Test #1 Flashcards

1
Q

TERMINOLOGY
Constellation

A

Regions in the night sky with well defined bordered (typically contains asterisms/ patterns of stars)

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2
Q

Asterism

A

Patterns of stars

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3
Q

Celestial Sphere

A

Ancient Greeks thought the Earth was surrounded by a dome where all the stars and constellations were. (They didn’t know it was 3D thought they all were next to eachother)

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4
Q

Eliptic

A
  • Sun/planets traverse the sky along eliptic
  • eliptic makes similar angle with celestial equator as Earths tilt (mb if that sentence is confusing)
    -Zodiac constellations lie on it
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5
Q

Zenith

A

Look straight up

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6
Q

Meridian

A

Line arching from North to South through Zenith

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7
Q

Altitude

A

How high in degrees (horizon to zenith 90 degrees)

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8
Q

Azimuth

A

Idk

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9
Q

Revolution

A

-Orbit a central point/ object
- 365.25 days

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10
Q

Rotation

A

-Move/turn around on axis
-24 hrs
- stars seem to move because of rotation - Polaris doesnt move since lined up w North Celestial Pole

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11
Q

Circumpolar stars

A

Stars near North Celestial Pole

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12
Q

Latitude

A

Measures North to South position on Earth 0 degrees = equator
90 degrees = N
90 degrees = S
Idk if this is right 🤗

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13
Q

Longitude

A

Measures East to West position
0 degrees = prime meridian

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14
Q

R.A.

A

Measured in time (hrs, mins, sec)

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15
Q

Declination

A

Measured in degrees N or S
Can be reported down to arc second

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16
Q

Solstice/equinox names

A

Summer solstice
Winter solstice
Vernal equinox
Autumnal equinox

17
Q

Summer solstice

A

June 21st
Max tilt toward sun
Longest day

18
Q

Winter solstice

A

Dec 21st
Max tilt away from sun
Shortest day

19
Q

Vernal Equinox

A

March 21st
Slightly toward sun, equal amount day/night

20
Q

Autumnal Equinox

A

Sept 21st
Northern hemisphere is slightly away
Equal amount of day/night

21
Q

Solar Day

A

Rotation of Earth with respect to sun

22
Q

Sidereal Day

A

Rotation of Earth w respect to stars

23
Q

Difference in mins between sidereal and solar

24
Q

Giant Impact theory

A

Moon formed during collision between Earth and a small planet (mars sized) caused debris which made the moon

25
Q

Synchronous Rotation

A

We always see the same face of moon bc the moon rotation occurs at the same rate as its revolution around the Earth.

26
Q

Types of eclipses

A

Total solar eclipse
Partial solar eclipse
Annular solar eclipse
Lunar eclipse

27
Q

Total solar eclipse

A

Moon completely covers sun
Blocks sunlight
Very small region can see it

28
Q

Partial Solar Eclipse

A

Moon partially covers sun
larger region but not visible everywhere on Earth

29
Q

Annular solar eclipse

A

Moon is at point in orbit where its further away from Earth
Ring of sunlight is seen
Ring of fire

30
Q

Lunar eclipse

A

Occurs when Earth passes between sun and moon casting shadow on the moon.
May appear red due to dust/clouds

31
Q

Sunspots

A

Photosphere is cooler than other areas
Occurs when tightly wound magnetic fields poke nearly straight out and hot plasma is unable to enter region

32
Q

Prominences

A

Sunspots tend to occur in pairs, connected by a
loop of magnetic field lines that can arc high above
the Sun’s surface
● Gas in the Sun’s chromosphere and corona
becomes trapped in these giant loops, called solar
prominences
Last DAYS TO WEEKS

33
Q

Solar flares

A
  • Energy is released when magnetic field lines snap - leads to dramatic solar flares
  • minutes to hours
34
Q

CMES

A

huge balloon shaped plasma bursts that disrupt radio signals

35
Q

Aurora Borealis

A

-north pole one
-Suns always emitting charged particles (solar wind) which erupt in big bursts from flares, CMES + prominences.
-Particles reach magnetic field, goes towards the poles + interacts w gases

36
Q

Electromagnetic radiation

A

I think its that chart thing with microwave, radio uv etc

37
Q

Refracting Telescope

A

-Uses lenses to magnify objects
-objective lense infront of telescope
-eye piece at end
-objective lens thinner than eye piece

38
Q

Reflecting telescope - Two types

A

Newtonian - uses mirrors, concave that focuses light to secondary mirror which transmits to eye piece

Cassegrain-light path folds back in on itself, makes telescope more compact than traditional Newtonian