astrology Flashcards

1
Q

what is the universe? where does this understanding come from?

A

the universe is all that exists everywhere, including all matter, energy, planets, stars, galaxies, and the space in which all of this exists. what we know and understand about the universe is based on who we are, where we live, what century we live in, and what culture we are from.

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2
Q

what sort of objects can we see in our skies? list them all

A

the sun, moon, stars, and planets (mercury, Venus, mars, Jupiter, and Saturn) along with comets, meteorites, novas and supernovas, and the Milky Way

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3
Q

how do we know that people in the past observed the movements and patterns of sky objects? what sort of evidence have they left us with?

A

people have made and left objects to show what they observed in the sky (drawings, sculptures, and monuments). they observe the movement of the sun and moon, and when solstices occur.

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4
Q

constellation

A

group of stars that form a pattern in the sky

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5
Q

how many constellations are there? give examples

A

88 known constellations (virgo, Hercules, Orion)

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6
Q

what is an asterism? give an example. how are they useful?

A

smaller groups of stars that form shapes within the constellation. the Big Dipper. they help to tell directions when compasses are not available.

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7
Q

celestial sphere

A

an imaginary rotating sphere on which lie all objects of the night sky. it extends around earth and is divided in to the northern and Southern Hemispheres (thus an observer can only see half).

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8
Q

ecliptic

A

path the sun and some other sky objects appear to take across the celestial sphere, due to earth’s orbit around the sun.

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9
Q

why do objects in the sky seem to move from east to west?

A

because of earth’s rotation

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10
Q

retrograde motion

A

makes planets appear to move across the sky, then loop back in the opposite direction
- due to earth going around the sun faster than the outer planets in the solar system

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11
Q

azimuth and altitude

A

azimuth: distance measured from the north along the horizon to a point below the celestial object
altitude: angular height of a celestial object measured from the horizon

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12
Q

the voyageur and its purpose

A

a spacecraft carrying gold-plated greetings, sights, and sounds from earth. purpose is to study outer planets

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13
Q

difference between optical telescope and radio telescope

A

radio telescopes can be used on cloudy days as well as at night because they detect radio waves, while optical ones only detect visible light (only detect small part of electromagnetic spectrum)

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14
Q

why are some telescopes placed in orbit above our atmosphere?

A

to observe space in more detail. (Ex/ only a fraction of electromagnetic radiation from space reaches earth’s surface. Therefore, some telescopes are in space to take advantage of the wealth of info the whole spectrum of this radiation provides).

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15
Q

how do telescopes that detect non-optical radiation contribute to our understanding of space?

A

from using them, we can determine what stars/planets are made up of and the radiation they give off.

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16
Q

galaxy

A

a collection of many billions of stars, plus gas and dust, held together by gravity. formed when a cloud of gravity, stars, and dust begins to contract.

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17
Q

what galaxy are we a part of?

A

The Milky Way (400 billion stars)

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18
Q

who discovered the first galaxy? when?

A

galileo discovered galaxies in 1610, but William Herschel discovered that the Milky Way is made of a collection of stars with his telescopes with his sister in 1780.

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19
Q

describe 3 types of galaxies

A

elliptical galaxies: - spherical to oval in shape
- older galaxies with few young stars
- 15-20 percent of all galaxies we see
spiral galaxies: - have a bulge in the centre and spiral arms on the sides
-70-75 percent of all galaxies
- have old stars in the centre and young stars on spiral arms
irregular galaxies: - have no definite shape and no spiral arms or central core
- 10 percent of all galaxies

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20
Q

star cluster

A

a collection of stars held together by gravity. open clusters have 50-1000 stars and appear around the Milky Way’s disk, and globular clusters have spherical shapes and 100000-1000000 stars

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21
Q

diameter of Milky Way

A

100 000 light years

22
Q

characteristics of Milky Way

A
  • it’s special.
    a) it’s got a disk-like shape
    b) it’s got a halo of globular star clusters in the centre
    c) it’s got lanes filled with clouds of gas and dust
  • it’s part of the Local Group made up of 50 galaxies
  • the Local Group belongs to the Virgo Supercluster, which is a large collection of galaxies
23
Q

what’s our nearest galaxy?

A

Andromeda (2.6 million ly away)

24
Q

the Local Group

A

made up of many small irregular and elliptical galaxies and is dominated by 2 large spiral galaxies: the Milky Way and Andromeda

25
Q

what’s an AU? what’s the distance between the sun and neptune? what’s the distance to the closest star?

A

astronomical unit. 30 AU between the sun and Neptune. 268 000 AU to the closest star.

26
Q

light year

A

a unit of distance equal to the distance light travels in 1 year

27
Q

what’s parallax and how does it help us determine distance?

