a parallel global warming; everyone is

increasing temperature at the same rate. A parallel global warming would concur

with the evidence that Mars and Earth have increased average surface

temperatures of about the same rate over the past 40 years. While this theory is

backed by a few scientists, it is widely regarded as ludicrous by the majority of

the scientific community. Aside from the many other reasons why this theory is a

tad bit preposterous, this theory also claims that humans have no impact

whatsoever on our current climate change on Earth. Not only does this theory

make little physical sense, solar irradiance could also be attributed to the elliptical

rotations of the planets around the sun. Although this theory receives censure

from the large majority of the scientific community, the solar irradiance theory
agrees with both the wind-                  Figure 3: This graph
                                                                                 dust storm and axial tilt
                                            shows the amount of
theories in that they show                 solar flux received per               that Mars is rapidly heating
                                            year. The function is
                                                  sinusoidal
up, and causing its polar                                                        ice caps to evaporate into
                                         http://wattsupwiththat.com/2009/05/14
                                             /the-solar-radio-microwave-flux/
the atmosphere. However                                                          Mars has an incredibly thin

atmosphere, and water vapor composes only .03% of its atmosphere

(http://www.daviddarling.info/encyclopedia/M/Marsatmos.html). Since Mars has a thin atmosphere and water

vapor is an infinitesimal portion of it, water vapor is, essentially, non-existent in

the Martian atmosphere. Where is the final destination of the evaporated water if

it is essentially not in the composition of the Martian atmosphere?

                                                                  2GM
        We have learned in class that v esc =                         . Although the radius of Mars
                                                                    r

is about 50% of Earth’s radius, the mass of Mars is about 11% of Earth’s mass.

Using the equation, this means that the escape velocity is going to be

significantly smaller on Mars compared to Earth. A smaller escape velocity

means that a significantly larger amount particles are able to escape from the

Martian atmosphere in comparison to Earth’s atmosphere. In class, we have

                                                  3KT
also learned the equation vThermal =                  . Using 218 K as the average
                                                   m

temperature on Mars, we find that vThermal = 17.36800756 m/s. Using 3,376.2 km
as the radius of Mars and 6.4185 * 1023 kg, we can plug these variables into the

escape velocity equation. We find that vesc = 5027 m/s. Since the escape

velocity only needs to be six times greater than the thermal velocity, and

5027/17.36800756 = 289.2392482, water vapor is able to escape out of the

Martian atmosphere and into space. Will the disappearing ice have an impact on

the average surface temperature on Mars?

       Since ice is a brighter surface than liquid water, it has a higher albedo.

Albedo is the reflectivity

of an object. The higher

the albedo an object has,

the less amount of light

the object can absorb.

The lower the refelectivity

the more the surface of

the object can heat up.

When Mars was given a slight heat                                                     boost from
                                                 Figure 4: This figure
either wind-dust storms, an increased          indicates what happens                 axial tilt, or
                                                  when the albedo is
                                               lowered. This occurred
solar irradiation, the seasonal ice, and         on Mars through the                  even some of
                                                original melting of ice.
the permafrost, began to melt. This            http://maps.grida.no/go/graphic/ice-
                                                                                      decreased the
                                                     albedo-feedback-process

albedo of Mars because there was less                                                 ice covering

the surface. This in turn led to a rapid heating on the surface of Mars, and can

explain the .5 C increased temperature over the last 40 years. Now that we
know the end result of this whole process, which heating process makes the

most sense for Mars?

       I believe that each of the three theories played a role, whether large or

small, in the process of evaporating ice on Mars. Certain concepts from each of

these theories could be an explanation for what has been a big question mark for

scientists over the past few years of noticing this change. Wind-dust storms, the

axial tilt, and solar irradiance could have all greatly been catalysts for the climate

change on Mars over the past few decades, which led to the lower albedo on

Mars. Climate change is becoming an important topic to discuss, not just for

Earth, but for Mars, as well.
WORKS CITED

1. "Climate change hits Mars." The Sunday TImes. N.p., 29 Apr. 2007. Web.

   8 Aug. 2011.

   .

2. Wikipedia contributors. "Climate of Mars." Wikipedia, The Free

   Encyclopedia. Wikipedia, The Free Encyclopedia, 5 Aug. 2011. Web. 8

   Aug. 2011.

3. Wikipedia contributors. "Solar variation." Wikipedia, The Free

   Encyclopedia. Wikipedia, The Free Encyclopedia, 21 Jul. 2011. Web. 8

   Aug. 2011.

4. "Global warming and climate forcing by recent albedo changes on Mars."

   Nature International Weekly Journal of Science (Feb. 2007): n. pag.

   Nature Publishing Group. Web. 8 Aug. 2011.

5. "Mars Melt Hints at Solar, Not Human, Causing for Global Warming,

   Scientist Says." National Geographic 28 Oct. 2010: n. pag. National

   Geographic. Web. 8 Aug. 2011.

   .

6. Cook, John. "Climate Change on Mars." Skeptical Science. N.p., 13 Mar.

   2008. Web. 8 Aug. 2011. .
7. Wikipedia contributors. "Mars." Wikipedia, The Free Encyclopedia.

   Wikipedia, The Free Encyclopedia, 7 Aug. 2011. Web. 8 Aug. 2011.

8. Barry, Patrick. "A Tale of Planetary Woe." NASA. N.p., 6 Nov. 2009. Web.

   8 Aug. 2011. .

9. "Evidence for Recent Climate Change on Mars." Malin Space Science

   Systems. N.p., 6 Dec. 2001. Web. 8 Aug. 2011.

   .

10. Wikipedia contributors. "Milankovitch cycles." Wikipedia, The Free

   Encyclopedia. Wikipedia, The Free Encyclopedia, 8 Aug. 2011. Web. 8

   Aug. 2011.

11. Wikipedia contributors. "Solar variation." Wikipedia, The Free

   Encyclopedia. Wikipedia, The Free Encyclopedia, 21 Jul. 2011. Web. 8

   Aug. 2011.
You can also read