astronomy: mars
24.6 hours
length of day on mars
erosion
overall, _______ is about 100x slower than on earth, but still faster than on the moon or venus
borealis basin
the giant ________ _____ around the martian north pole could be the result of one of the largest known impacts in the solar system
surface gravity
the height of these volcanoes is a direct consequence of the low _______ _______ on mars
tharsis bulge
the major geological feature of mars is the _______ _____. it lies at the equator and rises about 10 km higher than the rest of the surface
seasons
the most obvious features from earth are the bright polar caps which grow and shrink depending on the _______
valles marineris
the most prominent feature of the tharsis bulge is the great "canyon" known as ______ _________ (the mariner valley)
volcanic plains
the northern hemisphere is made up largely of rolling ________ _____similar to the lunar maria
lava
the northern hemisphere must have been lowered in elevation and then flooded with ____.
southern summer
the only difference is the _________ _______
smaller, brighter
the residual caps are _______ and _________ than the seasonal caps
highlands
the southern hemisphere consists of heavily cratered _________
crustal forces
the valles marineris is believed to have been created by _______ ______, not from erosion due to flowing water. it is 4000 km long and can reach depths of 7 km at its deepest places. it runs nearly a 5th of the way around the planet. it can never be seen from earth.
outflow channels
the volcanism and bombardment by space stuff melted that what frozen water was left causing those ________ ________
ocean
the whole northern lowlands may have been a huge _____
warmer
their temperatures never get ______ thank 150 K (-120 C/ -184 F)
high winds
there are frequent dust storms, with ____ _____
magnetic field
there is no ________ _____, so the core is probably not metallic, not liquid, or neither liquid nor metallic
active
there is no direct evidence that the volcanoes are ______
eruptions
they are much larger than their counterparts on either the moon or earth and a result of __________ that included a lot of material
olympus mons
three volcanoes are located on tharsis bulge, the largest of which is the _______ ____. it measures over 700 km in diameter (about the size of texas)
chryse planitia, isidis planitia
to the east of tharsis is ______ _______ (plains of gold) and to its west a region called ______ ________ (plains of isis)
water
although dry and desolate now, there is a lot of evidence to support that mars may have _____ on its surface in its past
reflective
as water ice froze, mars became more and more ___________ and its atmosphere thinner and thinner, freezing more and more water and eventually carbon dioxide as well
24.0 degrees
axial tilt of mars, very close to earth's 23.5 degrees
conjunction, opposition
because of mars' superior orbit (lying outside of earth's), it can appear to be: closer to the sun - ___________ opposite the sun - __________
composition of atmosphere
95.3% co2 2.7% n2 1.6% ar .13% o2 .07% co .03% h2o
great bombardment
its impact craters suggest that it formed very early in the martian history, probably during the _____ ___________
dry ice
the frozen caps are mostly frozen co2 (___ ___), not water like on earth
mars odyssey, mars express, mro
____ _______, ____ _______, and the ___ have all found direct evidence of large deposits of ice all over the planet
water ice
_____ ___ is permanently frozen. there is some water mixed in with this, but it is not the dominant presence.
runoff channels
______ ________ are extensive systems of interconnecting, twisting channels that seem to merge into larger, wider channels. they are very similar to how the river systems on earth look. generally found in the southern highlands
outflow channels
_______ ________ are probably the paths taken by huge volumes of water draining from the southern highlands into the northern plains. believed to be a result of a slightly more recent catastrophic flooding events. they are found only in equatorial regions and generally don't form the interconnecting networks of the runoff channels.
