Beyond Our Solar System - PowerPoint PPT Presentation

1 / 57
About This Presentation
Title:

Beyond Our Solar System

Description:

Beyond Our Solar System Ch. 25 star: a body of gases that gives off a tremendous amount of radiant energy in the form of light and heat Star Groups constellations: a ... – PowerPoint PPT presentation

Number of Views:35
Avg rating:3.0/5.0
Slides: 58
Provided by: NewHanove1
Category:

less

Transcript and Presenter's Notes

Title: Beyond Our Solar System


1
Beyond OurSolar System
  • Ch. 25

2
  • star a body of gases that gives off a
    tremendous amount of radiant energy in the form
    of light and heat

3
Star Groups
  • constellations a group of stars that form a
    pattern in the sky (88 different ones)

4
(No Transcript)
5
Orion
6
Ursa Minor
Ursa Major
7
Composition and Temperature
  • stars differ in size, density, mass, and
    composition

8
  • color of a star depends on its surface
    temperature
  • hot stars are blue (average surface temperature?
    35,000 K)
  • cool stars are red (average surface temperature?
    3,000 K)
  • our sun is yellow (average surface temperature?
    5,500 K)

9
(No Transcript)
10
Parallax
the slight shifting of the apparent position of
a star due to the orbital motion of Earth.
the nearest stars have the largest parallax
angles, while those of distant stars are too
small to measure.
11
(No Transcript)
12
(No Transcript)
13
Distance to Stars
  • light-year the distance light can travel in one
    year (9.5 trillion km)
  • it takes 8 minutes for the suns light to reach
    Earth
  • closest other star- Alpha Centauri (4.3 l.y.a)

14
Motion
  • actual motion must be measured only with a
    telescope
  • apparent motion motion due to the Earths
    movement

15
Stellar Magnitudes
  • apparent magnitude how bright a star appears
    from Earth- the lower the number, the brighter
    the object
  • absolute magnitude how bright a star really is

16
(No Transcript)
17
Distance, Apparent Magnitude, and Absolute
Magnitude of Some Stars
18
(No Transcript)
19
Life Cycle of a Star
20
  • nebula a cloud of gas and dust

21
(No Transcript)
22
(No Transcript)
23
  • protostar shrinking, spinning, glowing nebula
    (temperature rises)

24
Nuclear fusion begins- a star forms!
25
  • main sequence star longest stage of life cycle-
    nuclear fusion releases energy

26
  • red giant very large, cool bright stars- starts
    when hydrogen is used up- star cools and outer
    layers expand- size is 10xs bigger than our sun-
    this is next stage of our sun!

27
(No Transcript)
28
(No Transcript)
29
  • white dwarf small, hot, dim star- outer gases
    are lost and only core remains

30
  • supergiant extremely large, cool giant stars-
    very bright- 100 xs larger than the sun

31
  • supernova star that blows apart with a
    tremendous explosion- occurs in very massive stars

32
(No Transcript)
33
(No Transcript)
34
  • neutron star collapsed core of a supernova-
    dense ball of neutrons

35
(No Transcript)
36
  • black hole hole in space with gravity so great
    that not even light escapes- formed from
    collapsed supernova

37
(No Transcript)
38
(No Transcript)
39
(No Transcript)
40
Classification of Stars
  • H-R Diagram graph plotting surface temperature
    and absolute magnitude of each star

41
(No Transcript)
42
  • galaxies large scale groups of stars held
    together by gravity
  • there are 50 billion-1 trillion galaxies
  • we are in the Milky Way galaxy

43
Images of the Milky Way Galaxy
44
(No Transcript)
45
(No Transcript)
46
(No Transcript)
47
Types of Galaxies
  • spiral bright center of stars with arms
    spiraling out
  • Milky Way is a spiral

48
Andromeda Galaxy
49
Structure of the Milky Way
50
  • barred spiral have a group of stars making a bar
    through the center

51
  • elliptical shape ranges from spherical to oblong
  • no arms

52
  • irregular small, faint stars spread out
    unevenly with no pattern

53
Large Magellanic Cloud
Small Magellanic Cloud
54
Galaxy Cluster
55
The Big Bang
? The big bang theory states that at one time,
the entire universe was confined to a dense, hot,
supermassive ball. Then, about 13.7 billion years
ago, a violent explosion occurred, hurling this
material in all directions.
56
(No Transcript)
57
Big
Write a Comment
User Comments (0)
About PowerShow.com