Members of the Inner Planets - Monadnock Regional High School · 2018. 8. 18. · Mercury BASIC...
Transcript of Members of the Inner Planets - Monadnock Regional High School · 2018. 8. 18. · Mercury BASIC...
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Name: __________________________
Date: _________________
Pd: ________
M e m b e r s o f t h e I n n e r P l a n e t s o ___________________________
o ___________________________
o ___________________________
o ___________________________
The Terrestrial Planets Notes
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Mercury BASIC CHARACTERISTICS:
o Mass = 3.302x1023 kg (______________________) o Radius = 2,440 km (_______________________) o Albedo (_________________) = ________ (Earth = 0.39) o Averange _____________________ = __________________ o _________________________________________________________
KEY CONCEPTS:
1) Mercury has a __________________________________________ (_____________________________________________________) o Time between one noon and the next is ______________ o Sun is above the horizon for _________________ at a time
2) Mercury has ____________________________________ because
it is too hot o Daytime temperatures reach as high as ______________ o Night-time temperatures drop as low as ______________
3) Like the Moon, Mercury has ________________________ AND
____________________ o Mercury has _________, or cliffs, as much as 3 km high,
500 km long o They are probably the result of ________________________
4) Mercury has an _____________________________________
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VENUS BASIC CHARACTERISTICS:
o Mass = 4.868 x1024 kg (______________________) o Radius = 6,052 km (_______________________) o Albedo (Reflectivity) = ________ (Earth = 0.39) o Averange distance from the Sun = __________________ o Travel time from Earth ______________________________
KEY CONCEPTS:
1) Venus has ________________________________ (backwards!) o Orbital Period (Revolution) = _______________________ o Rotation period = _______________________ o On Venus, the time from noon to noon = ______________
2) The surface of Venus is hidden from us by _________________
_________________________________
3) The surface of Venus shows ______________________________ _________________________________ o More than _____________________________________
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4) The atmosphere of Venus is ________ because of a
____________________________________ o Venusian Atmosphere
• ____________ Carbon Dioxide (CO2) • ____________ Nitrogen (N2) • ____________ Sulfur Dioxide (SO2) • ________________________
o CO2 is a _____________________ (________________ in the
atmosphere) o Surface temperature = _________________________ Even
______________ than Mercury!
o Temperatures ________________________________________ thanks to the _________________________________
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MARS BASIC CHARACTERISTICS:
o Mass = 6.418 x1023 kg (______________________) o Radius = 3,377 km (_______________________) o Albedo = ________ (Earth = 0.39) o Average distance from the Sun = __________________ o Travel time from Earth ______________________________
KEY CONCEPTS:
1) Mars has ________________________________________________ o Orbital Period (____________________)= ______________ o Rotation Period = _______________________ o _____________________ of Mars is ____________ by _______ o Martian _________________ to Earth seasons (only longer)
2) Mars has a ______________________________________________ with little water vapor and few clouds o Scientists believe it was _____________________________
due to it’s ___________________________________________ o Low density atmosphere implies:
1) ______________________________ 2) ______________________________
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3) Mars has _________________________ and a ________________ ______________ but ______________________________________ o ____________________________________________________ o About ___________________________ or Poland (~600km) o Last eruption was about 300 million years ago
4) Mars has two small irregular moons, ____________________ and ______________________.
5) Robotic __________________________________________________
o Mars Exploration Rovers________________________________ - 2004 o Mars Pathfinder ____________________________ - 1997 o Mars Science Laboratory _______________________ - 2012
* Both the _______________________________________________________________