Astronomy: Chapter 2 Flashcards

1
Q

Describe the coordinate system of the celestial sphere.

A
  • Used to locate object, aim telescopes, and study the relationship of night sky to ancient culture.
  • an imaginary spear of a large radius surrounding Earth.
  • has Northern and Southern celestial poles, in which the sky appears to rotate westward.
  • if the earth did not rotate, we would not be able to find the celestial pole and equator because the poles and equators are located where the sky appears to rotate.
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2
Q

What is a constellation and how is it different from a star cluster?

A

Constellation: one of the stellar patterns identified by name, usually of mythological gods, people, animals, or objects. Also, the region of the sky containing that star pattern.

Star Cluster: stars that are bunched together.

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3
Q

Hipparchus method of measuring the brightness of stars.

A
  • Hipparchus came up with a method to determine the brightness of a star. He used a “magnitude scale”
  • Magnitude scale: the brightest stars were ranked as 1 and the dimmer stars were ranked as 6. Some stars are so bright they have extended them to negative numbers. it has also been extended for fainter stars.
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4
Q

What does a Foucault Pendulum demonstrate? How does it work? where does it work best? worst?

A

Demonstrates the earths rotation on its axis.

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5
Q

Precession

A
  • The slow change in orientation of the Earth’s axis of rotation. One cycle takes nearly 26,000 years.
  • a spinning top precesses in a slow circular motion around the perpendicular to the floor because its weight tends to make it fall over.
  • earth precesses around the perpendicular to its orbit because the gravity of the sun and moon tend to twist it “upright”
  • Precession causes the north celestial pole to drift among the stars
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6
Q

Why is it cold in the winter and hot in the summer?

A
  • This is due to the tilt of earth on its axis.
  • Summer Solstice: Earth’s northen hemisphere is inclined toward the sun, and sunlight shines almost straight down at northern latitudes.
  • winter solstice: Earth’s northern hemisphere is inclined away from the sun, and sunlight strikes the ground at an angle and spreads out.
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7
Q

Solar Day vs Sidereal Day

A

A solar day takes 24 hours, but a sidereal day takes 23 hours and 56 minutes because it takes 4 minutes to realize the rotation of the earth.

in the time it takes the earth to spin, the sun has moved about 1 degree in its journey around the earth. so a solar day (on average) 4 minutes longer than a sidereal day.

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8
Q

Do people from other cultures on Earth see the same stars, constellations, and asterisms that you see?

A

no

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9
Q

If earth did not rotate, could we define the celestial pole and celestial equator?

A

No, the poles and equator are located where the sky appears to rotate.

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10
Q

Name and sketch the eight phases of the moon in order, beginning with the new moon.

A

New Moon, Waxing Crecent, First quarter, Waxing Gibbous, Full moon, Waning Gibbous, Third Quarter, Waning Crecent.

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11
Q

How does the moon keep the same face toward the earth? doesn’t it rotate?

A

Because the same side of the moon faces Earth, and both Earth and the moon rotate together.

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12
Q

Solar Eclipse

A
  • Total Eclipse of the sun
  • During a solar eclipse, the moon is between the earth and the sun.
  • the moon blocks our view of the sun.
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13
Q

Lunar Eclipse

A
  • Total eclipse of the moon.
  • the earth is between the sun and the moon.
    the full moon darkens as the moon moves through the shadows of the earth.
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14
Q

Why can you never see a full moon overhead at sunset?

A

A full moon always rises at sunset and a full moon is always overhead at midnight.

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