Solar System - Unit 2 Test Flashcards

1
Q

Briefly outline the catastrophic theory to explain the formation of the solar system

A

accidental catastrophes such as stellar near-collisions:

a rotating nebula underwent gravitational collapse into a star with an accretion disk, from which planets condensed or formed by coagulation of dust particles into increasingly larger bodies

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2
Q

Briefly outline the non-catastrophic theory to explain the formation of the solar system

A

natural, non-catastrophic events such as nebular condensation:

proposed by Immanuel Kant (1755) and expanded by Pierre LaPlace (1796).

A large, slowly rotating solar nebula contracted due to gravitational attraction, as it contracted, it sped up (conservation of angular momentum). When the centripetal force on the outer rotating edge exceeded gravitational attraction, a ring of gaseous matter split off, matter eventually coalesced into a planet. The process repeated itself, making concentric rings all of which formed planets. The central core formed the sun and satellites are miniature recurrences of the larger phenomenon.

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3
Q

Briefly describe the Medieval system of the universe.

A

In this geocentric (earth-centered) model, the earth was the motionless center of the universe, with the rest of the universe revolving around it in spheres.

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4
Q

Briefly describe how Ptolemy explained the motion of the planets.

A

Ptolemy used epicycles to explain the retrograde motions of planets. Epicycles Explain Retrograde Motion. As a planet moves around on its epicycle, the center of the epicycle (called the deferent) moves around the Earth. When its motion brings it inside the different circle, the planet undergoes retrograde motion.

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5
Q

Why was the heliocentric model of the solar system rejected?

A

Planets do not move in exact circles around the Sun, they move in oval paths called ellipses

If the Earth is rotating about its axis, and orbiting around the Sun, then the Earth must be in motion

The Church disapproved of this theory because the Holy Scriptures state that the Earth is at the center, not the Sun.

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6
Q

What was Copernicus’ model of the solar system?

A

proposed a heliocentric system, that the planets orbit around the Sun; that Earth is a planet which, besides orbiting the Sun annually, also turns once daily on its own axis; and that very slow changes in the direction of this axis account for the precession of the equinoxes.

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7
Q

Why is Newton’s Universal Law of Gravitation so significant?

A

one of the most important and fundamental laws in classical physics as it explains the movement of objects as a result of an “invisible force”

simple equation, but devastatingly effective: plug in the numbers and you can predict the positions of all the planets, moons and comets you might ever want to watch, anywhere in the solar system and beyond. And it allowed us to add to those celestial bodies too, heralding the space age.

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8
Q

State Kepler’s three laws of motion

A
  1. planet’s distance from the sun will change throughout its orbit
  2. speed of a planet in its orbit is not constant
  3. planet’s period can be calculated if it’s distance to the sun is known, and vice versa
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9
Q

State how Kepler’s three laws of motion have significance for space travel.

A

Describe how planetary bodies orbit the Sun. They describe how (1) planets move in elliptical orbits with the Sun as a focus, (2) a planet covers the same area of space in the same amount of time no matter where it is in its orbit, and (3) a planet’s orbital period is proportional to the size of its orbit (its semi-major axis).

show the effects of gravity on orbits. They apply to any object that orbits another: planets orbiting the Sun, moons orbiting a planet, spacecraft orbiting Earth.

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10
Q

What was the nature of the raw material of the planets?

A

About 4.6 billion years ago our solar system formed from a cloud of gas and dust which slowly contracted under the mutual gravity of all of its particles. The cloud was made largely of hydrogen (H) with some helium (He)

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11
Q

What is the Kuiper belt?

A

a circumstellar disc in the outer Solar System, extending from the orbit of Neptune at 30 astronomical units (AU) to approximately 50 AU from the Sun

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12
Q

What is the Oort Cloud?

A

Is a spherical shell surrounding everything in our solar system, made up of icy pieces of space debris

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13
Q

What 3 rules define a planet?

A

It must orbit a star (in our cosmic neighborhood, the Sun). It must be big enough to have enough gravity to force it into a spherical shape. It must be big enough that its gravity cleared away any other objects of a similar size near its orbit around the Sun.

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14
Q

Why was Pluto “demoted” to being a dwarf planet?

A

Pluto is now classified as a dwarf planet because, while it is large enough to have become spherical, it is not big enough to exert its orbital dominance and clear the neighborhood surrounding its orbit.

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15
Q

Name the two spherical asteroids or dwarf planets.

A

Spherical asteroids: (3) Juno and (48) Doris

Dwarf planets: Pluto, Ceres, Eris

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16
Q

Why did the church leadership seek to silence Galileo?

A

His ideas went against their beliefs, that the Earth was the center of the universe and he agreed with ideas of Copernicus.

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17
Q

What is a light year? How would you calculate it?

A

A light-year is the distance light travels in one year. How far is that? Multiply the number of seconds in one year by the number of miles or kilometers that light travels in one second, and there you have it: one light-year. It’s about 5.9 trillion miles (9.5 trillion km).

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18
Q

Describe our Sun in detail.

