ASTR 1210 (O'Connell) Study Guide 16
Crescent Mars during Viking 2 approach 1976.
Clouds trail downwind of volcano Ascraeus Mons.
Mars is the most intriguing planet. From Earth, it exhibits the
largest brightness variations of any planet and has the
most
distinctive color (red/pink). Telescopes have revealed it to be
the
most Earth-like planet, with a transparent atmosphere,
varied terrain, polar caps, and seasonal changes.
Although Mars is smaller than Earth, it has no oceans, so its
land
area is comparable to Earth's. Space missions have revealed fantastic
topography, including the largest canyon and the largest mountain in
the solar system.
Finally, for over 100 years, Mars has been the
favorite candidate
for another biosphere. Claims by some astronomers that there were
artificial
"canals" on Mars had tremendous impact on popular
culture.
The canals were optical illusions, but recent
evidence for possible fossil lifeforms and for abundant water on its
surface in the past finally have given real credence to speculations
about life on Mars. Consequently, Mars is now under intense scrutiny
by spacecraft for evidence of a favorable habitat (now or in the
past).
A. Mars: Introduction
Size: A small planet: 50% Diam(Earth); 10% Mass(Earth)
Orbit: Semi-major axis 1.5 AU. Orbital period 1.88 yr.
"Oppositions" occur every 2.1
years
- Mars' distance & brightness at opposition (closest approach to
Earth) vary significantly because of its large orbital ellipticity
(10%). See the diagram at the right; click for an enlargement.
- When brightest, Mars is a very conspicuous, red-pink object --
hence its association with the God of War. Mars can be brighter than
Jupiter.
Atmosphere: thin. Mass ~1% Earth's. Mainly CO
2;
some H
2O vapor.
Surface: easily visible since CO
2 is transparent. Has been
explored in ever increasing detail by Earth-bound telescopes and by
spacecraft, including orbiters, landers and rovers.
- Mars' red color is caused by iron oxide compounds such as
hematite on its surface. This is equivalent to rust(!). Other
conspicuous markings include white polar caps and large dark areas,
some appearing greenish to the eye in a telescope.
- Mars is distant enough even at opposition that telescopes on
Earth yield relatively poor resolution. This led to a long and
controversial history over whether or not there was evidence for
"canals" or other artificial features on its surface. (See
Section C below.)
- The image below was taken from Earth orbit by the Hubble Space Telescope and shows the
main kinds of features visible from Earth.
B. Major Spacecraft Missions to Mars
Mars has been the target of over
40
robotic spacecraft missions, many of which, especially the USSR's, failed
(wow! incompetence or
conspiracy??). Four types
have been undertaken:
flybys, orbiters, landers, rovers.
Successful missions have mapped nearly its entire surface and have
sampled its atmosphere and soil and even subsurface layers using
special techniques.
Important Earlier Missions:
- Mariner
Missions: 3 flybys, 1 orbiter, 1964-71; preliminary imaging
reconnaissance of Martian surface
- Viking
Missions: 2 orbiters/2 landers. 1976. Sampled soil and searched
for chemical signatures of lifeforms.
- Mars
Pathfinder: a lander with the first rover. Sampled soil and
rocks near landing site. 1997.
-
Mars Global Surveyor: orbiter. Mapped surface at high
resolution with a camera and the MOLA laser altimeter. 1998--2006.
- Mars
Exploration Rovers Mission: orbiter plus two landers and rovers
("Spirit" and "Opportunity"), placed on opposite sides of the planet
in areas thought to be associated with large water flows in the past. The
rovers traveled a combined distance of over 33 miles on Mars' surface.
2004-2018.
Current Missions:
- 2001 Mars
Odyssey: orbiter. Studying mineralogy, elemental abundances
(including hydrogen, a water tracer). 2001-- .
- Mars Express: first European mission to Mars. Lander
failed (2003), orbiter (2004-- ) studying surface features,
mineralogy, atmosphere. Carries a stereoscopic camera and the MARSIS
radar instrument for probing subsurface materials.
- Mars
Reconnaissance Orbiter: Entered Mars orbit in March 2006.
Instrumentation includes the HIRISE camera for high resolution (3 ft on
the Martian surface) imaging and experiments for mineral mapping and
subsurface analysis by radar.
- The Mars Science
Laboratory, successfully landed its "Curiosity" rover in August
2012 in
Gale Crater, a
large, ancient impact crater which contains an interior mountain of
sedimentary deposits.
