Astronomy Final Exam: Chapters 3 & 4 Flashcards

1
Q

What are the Moon phases?

A

New Moon, Waxing Crescent, First Quarter, Waxing Gibbous, Full Moon, Waning Gibbous, Third Quarter, and Waning Crescent

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2
Q

How long does it take for the Moon to complete its synodic cycle?

A

29.5 days

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3
Q

How long does it take for the Moon to complete its sidereal cycle?

A

27.3 days

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4
Q

Is the Moon larger on the horizon?

A

No, this is an illusion

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5
Q

When do lunar eclipses occur?

A

Only occur at full moon if the Moon’s path carries it through the shadow of Earth, sunlight is blocked, & the Moon gives temporary dim

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6
Q

When do solar eclipses occur?

A

When the Moon moves between Earth & the Sun w/ the Moon being the same angular diameter as the Sun

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7
Q

What is the umbra?

A

The region of total shadow w/ no sunlight (3x longer than the distance from earth to the Moon)

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8
Q

What is the penumbra?

A

The region of partial shadow & partial sunlight

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9
Q

What is a total lunar eclipse?

A

The Moon is COMPLETELY hidden behind Earth from the Sun causing a red glow of the Moon (Earth’s sunrise / sunset)

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10
Q

What is a partial lunar eclipse?

A

When the Moon does not pass through the center of the umbra of Earth’s shadow

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11
Q

What is a total solar eclipse?

A

The Moon covers the disk of the Sun completely

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12
Q

What is a partial solar eclipse?

A

The Moon covers only part of the Sun

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13
Q

Glow of the lunar eclipse is due to what?

A

The red tinted Moon is illuminated by some sunlight that is reflected (bent) through Earth’s atmosphere

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14
Q

What are elliptical orbits?

A

Oval-shaped path, like a slightly elongated circle

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15
Q

What is the Corona?

A

The part of the Sun visible during solar eclipses

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16
Q

What are Kepler’s Laws?

A

1.) Orbits are elliptical, with focal points of a star
2.) Orbits sweep out equal areas in equal times
3.) Square of a period equals the cube of a semimajor axis (Pr^2=aau^3)

17
Q

What are ellipses?

A

A figure that can be drawn around 2 points, focis, in such a way that the distance from one focus to any point on the ellipse and back to the other focus equals a constant (the semi-major axis is half the longest distance)

18
Q

What are eccentricities?

A

Half the distance between foci divided by the semimajor axis (close to 0=circular and 1=elliptical)

19
Q

What was Brahe’s contribution?

A

-No direct contribution
-Value of his work lies in observational data & Rudolphines Tables

20
Q

What was Galileo’s contribution?

A

-Observed Venus orbiting the Sun through phases that supported the Copernicus Model
-Use of the telescope = made observational data to make the book “Sidereus Nuncis” (The Sidereal Messenger)