A

The Sun is a yellow dwarf star, a hot ball of glowing gasses at the heart of our solar system. Its gravity holds everything from the biggest planets to tiny debris in its orbit
Our Sun is a 4.5 billion-year-old star – a hot glowing ball of hydrogen and helium at the center of our solar system. The Sun is about 93 million miles (150 million kilometers) from Earth, and without its energy, life as we know it could not exist here on our home planet.
The Sun’s activity, from its powerful eruptions to the steady stream of charged particles it sends out, influences the nature of space throughout the solar system.

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19
Q

What is the purpose of the Parker Solar Probe?

A

swoop within about 4 million miles (6.5 million kilometers) of the Sun’s surface to trace the flow of energy, to study the heating of the solar corona, and to explore what accelerates the solar wind.

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20
Q

List the planets in order starting closest to the sun.

A

Mercury, Venus, Earth, Mars, Jupiter, Saturn, Uranus, Neptune, Pluto(?)

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21
Q

Provide a few details of each planet,

A

Mercury: the smallest and fastest planet in the solar system
Venus: extremely hot, Venus is unusual because it spins in the opposite direction of Earth and most other planets. It also has a very slow rotation making its day longer than its year.
Earth: only astronomical object known to harbor life
Mars: huge dust storms which last for months and can cover the entire planet.
Jupiter: gas giant, made up almost entirely of hydrogen and helium
Saturn: bright, beautiful rings that circle its equator.
Uranus: equator is nearly at a right angle to its orbit
Neptune: dark, cold, and very windy.

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22
Q

Could we live on any other planets? Why, or why not?

A

Living beings need the atmosphere to be of a specific composition, with oxygen to breathe and live, the atmosphere and the plants provide them with this gas. The temperature of the planet matters a lot too, living beings would cease to exist if the temperature on the planet was too high or too low for them to handle.

Among the stunning variety of worlds in our solar system, only Earth is known to host life. But other moons and planets show signs of potential habitability.

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23
Q

Why is Venus considered Earth’s twin?

A

Venus is often called “Earth’s twin” because they’re similar in size and structure, but Venus has extreme surface heat and a dense, toxic atmosphere.

24
Q

What is Earth made of?

A

Our home planet Earth is a rocky, terrestrial planet. It has a solid and active surface with mountains, valleys, canyons, plains and so much more. Earth is special because it is an ocean planet. Water covers 70% of Earth’s surface.

Iron, Oxygen, Silicon, Magnesium, Sulfur, Nickel, Calcium and Aluminum

25
Q

Why is it necessary to use two different scales in Grade 9 for the size of the planets and the distance of the planets from the sun?

A

Distance and sizes in the solar system are difficult to visualize because the numbers are so large. In making a scale model, you need to divide the actual figure by any standard number to make a scaling factor.

Our Solar System is huge and the distances between the planets are difficult to comprehend…To get a better visualization of the scale of our solar system

26
Q

What do you think the two craters would look like ten million years in the future?

A

Lunar crater will change very little; Earth crater will be highly eroded or erased

27
Q

How do you think an ocean impact would differ from an impact on land?

A

Ocean impacts could produce huge tsunamis that would flood coastlines across the globe. Land impacts would result in a crater, and huge amounts of rock materials would enter the atmosphere

28
Q

The acceleration of gravity (g) on Earth is 9.8 meters/sec2, but on the Moon, it is only 1.6 meters/sec2. How might this relate to the sizes of craters produced by impacts with identical amounts of kinetic energy on the two bodies?

A

Earth’s higher g requires more energy for lifting materials from its surface to excavate a crater. Just as an astronaut can jump more easily on the moon, impact energy lifts material off the moon’s surface more easily

29
Q

How does the kinetic energy of a 1000 m diameter iron asteroid traveling at 17 km/sec compare to a similar one traveling at 34 km/sec?

A

Kinetic energy increases by a factor of four when the speed is doubled.

30
Q

How old is the Sun? How did it form? How much of the Solar System’s mass is in the Sun?

A

The Sun formed about 4.6 billion years ago in a giant, spinning cloud of gas and dust called the solar nebula. As the nebula collapsed under its own gravity, it spun faster and flattened into a disk.

Most of the nebula’s material was pulled toward the center to form our Sun, which accounts for 99.8% of our solar system’s mass.

31
Q

What is the difference between the far side of the Moon and the dark side of the Moon?

A

The far side has far fewer ‘maria’, which are large dark patches caused by ancient volcanic flows. Instead it is much more densely covered with craters compared to the near side.

The ‘dark side’ of the Moon refers to the hemisphere of the Moon that is facing away from the Earth.

32
Q

Name and describe the function of each layer of the Sun.

A

Inner layers:

  • Core (energy via thermonuclear reactions),
  • Radioactive zone (energy moving slowly outwards),
  • and convection zone (energy moves toward surface causing convection currents)

Outer layers:

  • Photosphere (deepest layer),
  • chromosphere (hotter further away), transition region (extremely narrow layer that divides the Chromosphere from the Corona, temperatures rise tremendously),
  • and Corona (outermost atmosphere layer - In spite of its high temperature, the corona yields relatively little heat, because of its low density)
33
Q

What are the essentials that Earth has for humans to survive on it?