impactor
computer simulations show that it could be the result of huge (2000 km across) ________ that grazed the planet
3900 kg/m^3
density of mars, only slightly greater than the moon
hellas basin
diametrically opposite to tharsis, is ______ _____ which contains the lowest point on mars. it is an impact feature and lies over 6km below the average surface
increasing
during martian summer, the exposure to the sun causes co2 to evaporate into the atmosphere there by __________ atmospheric pressure
seasonal cap, residual cap
each cap is composed of two distinct parts: the ________ ___, which grows and shrinks each year the ________ ___, which remains permanently frozen
variation
for most of the year there is little day to day __________: the sun rises, heats up the surface, light winds blow, then the sun sets and it cools again
permafrost
for reasons unknown this water either became frozen as ___________ and in the caps or escaped into the atmosphere and then escaped into space
martian dust
from a distance it appears that ground too changes. we know now that it is just the _______ ____ blowing around making certain areas appear different
100 km
from behavior of the crust, it is estimated to be ____ __ thick
retrograde
from our vantage point, mars appears to travel in a great circle across the sky with period points of __________ motion
permafrost
geologists think that this fluidized ejecta crater indicates that a layer of __________, or water ice, lies just a few meters below that surface.
lake
hellas basin would be another candidate for a giant ____
plate tectonics
if we go with the idea of "continents", tharsis would be the only one however there is no evidence of _____ _________ on mars
viking
in the 70s ______ gave us some of our first images of the martian surface
plate motion
like with venus, none of the volcanoes are associated with _____ ______; they are shield volcanoes sitting atop a hot spot in the underlying mantle
thinner atmosphere
mars also undergoes seasonal change, but it is very different from earth given mars' eccentricity and _______ __________
opposition
mars appears the brightest in the night sky at __________ and especially if this occurs near the martian perihelion
volcanoes
mars contains the largest known ________ is the solar system
deimos, phobos
mars has two tiny moons: ______ (right, 16 x 10 km2) - was probably captured from the asteroid belt ______ (left, 28 x 20km2) - may have formed later, from material ejected from mars by a meteor strike
venus
mars is considerably fainter than _____ due to the fact that: it is twice as far from the sun as _____ it is much less reflective, only about 15% of the sun's light reflects off
fourth
mars is the ______ planet from the sun and is the outermost of the terrestrial planets
.093
mars is the second most eccentrical planet in the solar system with an e of ____
runaway greenhouse effect
mars may be victim of ________ ___________ ______ in the opposite sense of venus'
sunlight
mars' eccentricity results in a large variation of the amount of ________ striking the planet throughout its year
eccentric
mars' orbit is more ________than earths
6.4 x 10^23 kg
mass of mars
demos and phobos
moons of mars
mars global surveryor
more recently, the ____ _____ ________ has mapped out the martian surface to within an accuracy of a few meters
crust
most scientists agree that the southern region is mars' original _____
seismic
no ________ studies have been done
impact craters
on mars, as with venus, there is a lack of small ______ _______. this is most likely due to the thin atmosphere and seasons that move dust and debris around on mars.
3394 km
radius of mars
dust
strong surface winds here carry ____ high into the atmosphere that then get deposited all over the planet
warmer
summers in the south (around perihelion) are much _______ than summers in the north
gullies
surveyor missions since 2000 have reported numerous discoveries of small-scale "_______" in martian cliffs and crater walls that were apparently created by running water in the recent past
youngest
tharsis also appears to be less heavily cratered, suggesting that it is the ________ region on the planet
caldera
the ______ of the olympus mons measures 80 km across.
ejecta
the _______ around impact craters on mars look very different than of those on the moon
northern residual cap
the ________ ________ ___ is much larger and reach slightly warmer temperatures especially during northern winter
younger
the assumption is that the northern surface is _______ than southern (3 billion years old vs 4 billion years old)
co2
the atmosphere of mars is very thin and composed mainly of ___
1/150th
the atmospheric pressure is about _/_____ that of earths
4 billion
the best that scientists can guess is that _ _______ years ago mars had liquid water
carbon dioxide frost
the caps are composed predominantly of ______ _______ _____ - dry ice - and show seasonal variations
.37
the closest mars and earth come to each other is ___ au. the closest approach occurs about every 15 years, the last time being 9/28/03