VOCAB: Unit 2 Flashcards

1
Q

Geocentric Model*

A

Earth is at the centre of the Solar System

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2
Q

Heliocentric Model*

A

Sun is at the centre of the Solar System

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3
Q

Perihelion*

A

The point of nearest approach of a planet to the Sun

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4
Q

Aphelion*

A

The point of greatest separation

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5
Q

Photosphere

A

The visible outer layer of a star, represents the depth within that gas at which we can see no deeper toward the core

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6
Q

Chromosphere

A

Surrounding the photosphere, an irregular layer of gasses that extend up and away from the photosphere, invisible to the eye

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7
Q

Corona

A

The outermost region of the Sun’s atmosphere, extends for millions of km in the space above the photosphere

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8
Q

Kelvin

A

A scale of temperature

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9
Q

Astronomical Unit

A

1 AU is the mean avg distance between the Sun and Earth

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10
Q

Spectroscopy

A

Measurement and analysis of energy spectra to determine the composition of matter

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11
Q

Genesis Mission*

A

Set out to capture particles of the solar wind and return them to study on Earth

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12
Q

Promineces

A

Arcs of gas that begin on the bright surface and soar to as much as 10000 km into the corona

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13
Q

Flares

A

Short-lived gas eruptions that generally last no longer than 20 min

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14
Q

Sunspots*

A

A region of the Sun’s photosphere marked by lower than average temperature, appearing black

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15
Q

Solar Wind*

A

Made up of charged particles sent out from the Sun at all times in all directions

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16
Q

Plasma

A

Ionized gas made up of a mixture of electrons and protons

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17
Q

Magnetosphere*

A

Magnetic field volume around a body like earth, which generates a magnetic field

18
Q

Aurora*

A

Visual effects of collisions, which produces lots of light photons. Borealis in the North and Australis in the South

19
Q

Red Giant

A

Lost all Hydrogen fuels

20
Q

White Dwarf

A

As the core cools down

21
Q

Black Dwarf

A

When it stops glowing

22
Q

Refractors*

A

Collect light by means of a glass lens

23
Q

Reflectors*

A

Collect light with a curved mirror

24
Q

Aperture

A

Determined by the diameter of the glass lens or the mirror

25
Q

Orbital Velocity*

A

Enough velocity to a place the satellite in a position that exactly balances gravity’s pull on the satellite w/the inertia of the satellite’s motion

26
Q

Geostationary satellite*

A

Satellite stays right over the same spot all the time

27
Q

Terrestrial Planets*

A

4 planets closest to the Sun that are dense, Mercury, Venus, Earth and Mars

28
Q

Gas Giants*

A

Large, low density planets, Jupiter, Saturn Uranus and Neptune

29
Q

Asteroids and Asteroid Belt*

A

Between terrestrial and gas giants, these were small, rocky objects

30
Q

Ceres*

A

Largest object in the asteroid belt

31
Q

Pluto*

A

Past the gas giants, VERY small, declassified as a planet

32
Q

Kuiper Belt*

A

Area past Pluto, icy bodies of all shapes and sizes

33
Q

Eris and Sedna

A

Larger objects found in the Kuiper Belt

34
Q

Oort Cloud

A

A belt, we have never seen, but we keep finding evidence of it’s existence

35
Q

Plutoids

A

All dwarf planets located toward the outer regions of the Solar System: Pluto, Eris, Haumea, and Makemake

36
Q

‘Nice’ Model*

A

Idea that Uranus and Neptune were pushed out

37
Q

‘Grand Tack’ Model*

A

Explains the size and distribution of the terrestrial planets

38
Q

Canada-France-Hawaii-Telescope (CFHT)*

A

A number of joint-venture instruments

39
Q

Hubble Space Telescope (HST)*

A

Orbits 600km about Earth, purpose was to gather light from cosmic objects. All telescopes on Earth had to make some compensation for the atmosphere and the distortion it created so they launched HST

40
Q

Escape Velocity*

A

Initial velocity any object needs to escape gravity