The scale of things and the view from the earth Flashcards

1
Q

Who measured the circumference of the earth in 200BC

A

Eratosthenes

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2
Q

–1—- proposed a method to measure the distance to the Sun and the Moon in 280BC. Using how long it takes for the Moon to cross —2— shadow during —3–, he also tried to measure their sizes. He measured the —4— between the sun and the —5— or –6— quarter moon. Using these —7— and geometry, he calculated the —8– of the Earth-Sun distance and the —— - Moon distance.

A

1) Aristarchus
2)Earth’s
3)eclipses

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3
Q

From slide 9 picture, what is cos(theta) ?

A

Dm/Ds
Dm = distance to moon from earth
Ds = distance to sun from earth

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4
Q

The earth is –1– times bigger than the Moon

A
  • 4 times
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5
Q

the sun is 400 times bigger than the —–

A

Moon

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6
Q

astronomical unit is

A

the average distance between Earth and Sun 1AU = 1.5*10^8

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7
Q

one Light-year is —–( 1 a sentence)—– and is approx. —-2—

A

1) Distance travelled by light in one year
2) 9.46MM km (mega *mega)

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8
Q

Parsec is a distance at which 1AU perpendicular to the —–1—- line of sight —–2—– an angle of 1 —-3—-

A

1)observers
2)subtends
3)arcsec

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9
Q

a theory is

A

a set of tested ideas written using math to try explaining how things behave

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10
Q

A hypothesis is

A

an idea or set of ideas

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11
Q

A model is

A

an idea written in math language and that can be tested via experiments

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12
Q

theory

A

Models that can explain
and predict behaviours

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13
Q

Laws - theories that —1—- be proved –2—

A

1)cannot
2)proved

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14
Q

if earth was flat, —– and —- will happen at the same for —— on Earth

A

1) daytime
2) nighttime
3)everyone

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15
Q

earth curves —- m every —- km

A

5m
8km

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16
Q

kilometers for :
astronomical unit :
light years:
parsecs:

A

1) nearby objects / planets
2)distances within solar system
3) distance between stars
4)distances between galaxies

17
Q

Constellations:

-How many altogether?
-What are they?
-How many stars can the human in the best conditions

A
  • 88 constellations
    -groups of stars forming -images
    -6000
18
Q

angles can be used to measure the _____ size of an object. That is how ______ the object appears in the sky.

A

angular, wide

19
Q

angular distance: the distance in ____________ that seperates two objects in the sky

A

degrees

20
Q

diurnal motion is a consequence of …

A

Earth’s rotation around itself

21
Q

what is diurnal motion ….

A

how every day we see the sun, moon planets and stars rising in the east and setting in the west.

22
Q

How do we know that it’s earth rotating and the planets stars etc?

A

Foucaults pendulum

23
Q

yearly motion is a consequence of

A

consequence of Earth’s rotation around the sun

24
Q

celestial sphere is

A

an imaginary surface surrounding Earth that contains all objects in the sky

25
Q

Key points of the celestial sphere

A

Clestial equator
Zenith
North/South celestial poles
Horizon
Circumpolar stars

26
Q

MOTIONS OF THE CELESTIAL SPHERE
> The ____ axis of earth is slowly moving with time. This is called ————-

A

> rotation axis
Precession

27
Q

CELESTIAL CO-ORDINATES
Declination: measured in degrees, arcmin and arcsec. ——- distance —– or —– from the equator

A

1) angular distance
2)north
3)south

28
Q

Right ascension: ______ distance from the ___ _____ eastword along the celestial equator up to the circle used to measure its ________

A

1) angular distance
2) vernal equinox
3) declination