Moon phases, eclipses, Universal Law of Gravitation, Galaxies, Star Systems, and the Sun Test Review

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34 Terms

1

What causes the phases of the Moon?

The Moon’s orbit around Earth and the reflection of sunlight

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2

Why do solar eclipses not occur every month?

The Moon’s orbit is tilted relative to Earth’s orbit

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3

How does a lunar eclipse differ from a solar eclipse?

A lunar eclipse occurs when Earth is between the Sun and Moon; a solar eclipse occurs when the Moon is between the Sun and Earth

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4

What is the difference between the umbra and penumbra?

The umbra is the darkest part of a shadow, while the penumbra is the lighter outer region.

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5

What happens to the gravitational force between two objects if their distance doubles?

It decreases to one-fourth of its original strength.

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6

What is the equation for Newton’s Universal Law of Gravitation?

F = G(m1m2/r^2)

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7

What is the primary source of the Sun’s energy?

Nuclear fusion in the Sun’s core.

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8

What are the effects of the solar wind on Earth?

Causes auroras and can disrupt electronics and communications

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9

Why does the Sun’s corona appear hotter than its surface?

Magnetic fields accelerate particles in the corona.

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10

How does a barred spiral galaxy differ from a regular spiral galaxy?

It has a bar-like structure at its center.

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11

What type of galaxy is the Milky Way?

 A barred spiral galaxy.

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12

How does an open star cluster differ from a globular cluster?

Open clusters are younger and loosely bound; globular clusters are older and densely packed

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13

What is the significance of Hubble’s Tuning Fork diagram?

It classifies galaxies based on their shape.

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14

What are coronal mass ejections (CMEs) and their effects on Earth?

Large bursts of solar particles that can disrupt Earth's magnetic field.

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15

What phase must the Moon be in for a solar eclipse to occur?

New Moon

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16

What phase must the Moon be in for a lunar eclipse to occur?

Full Moon

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17

What is the role of gravity in planetary orbits?

It keeps planets in orbit around the Sun

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18

What will happen to the Sun after it exhausts its nuclear fuel?

 It will become a white dwarf.

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19

What are auroras, and how do they form?

Light displays caused by solar wind interacting with Earth's atmosphere.

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20

What is a binary star system?

 A system with two stars orbiting a common center

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21

Phases of the Moon

The different appearances of the Moon as seen from Earth, caused by the varying angles of sunlight reflecting off its surface as it orbits Earth

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22

Umbra

  1. The central, darkest part of a shadow, where all direct light is blocked; during an eclipse, this is where totality occurs.

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23

Penumbra

The outer, lighter part of a shadow where only some of the light is blocked, causing partial eclipses

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24

Solar Eclipse

 An astronomical event that occurs when the Moon moves between the Earth and the Sun, temporarily blocking sunlight and casting a shadow on Earth.

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25

Lunar Eclipse

An event that happens when Earth moves between the Sun and the Moon, causing Earth's shadow to be cast on the Moon, making it appear darker or reddish

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26

Gravity

The attractive force exerted between two masses; it governs the motion of celestial bodies and keeps planets in orbit around stars.

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27

Newton’s Universal Law of Gravitation

A scientific law stating that every mass attracts every other mass with a force proportional to their masses and inversely proportional to the square of their distance.

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28

Orbital Path

The continuous trajectory that an object follows around another celestial body due to gravitational forces, such as the Moon orbiting Earth

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29

Core (of the Sun)

The innermost region of the Sun where nuclear fusion occurs, generating immense energy that powers the Sun and emits light and heat

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30

Photosphere

The outermost visible layer of the Sun’s surface that emits the light we see; it has a temperature of approximately 5,500°C (9,932°F)

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31

Corona

The Sun’s outermost atmospheric layer, extending millions of kilometers into space, visible as a halo during a total solar eclipse.

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32

Solar Wind

A continuous flow of charged particles (plasma) released from the Sun’s corona, which can influence Earth's magnetic field and cause auroras.

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33

Coronal Mass Ejection (CME)

A powerful eruption of plasma and magnetic fields from the Sun’s corona, capable of causing geomagnetic storms on Earth.

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34

Solar Prominence

A large, bright, loop-shaped structure of plasma that extends from the Sun’s surface, often associated with sunspot regions.

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