- The Mars InSight Mission
successfully landed on Elysium Planitia in November 2018. InSight is
a non-rover mission intended to examine the deep interior of Mars
using seismometers.
- The Mars Perseverance
Mission made a successful landing in Jezero Crater on Mars on
February 18, 2021. The most ambitious rover mission yet, Perseverence
is intended to search for evidence of (microbial) life on Mars. It is
exploring the sediments of an ancient lake bed that might have been
life-bearing in the first billion years or so after Mars formed.
It will store soil samples in special containers that can be
retrieved and returned to Earth by the next NASA Mars mission.
C. Percival Lowell and Canals on Mars
"What goes on upon all those distant globes? Are they
worlds, or are they mere masses of matter? Are physical forces alone
at work there, or has evolution begotten something more complex,
something not unakin to what we know on Earth as life? It is in this
that lies the peculiar interest of Mars."
--- Percival Lowell (1895)
|
Astronomer
Percival
Lowell devoted his career and his observatory (ca. 1890-1915) to
the study of dark features on Mars' surface that he believed to be
artificial canals engineered by an advanced civilization for
survival on a desert planet. He made numerous sketches using a
medium-sized telescope (at left). An example of a Lowell sketch is at
right and shows the long, linear features he called canals. Another, much
more detailed, Lowell map can be
seen
here.
Lowell
was
not
the only astronomer claiming to have seen the canals. The visibility
of any such features is strongly affected by the blurring effects
("seeing"---see
Study Guide 14) of Earth's
atmosphere. The canal enthusiasts claimed to have seen the sharp,
straight-line features crossing the planet's face emerge during brief
moments of atmospheric stability. They believed they saw systematic
changes that implied the Martians were improving their canal system
and greening of the surface indicating vegetation spreading in the
springtime. However, many careful observers were never able to see
the canals at all.
Lowell's efforts to popularize the idea of civilizations on Mars (see
his article proclaiming
"Martians Build Two Immense Canals in Two Years") had a great
impact on the public imagination. They were the stimulus for H.
G. Wells' novel
War of the
Worlds, the archetypal story of an alien invasion, and a
tidal wave of subsequent science fiction and fantasy stories
(see
Study Guide 18).
A civilization on Mars as it might have been
envisioned by Lowell.
From cover art by Michael Whelan for an
edition of "The Martian Chronicles" by Ray
Bradbury.
But the canals
are
optical
illusions!, created by the tendency of the human brain to
link
threshold markings together. "Pattern recognition" by the eye-brain
system is an important survival adaptation for human beings: those who
could see the tiger lurking in the forest shadows survived longer than
those who could not. However, in many situations (e.g. at the
telescope or in sudden emergencies) it can produce misleading memories
of what was seen. The
canals were never photographed even with the
largest Earth-bound telescopes (see comparison below).
A photograph (left) and drawing of Mars made on the
same night.
Click for an
enlarged comparison of an HST image to classical drawings.
- Beginning in the 1960's, close-up images from spacecraft proved
there to be no artificial structures on Mars.
- The claimed "green" markings are likewise an optical
illusion, produced by the color contrast between reddish and
grey-brown areas.
The "canals" are an object lesson in dealing with marginal evidence,
a not uncommon situation in science:
There is a great temptation to overinterpret marginal data and
to try to force them to conform to preconceived ideas. This is a
major factor in many "pseudo-scientific" phenomena (see the discussion
of these in Guide 18.) Good scientists will
resist this. They will honestly assess the uncertainties in the
situation and will withhold judgement until the evidence improves.
It turns out that few of the
real topological features on
Mars -- such as the enormous mountains, canyons, and craters revealed
by spacecraft imaging, all larger than any comparable features
on Earth -- are even visible in Earth-based telescopes
despite their scale. Instead, the patterns conspicuous from Earth
are
large-scale differences in albedo (reflectivity) caused by
surface dust and mineral deposits. The pink/orange dust is very fine.
Winds carry it easily across the surface, causing continuous small
changes in appearance.
An example of the best maps of Mars produced by Earth-based telescopes
before the first spacecraft imaging was obtained in the 1960's is
shown here. It bears little
resemblance to modern topographic maps
produced by orbiting spacecraft -- and it also shows no evidence of
the multiple canals claimed by Lowell.
There
is good evidence for water and possibly primitive
lifeforms on Mars in the distant past (discussed below and in
Guide 17) -- but not for
civilizations.
