The Moon and Planets; Small Bodies in the Solar System Flashcards

1
Q

Describe the causes and effects of the atmospheric greenhouse effect and global warming

A

Sunlight heats the ground (which emits infrared radiation). Certain molecules absorb the radiation so the Earth doesn’t cool off because it can’t escape. Water vapor and CO2 block the infrared radiation because they’re greenhouse gases. Humans add CO2 to the atmosphere= warmer temperature= Global Warming

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
2
Q

Describe the impact of human activity on our planet’s atmosphere and ecology

A

Global Warming

  • Climate Change
  • Melting icecaps
  • Rising sea levels
How well did you know this?
1
Not at all
2
3
4
5
Perfectly
3
Q

Explain the scarcity of impact craters on Earth compared with other planets and moons

A

Earth was heavily impacted by craters just as much as the Moon. Craters destroyed by active geology. Plate tectonics renews the crust. Objects burn up in the Earth’s atmosphere. Erosion

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
4
Q

Describe the evidence for recent impacts on Earth

A

1) Tunguska River in Siberia but no craters (if it penetrates the Earth it would be classified as a crater) because it only damaged the surface
2) Arizona called the Meteor Crater

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
5
Q

Detail how a massive impact changed the conditions for life on Earth, leading to the extinction of the dinosaurs

A

Mass extinction: more than half of the species on our planet died out
Chicxulub: crater that killed the dinosaurs. Airborne material blocked out sunlight. Other results such as the fires and acidic rains led to the extinction of the dinosaurs

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
6
Q

Discuss what has been learned from both manned and robotic lunar exploration

A

Manned- terrestrial planets

Robotic- (terrestrial and) jovian planets

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
7
Q

Explain the process of impact crater formation

A

The projectile penetrates 2-3x its own diameter before stopping; energy as a shock wave and heat
Crater size is usually 10-15x greater the diameter of the projectile

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
8
Q

Characterize the orbit of Mercury around the Sun

A

Highest average orbital speed

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
9
Q

Describe Mercury’s structure and composition

A

The smallest terrestrial planet and planet overall
Greater density than the Moon= made up of 2 very different elements (mass: up to 60% iron-nickel, the rest being silicates)
Weak magnetic field (part of the core is liquid to create the field)

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
10
Q

Explain why it’s difficult to learn about Venus from Earth-based observation alone

A

Surface is not visible b/c of clouds

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
11
Q

Compare the basic physical properties of Earth, Mars, and Venus, including their orbits

A

All about the same size

All terrestrial planets- mostly solid

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
12
Q

Provide an overview of the composition of the giant planets

A

Material: gas (mostly hydrogen and helium), ice, rock (less abundant than ices)
Gas giants- Jupiter and Saturn
Ice giants- Uranus and Neptune (interiors contain more ice)

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
13
Q

Describe typical orbits of asteroids

A

Ellipse oribit like all the planets. Some are in the KB (outside of the solar systeml has the comets, asteroids, and other small bodies of ice adn rock)

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
14
Q

Characterize the general physical appearance of comets

A

Comet: small chunk of icy material that develops an atmosphere as it approaches the Sun (has a very faint nebulous tail). Not spectacular; very faint. Appear at unpredictable times. Visible for a couple weeks to months

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
15
Q

Explain what a meteor is and why it is visible in the night sky

A

What: a small piece of solid matter that enters Earth’s atmosphere and burns up, popularly called a shooting star because it is seen as a small flash of light. a small rocky or metallic body in outer space.

Why: It’s heating up and it’s getting hot as it’s traveling through the air.

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
16
Q

Describe the origins of meteor showers

A

Ash, dust, debris from the comets/rock/asteroids. Falling fast which makes it appear on fire and glowing like.

Many meteors appearing to radiate from one point in the sky; produced when Earth passes
through a cometary dust stream.

A sudden burst of meteor activity usually lasts several hours. Often named by the constellation from where the radiant is located

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
17
Q

Explain how the study of meteorites informs our understanding of the age of the solar system

A

Includes oldest and most primitive material

Classifications of meteorites: iron, stones, and stony-irons (obvious which type they fall into)

18
Q

Describe the motion, chemical, and age constraints that must be met by any theory of solar system formation

A

Motion constraints: most planets rotate in the same direction as they revolve. Most moons orbit counterclockwise. Besides comets and other TNOs motion is defined by a disk or frisbee shape. Exceptions include the retrograde rotation of Venus

Chemical constraints: Jupiter and Saturn have the same compositions (mostly hydrogen and helium). Comets in the Oort cloud and TNOs in the Kuiper belt are icy, asteroids are rocky w/ dark, carbon-rich material. Temperature sequence with planets’ position to the Sun. Exception w/ water on Earth and Mars.

