READING: - PowerPoint PPT Presentation

1 / 27
About This Presentation
Title:

READING:

Description:

READING: Units: 59, 60 – PowerPoint PPT presentation

Number of Views:30
Avg rating:3.0/5.0
Slides: 28
Provided by: wis119
Category:
Tags: reading | dwarf | planets

less

Transcript and Presenter's Notes

Title: READING:


1
READING
Units 59, 60
2
The Family of Stars
3
Stars come in all sizes
4
The Mass-Luminosity Relation
  • If we look for trends in stellar masses, we
    notice something interesting
  • Low mass main sequence stars tend to be cooler
    and dimmer
  • High mass main sequence stars tend to be hotter
    and brighter
  • The Mass-Luminosity Relation
  • Massive stars burn brighter!

5
Massive stars burn brighter
LM3.5
6
Luminosity Classes
7
Stellar Evolution Models and Observation
  • Stars change very little over a human lifespan,
    so it is impossible to follow a single star from
    birth to death.
  • We observe stars at various stages of evolution,
    and can piece together a description of the
    evolution of stars in general
  • Computer models provide a fast-forward look at
    the evolution of stars.
  • Stars begin as clouds of gas and dust, which
    collapse to form a stellar disk. This disk
    eventually becomes a star.
  • The star eventually runs out of nuclear fuel and
    dies. The manner of its death depends on its
    mass.

8
Evolution of low-mass stars
9
Evolution of high-mass stars
10
Tracking changes with the HR Diagram
  • As a star evolves, its temperature and luminosity
    change.
  • We can follow a stars evolution on the HR
    diagram.
  • Lower mass stars move on to the main sequence,
    stay for a while, and eventually move through
    giant stages before becoming white dwarfs
  • Higher mass stars move rapidly off the main
    sequence and into the giant stages, eventually
    exploding in a supernova

11
Our Sun will eventually
A. Become white dwarf
B. Explode as a supernova
C. Become a protostar
D. Become a black hole
12
The spectral type of a star is most directly
related to its
  • Absolute magnitude
  • b. Surface temperature
  • c. Size or radius
  • d. Luminocity

13
Which two vital parameters are used to describe
the systematics of a group of stars in the HR
diagram?
  • a. Mass and weight
  • b. Luminocity and radius
  • c. Surface temperature and mass
  • d. Luminocity and surface temperature

14
Which is one of Keplers laws
  • a. For every action has an equal and opposite
    reaction
  • b. Planets move in elliptical orbits
  • c. Fma
  • d. Planets move in perfect circles around the sun

15
A solar exlipse can occur ONLY when
  • a. the Moon comes between the Earth and the Sun
  • b. the Sun comes between the Moon and the Earth
  • c. the Earth comes between the Moon and the Sun
  • d. the Sun, Moon and Earth form a precise
    right-angled triangle

16
When dropped by an astronaut on the Moon, two
objects of different mass will
  • a. Have different accelerations proportional to
    their masses
  • b. Have different accelerations, the more massive
    object having the smaller acceleration
  • c. Have the same acceleration
  • d. Have no acceleration at all in the airless
    space

17
According to Newton's laws, a force must be
acting whenever
  • a. an object's position changes
  • b. the direction of an object's motion changes
  • c. time passes
  • d. an object moves with non-zero speed

18
Kepler's first law states that a planet moves
around the Sun
  • a. in a circle with the Sun at the center
  • b. in an elliptical orbit, with the Sun at the
    center of the ellipse
  • c. in an elliptical orbit, with the Earth at the
    center of the ellipse
  • d. in an elliptical orbit, with the Sun at one
    focus

19
If an object has an orbit around the Sun that has
an essentricity of 0.1, then the orbit is
  • a. a straight line
  • b. exactly circular
  • c. almost circular, but not quite
  • d. a long, thin ellipse

20
What causes sunspots?
  • a. differential rotation on the Sun creates
    vortices, or eddies, which are cooler and darker
    than the rest of the solar surface
  • b. solar flares cause the photoshere to expand
    and cool in the vicinity of the flare
  • c. magnetic fields breaking through the
    photosphere inhibit heat conduction where the
    field is strong
  • d. masses of heavy elements occlude solar light

21
Spectral types (e.g. O, B, A, F, G, K, M) define
uniquely their
  • a. surface temperatures
  • b. luminosities
  • c. sizes of radii
  • d. brightnesses

22
Which of the following astronomical systems are
held together by gravity
  • a. The Sun
  • b. The Solar System
  • c. The Milky Way
  • d. All of them

23
If a new planet were found with a period of
revolution of 6 years, what would be its average
distance from the Sun?
  • a. About 1AU
  • b. About 3.3 AU
  • c. About 6 AU
  • d. About 36 AU

24
In order of increasing wavelength the
electro-magnetic spectrum is
  • a. gamma rays, blue light, red light, radio
    waves
  • b. ultraviolet, gamma rays, blue light, radio
    waves
  • c. red light, radio waves, X rays, blue light
  • d. visible, ultraviolet, X-rays, radio

25
Light has properties
  • a. of waves
  • b. of particles
  • c. none of the above
  • d. both a. and b.

26
What is the Law of Inertia?
  • A body at rest stays at rest unless acted on by
    an outside force
  • b. Fma
  • c. P2A3
  • d. FgmMG/R2

27
What is retrograde motion?
  • a. backward moving/ or interrupted movement of
    a planet on the sky
  • b. Clockwise rotation of the moon around the
    earth
  • c. Rotation of planets around the sun
  • d. Large elliptical movements of comets
Write a Comment
User Comments (0)
About PowerShow.com