Topographic charts of Mars, color-coded for altitude,
with
main features identified (from the MGS MOLA Altimiter)
D. Martian Topography
Mars features an
amazing landscape. Martian topography has been
surveyed by many spacecraft (see above), now reaching an accuracy
of about one meter.
ASTR
1210 Mars Images Page. For illustrations, click here or on
highlighted items below.
- The dual-hemisphere image above shows the main topographic
features of Mars.
- The image at right illustrates the red color, craters, mountains,
plains, and dust-laden atmosphere of Mars. Click for a larger
view.
- Impact Craters: are widely distributed with more in the
southern hemisphere, which is therefore older. Craters are weathered
and often partially dust-filled. The Hellas Basin is the largest impact crater.
- Volcanos: There are 5 large
"shield" volcanos plus a
number of smaller ones.
- First among these, Olympus
Mons is the largest mountain in the entire solar system
(85,000 ft altitude).
- All the volcanos are dormant now, but there is some
evidence for smooth, minor lava flows in the Tharsis region over the
past few 100 million years.
- Olympus Mons and the other volcanos in its vicinity are thought
to have originated from the upwelling of a warm mantle
plume, 3-4 billion years
ago
- The plume's effect was concentrated into a huge uplift region
(the "Tharsis bulge")
because there was minimal motion of the crust past the plume.
- This qualifies as proto-tectonic activity. But Mars' surface
is not broken into tectonic plates, and extensive mantle activity has been
dormant for most of the last billion years.
- So, neither Mars nor Venus have widespread tectonic plate
structures like those on Earth. Mars, however, has not
experienced a violent resurfacing episode like that 500 Myr ago on
Venus.
- Valles Marineris is
the largest canyon in solar system. It was not produced by
water (though some "tributary" canyons may have been). Instead, VM is
a surface rift, like
the African
Rift Valley, created by tearing of the rigid surface
layers during the Tharsis upwelling.
- Polar caps: the caps
in winter are a mixture of frozen CO2 and H2O.
They melt and refreeze with seasonal change. Water ice melts at a
higher temperature than CO2 ice, so any ice visible
between the two melting points must be water ice.
E. Evidence for Water on Mars
Click for illustrations.
There are no open bodies of water on Mars now, but there is extensive
evidence for the presence of frozen water at the poles and in the soil
and for liquid water on the surface in the past:
- Water ice has long been known to be present at the poles. There
is a trace of water vapor in the atmosphere [30 times smaller than on
Earth, in percentage, but much larger than on Venus]
- By mapping gamma-ray
emission, Mars Odyssey
(2001+) provided evidence for widespread deposition of
(frozen) water molecules in the
upper 1-meter of the surface, especially the poles.
- Layered terrain is
evidence for sedimentary rocks, deposited by lakes and oceans.
- Erosion channels are evidence of
massive floods at some time in the past.
The largest Martian flow channels
are much
larger than on Earth. They imply floods 100-10,000 times the
outflow of the Amazon River at some time in the past.
- Evidence for a huge ocean
basin in the northern lowlands.
- Radar evidence for water ice layers buried thousands of feet deep under
the Martian poles.
- Lander missions (7 to date, see Study
Guide 17) have found extensive evidence for water molecules bound
within Martian minerals. The
Phoenix lander (2008),
with a soil-sampling scoop, detected subsurface ice crystals; its
images of changing droplets are possible evidence for liquid (saline)
water. Data from
the Curiosity lander
(2013) indicate that the mean water content of soil minerals on Mars
is about 2%, or (if extracted) 2 pints of water per cubic foot of
soil.
- All the evidence points to large amounts of liquid water in
the past, perhaps one billion years ago. Water ice is widely
distributed in the soil and rocks now. It is likely that there are
large permafrost reservoirs of water under the surface. In the past,
these could have been melted by volcanic activity, inducing
widespread, possibly cyclic, floods.
- Independent sources of evidence concerning water are the
SNC meteorites (see Guide
17).
Discussion of Mars is continued on
Study Guide 17.
Reading for this lecture:
Study Guide 16
Bennett textbook, p. 206, Sec. 9.4.
Reading for next lecture:
Study Guide 17
Bennett textbook, p. 206, Sec. 9.4.
Web Links:
Last modified
March 2021 by rwo
"Red Mars" image copyright © 1997 by Calvin J. Hamilton. "Martian
Chronicles" cover art copyright © 1990 Michael Whelan. Text
copyright © 1998-2021 Robert W. O'Connell. All rights reserved.
These notes are intended for the private, noncommercial use of
students enrolled in Astronomy 1210 at the University of
Virginia.