Age constraints: radioactive dating. Age of building blocks= age of planetary system

19
Q

Summarize the physical and chemical changes during the solar nebula stage of solar system formation

A

The solar system formed about 4.5 B years ago. Rotating cloud of vapor and dust collapsed under its own gravity, making the material fall towards the center and become more hot and concentrated. Solar nebula began to rotate faster due to angular momentum. Faster materials collapsed into a disk to revolve around the center, which explains the motions of the solar system. When gravitational energy faded tha nebula cooled, but the center formed a star where it maintained its own energy. Turbulent motions and magnetic fields drained its angular momentum and therefore its spin. Some material fell into the growing star and the disk stabilized. Disk cooling produced compounds (liquids and solids) from gases. First solid materials were metals and rock-forming silicates. Temperature sequence (cool temp= oxygen could combine w/ hydrogen to form water= ice)

20
Q

Explain the formation process of the terrestrial and giant planets

A

Terrestrial: Grains condensed to form planetesimals
Accretion: when planetesimals are large enough to attract their neighbors gravitationally and grow in the process
Protoplanets: not quite ready for primetime planets
Planetesimals accelerate to combine with the protoplanet, heating the protoplanet
Planetary differentiation: heavier materials sink to the bottom and lighter materials float to the top

Giant: Protoplanets attracted gas. Heated by contraction, but were too small to raise core temperatures. Gradually cooled. Less gas was captured by Uranus and Neptune which is why they have icy and rocky cores.

21
Q

Describe pseudoscience and give some examples

A

Pseudoscience is an idea of different methods and concepts that falsely use science as validation of its effectiveness

Examples: astrology, numerology, hypnosis

22
Q

Explain what scientists mean by a hypothesis, theory, and law

A

Hypothesis: an explanation that can be tested over and over again. They explain the “how”
Theory: an explanation of a phenomenon supported by facts. Theories start out as hypotheses. They explain the “why”. Cannot turn into a law
Law: principles that can be used to predict processes in the natural world. They explain the “what”

All based on observations

23
Q

Explain why science poses no threat to religion and how many scientists can be – and are – very religious as well

A

Science and religion have coexisted for a while. About 40% of scientists are religious. Only a very small percentage of religious people are “anti-science”.

24
Q

Explain the northern lights

A

The direction of the solar wind is changed by the Earth’s magnetic field and is funneled into the North and South poles. The solar wind molecules crash through the atmosphere and excite the electron molecules. These electrons move up (absorb light) and down energy levels to emit light, which produce the lights we see at the North pole.

25
Q

Where are most of the asteroids in our solar system?

A

Between Mars and Jupiter; the asteroid belt

26
Q

Kuiper Belt

A

a disk of debris at the edge of our solar system; beyond Neptune

27
Q

What kind of object is Pluto?

A

Kuiper belt object

28
Q

Oort cloud

A

sphere of widely spaced comets; the large spherical region around the Sun from which most “new” comets come; a reservoir of
objects with aphelia at about 50,000 AU

29
Q

Describe Venus’ atmophere

A

Most of the atmosphere is CO2. It’s the hottest planet because of the greenhouse effect, which means it has few craters. It spins backwards.

30
Q

What is the “Runaway Greenhouse” effect?

A

The greenhouse effect on Earth worsens to the point it looks like Venus

31
Q

Why does Io have volcanic activity?

A

As Io revolves around Jupiter it’s closeness determines its volcanic activity. As Io gets closer to Jupiter, Jupiter’s tides evoke more heat from Io, but as Io gets farther away there is less volcanic activity.

32
Q

Describe the criteria of a planet

A

1) Orbits a star
2) Approx. round
3) Not a star or moon
4) Nothing big in its orbit

33
Q

Describe a comet

A

a “dirty snowball”; 2 tails: gas and dust. The solar wind blows gases out. The closer to the Sun the longer the tail. The position of the comet in its orbit depends on where it is in its tail development.

34
Q

Asteroid

A

a stony or metallic object orbiting the Sun that is smaller than a major planet but that shows no
evidence of an atmosphere or of other types of activity associated with comets

35
Q

Near-Earth Asteroid (NEA)

A

an Earth-approaching asteroid, one whose orbit could bring it on a collision course
with our planet

36
Q

Near-Earth object

A

a comet or asteroid whose path intersects the orbit of Earth

37
Q

Nucleus (of a comet)

A

the solid chunk of ice and dust in the head of a comet

38
Q

Exoplanet

A

a planet orbiting a star other than our Sun

39
Q

Iron meteroite

A

a meteorite composed primarily of iron and nickel

40
Q

Stony meteorite

A

a meteorite composed mostly of stony material, either primitive or differentiated

41
Q

Stony-iron meteorite

A

a type of differentiated meteorite that is a blend of nickel-iron and silicate materials