Lec9_2D
... two sources of energy, it becomes extremely bright. • The energy from this fusion (the radiation pressure) literally blows up (expands) the outer parts of the star many, many times. The surface of the star is moved far, far away from where the fusion is occurring, and so becomes cool. The star is no ...
... two sources of energy, it becomes extremely bright. • The energy from this fusion (the radiation pressure) literally blows up (expands) the outer parts of the star many, many times. The surface of the star is moved far, far away from where the fusion is occurring, and so becomes cool. The star is no ...
PHYS 2410 General Astronomy Homework 5
... 18. Which of the stars in the diagram above has the brightest absolute visual magnitude? ...
... 18. Which of the stars in the diagram above has the brightest absolute visual magnitude? ...
THE BIRTH AND DEATH OF A LOW/MEDIUM MASS STAR
... • THE STAGE WHEN A STAR IS IN IT’S “BEST” LIFE CYCLE • OUR SUN IS A MAIN SEQUENCE STAR • MAIN SEQUENCE STARS HAVE MOSTLY HYDROGEN. • THE HYDROGEN EXPLODES, GIVING OFF LIGHT AND HEAT • AS IT EXPLODES, THE HYDROGEN TURNS TO HELIUM. • HELIUM IS LIGHTER THAN HYDROGEN. • OUR SUN IS 4.6 BILLION YEARS OLD. ...
... • THE STAGE WHEN A STAR IS IN IT’S “BEST” LIFE CYCLE • OUR SUN IS A MAIN SEQUENCE STAR • MAIN SEQUENCE STARS HAVE MOSTLY HYDROGEN. • THE HYDROGEN EXPLODES, GIVING OFF LIGHT AND HEAT • AS IT EXPLODES, THE HYDROGEN TURNS TO HELIUM. • HELIUM IS LIGHTER THAN HYDROGEN. • OUR SUN IS 4.6 BILLION YEARS OLD. ...
The Life of a Star
... as a black hole. A small, very dense object with a force of gravity so strong that nothing can escape from it. Even light cannot get away from its surface so they can exist undetected. ...
... as a black hole. A small, very dense object with a force of gravity so strong that nothing can escape from it. Even light cannot get away from its surface so they can exist undetected. ...
Lecture103002
... light passing near the Sun was bent, stars appeared farther apart first demonstration of general relativity ...
... light passing near the Sun was bent, stars appeared farther apart first demonstration of general relativity ...
ASTR220 Collisions in Space
... Bright and variable X-ray emission. Found high-mass star at approximate location of X-ray source. Found that star has very large velocity shifts (40 m/s in each direction)… … must be something very massive swinging it around! ...
... Bright and variable X-ray emission. Found high-mass star at approximate location of X-ray source. Found that star has very large velocity shifts (40 m/s in each direction)… … must be something very massive swinging it around! ...
Basic Observations of Stars
... The apparent distribution of stars as seen on the sky can be monitored and the ‘sideways’ motions measured as changing directions, expressed as angles. This is called the star’s proper motion. (To calculate the actual speeds through space, we need to know their distances as well.) The changes are mo ...
... The apparent distribution of stars as seen on the sky can be monitored and the ‘sideways’ motions measured as changing directions, expressed as angles. This is called the star’s proper motion. (To calculate the actual speeds through space, we need to know their distances as well.) The changes are mo ...
L = σAT 4
... spectrum as all the gas is ionised so there are no bound electrons orbiting around the nuclei in the star. Thus absorption spectrums can also tell us something about the temperature of a star. ...
... spectrum as all the gas is ionised so there are no bound electrons orbiting around the nuclei in the star. Thus absorption spectrums can also tell us something about the temperature of a star. ...
Answers to Coursebook questions – Chapter E5
... A red giant forms out of a main sequence star when a certain percentage of the hydrogen of the star is used up in nuclear fusion reactions. The core of the star collapses and this releases gravitational potential energy that warms the core to sufficiently high temperatures for fusion of helium in th ...
... A red giant forms out of a main sequence star when a certain percentage of the hydrogen of the star is used up in nuclear fusion reactions. The core of the star collapses and this releases gravitational potential energy that warms the core to sufficiently high temperatures for fusion of helium in th ...
Barred Spiral Galaxy
... Galaxies that can't be classified as either spiral or elliptical are called irregular galaxies. ...
... Galaxies that can't be classified as either spiral or elliptical are called irregular galaxies. ...