A

parallax is the apparent change in position of an object against a fixed background when it’s viewed from 2 different lines of sight, so it can help us measure interstellar distances (the distances between stars in our galaxy) through triangulation

28
Q

luminosity

A

amount of energy a star gives off per second. indicates how bright a star is

29
Q

absolute magnitude

A

indicates how bright a star would be if it were 32.6 light years from earth

30
Q

colour of a star gives off what info?

A

how hot its surface temperature is (fairly hot star has bluish colour, fairly cool star has reddish colour)

31
Q

how do we know that the sun and other stars are made up of hydrogen and helium?

A

astronomers use a spectroscope to analyze the light from stars. a spectroscope is an instrument that produces a pattern of colours and lines, called a spectrum, from a narrow beam of light. a star’s spectrum identifies the elements of which it’s composed.

32
Q

what’s 1 solar mass? why’s this scale important?

A

1 solar mass is 10 x 10^30 kg. solar masses are how star masses are expressed so yeah it’s important… (NOT A QUALITY RESPONSE… COME BACK TO THIS)

33
Q

Hertzsprung-Russell diagram

A

graph that shows the colour and absolute magnitude of stars. has star colour (ranging from red to blue) on the x-axis, and absolute magnitude on the y-axis.

34
Q

main sequence

A

narrow band of stars on the H-R diagram that runs diagonally from the upper left (bright hot stars) to the lower right corner (dim cool stars). they account for 90 percent of stars we can see from earth

35
Q

compare and contrast life cycles of low mass, intermediate mass, and high mass stars

A

low: - use up their hydrogen fuel slowly over a period of 100 billion years
- will eventually become white dwarfs that are faint but hot
intermediate: - use up their hydrogen fuel in about 10 billion years
- when the hydrogen fuel is used up, the star becomes a red giant and eventually a planetary nebula and then a white dwarf
high: - use up their hydrogen fuel quickly and as a result form supergiants
- their core collapses violently and the outer layers explode causing a supernova

36
Q

supernova

A
  • massive explosion in which the whole outer portion of a star is blown off
  • Iron forms in the core of the star - its heat cannot be released through fusion and the core collapses violently, causing a shock wave to travel through he star
37
Q

neutron star

A

star so dense that only neutrons can exist throughout

38
Q

black hole

A

remnant of a supernova explosion with a gravitational field so strong that nothing can escape its pull

39
Q

Big Bang theory

A

the theory that the universe began about 13.8 billion years ago when something unimaginably small and dense suddenly and rapidly expanded to immense size

40
Q

Doppler effect

A

when spectral lines for galaxies are displaced from their normal positions (explains why ambulance changes pitch as it approaches you, passes you, and moves away. as it moves toward you, siren’s sound waves are compressed, resulting in shorter wavelength and higher pitch. as it moves away from you, siren’s sound waves are lengthened, resulting in longer wavelength and lower pitch). light waves from a moving object differ in colour as well.

41
Q

redshift and blueshift

A

redshifted: for objects moving away from an observer, the effect of lengthening their wavelengths toward the red end of the visible spectrum. blueshifted: for objects moving towards an observer, the effect of shortening their wavelengths toward the blue-end of the visible spectrum.

42
Q

conclusion drawn from redshift

A

the universe is expanding.

43
Q

cosmic microwave background radiation

A

radiation left over from the Big Bang which fills the universe. Robert Wilson and Arno Penzias discovered this when they observed static coming from all directions in the sky.

44
Q

dark matter and dark energy

A

dark matter: - there is more mass than can be accounted for by visible matter, and the missing matter is called this
- it emits no light and has not been detected
- it seems to form a large spherical halo around galaxies
- it is the most abundant form of matter in the universe
dark energy: - causes the universe to expand at an accelerating rate
- strength of dark energy increases with distance

45
Q

COBE and WMAP

A

COsmic Background Explorer and Wilkinson Microwave Anistropy Probe. they are NASA satellites that measure cosmic microwave background radiation

46
Q

how long does it take for light from the sun to reach earth?

A

8 mins. we are looking back in time bois

47
Q

triangulation

A

method that uses parallax to calculate the distance from earth to the stars

48
Q

binary star system and how it relates to star mass

A

two stars that orbit each other. mass of stars can be determined by calculating the size of the orbit of a binary star system and the time it takes for the stars to complete one orbit

49
Q

pulsar

A

neutron star that releases pulses of radiation

50
Q

Hubble law

A

The speed of a galaxy (which can be determined from the amount or extent of its redshift) is proportionate to the distance of the galaxy from Earth. when drawn on a graph, this relationship becomes the Hubble constant (rate at which universe is expanding)