Lecture 1 Flashcards

1
Q

What is our place in Universe?

A

Earth - Solar System - Milky Way Galaxy - Local Group - Local Supercluster

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2
Q

A cosmic Inventory

A

Stars, planets, moons, Asteroids, Comets, Solar System, Nebulae, Galaxies, Galaxies Groups, Galaxy Clusters, Universe

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3
Q

Star

A

A large, glowing ball of gas that generates heat and light through nuclear fusion

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4
Q

Planet

A

A moderately large object that orbits a star, it shines by reflected light. Planets may be rocky, icy, or gaseous in composition

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5
Q

Moon

A

An object that orbits a planet

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6
Q

Asteroid

A

A relative small and rocky object that orbits a star

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7
Q

Comet

A

A relatively small and icy object that orbits a star

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8
Q

Solar (Star) System

A

A star and all the material that orbits it, including its planets and moons

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9
Q

Nebula

A

An interstellar cloud of gas and/or dust

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10
Q

Astronomical Unit (AU)

A

Average distance between the Earth and the Sun (150 million kms)

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11
Q

Light Year

A

the average distance that light can travel in 1 year

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12
Q

Is light year a distance measurement or a time measurement?

A

Distance Measurement

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13
Q

Where to find the Orion Nebula

A

The Orion Nebula is about 1350 light years away and 13 light years wide
It is a star forming region

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14
Q

Galaxy

A

A great island of stars in space, all held together by gravity and orbiting a moon center

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15
Q

Where to find the Andromeda Galaxy

A

The Andromeda galaxy is about 2.5 million light years away. It will collide with the Milky Way Galaxy in 4 billion light years

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16
Q

Galaxy group

A

A gravitationally bound group of up to a few dozen galaxies typically a few million light years across

17
Q

Galaxy Cluster

A

A group of a few hundred to a few thousand galaxies
Abell 1689, about 2.2 billion light years away

18
Q

Light Travels at

A

Finite speed of 300,000km/s

19
Q

Light travel time to moon

A

1 second

20
Q

Light travel time to sun

A

8 minutes

21
Q

Light travel time to Sirius

A

8 years

22
Q

Light travel time to Andromeda Galaxy

A

2,5 million years

23
Q

How do we see objects as they were in the past?

A

The farther away we look in distance, the further back we look in Time

24
Q

Can we see the Entire Universe?

A

No, we cannot see the entire universe, because the universe is only about 14 billion years old. Its too far away for us to see it

25
Q

How did we come to be?

A

The Universe is expanding
All galaxies are moving away from each other
Tracing this motion backward leads to a point where the expansion began, referred to as the Big Bang
Gravities drives collapse of matter into galaxies and galaxy clusters
Most galaxies formed within a few billion years after the Big Bang.

26
Q

How did Gravity play a role in “How did we come to be?”

A

Gravity drives collapse of clouds of gas and dust to form stars and planets

27
Q

Stars go through

A

Life cycles

28
Q

How did we come to be?

A

The Big Bang produced hydrogen and helium.
– All other elements were constructed from H and He in stars
and then recycled into new star systems, including our solar
system.
– We are made of elements produced in the nuclear fusion
within the cores of stars.

29
Q
A