A

Strong magnetic field shielding from UV and harsh solar rays
Abundance of land and water
Moon steadies our climate
viable temperatures
Stable rotation
Ozone layer and atmosphere
Isolation (not pulled by a large galaxy body’s gravity)
Long lived sun providing just the right heat

34
Q

What are the important considerations when asked about “is there life on other planets”? What would life be like?

A

The standard definition for a habitable planet is one that can sustain life for a significant period of time. As far as researchers know, this requires a planet to have liquid water. To detect this water from space, it must be on the planet’s surface.

While the concept of life resembling human life on other planets may be possible as far as other planets in the universe it is certainly not a possibility on the planets that we have recognized so far in our own solar system

35
Q

Why is it important to study planets and other aspects of our solar system?

A

help scientists answer questions about its formation, how it reached its current diverse state, how life evolved on Earth and possibly elsewhere in the solar system, and what characteristics of the solar system lead to the origins of life.

36
Q

What are the 4 theories for the origin of the Moon?

A

Fission Theory, Capture Theory, Co-Accretion/Condensation Theory, and Giant Impact Theory

37
Q

Describe Fission Theory

A

In the 1800s, George Darwin suggested that the moon looked so similar to the Earth because at one point in Earth’s history, Earth might have been spinning so fast that part of our planet spun off into space but was kept tethered by Earth’s gravity.

38
Q

Describe Capture Theory

A

The moon originated elsewhere in the Milky Way, completely independent of Earth. Then, while traveling past Earth, the moon got trapped in our planet’s gravity.

39
Q

Co-Accretion/Condensation Theory

A

the moon and the Earth formed together while orbiting a black hole.

40
Q

Giant Impact Theory

A

The reigning theory is that a Mars-sized object impacted with a very young, still-forming Earth about 4.5 billion years ago. Does a better job than others of explaining the similarities in chemical compositions of the Earth and the moon, however it doesn’t explain why the moon and the Earth are chemically identical.

41
Q

Moon’s physical characteristics

A

The Moon is a spherical rocky body, probably with a small metallic core, revolving around Earth in a slightly eccentric orbit

No atmospheric shield to protect the surface so bodies have struck and cratered the Moon. This formed a debris layer, or regolith, consisting of rock fragments of all sizes down to the finest dust. Lots of large impacts from lava floods.

The Moon displays four main phases: new, first quarter, full, and last quarter.

42
Q

What is the difference between solar and lunar eclipses?

A

Solar eclipses occur when the Moon passes between Earth and the Sun, leaving a moving region of shadow on Earth’s surface. Lunar eclipses occur when Earth passes between the Sun and the Moon, casting a shadow on the Moon.

43
Q

Define umbra and penumbra.

A

The umbra is a total shadow.

The penumbra is a partial shadow

44
Q

TNOs

A

are very remote and faint objects.

45
Q

Comets

A

cosmic snowballs of frozen gasses, rock, and dust that orbit the Sun (produces visible tail).

46
Q

Asteroids

A

solid, rocklike, irregular masses mostly less than 1 km in length

47
Q

Meteors VS Meteorites VS Meteoroid

A

Meteors: enters Earth’s atmosphere and burns up
Meteorites: rock doesn’t burn up entirely and instead crash into the surface of the earth
Meteoroids: rocks floating around in space

48
Q

What is the composition of Meteorites?

A

Stony meteorites are rocks, mainly composed of silicate minerals; iron meteorites that are largely composed of metallic iron-nickel; and, stony-iron meteorites that contain large amounts of both metallic and rocky material.

49
Q

Solar wind

A

stream of charged particles released from the upper atmosphere of the sun, aka the corona.

50
Q

Proper names of Earth’s northern/southern auroras? Cause of auroras?

A

Aurora borealis and aurora australis.

Magnetic storms cause heightened displays, electrically charged particles from space entering earth’s upper atmosphere at high speed.

51
Q

Regolith

A

blanket of unconsolidated, loose, heterogeneous superficial deposits covering solid rock. It includes dust, broken rock

52
Q

Maria

A

large, dark, basaltic plains on Earth’s Moon, formed by ancient asteroid impacts

53
Q

pros/cons to space exploration?

A

Pros:

  • save humanity?
  • space industry jobs
  • learning more about universe
  • need artificial satellites
  • scientific advancement

Cons:

  • money could be better spent combatting climate change/issues on earth
  • need to clean space debris before we can start doing more trips
  • dangerous and alot of air pollution
  • waste production
  • rocket/probes could fail
54
Q

What space exploration spin-off technologies have impacted your life.

A
  • memory foam, scratch resistant glasses, gps, water filtration, wireless headsets, etc
55
Q

Do you think NASA’s budget should be increased or decreased? Why?

A

For: NASA funding helps small businesses research new ideas and develop innovative aeronautics, human exploration, science, and space technology solutions. Our partnerships fuel growth in industries that will define the future, such as artificial intelligence and advanced manufacturing.

Against: Space Exploration is a waste of resources. Instead of decreasing resources by space travel and such, we must deal with problems on Earth first. Why bother spending all this money on exploring space when we could be helping our own planet that us humans live on.