1. pp. 294 - 301

2. Stars: The View from Earth  Some stars in the sky appear to be in grouped patterns. The best-known star pattern in the northern hemisphere is the Big Dipper. Different cultures around the world refer to this collection of seven stars by other names, such as the Plough, the Ladle, and the Great Cart.  The Big Dipper is part of a larger star pattern known as Ursa Major, which is Latin for Great Bear. Ursa Major is an example of a constellation.

3. Stars: The View from Earth  A constellation is a group of stars that, from Earth, resembles a recognizable form.  Astronomers have officially listed a total of 88 constellations. Examples: Cassiopeia, Orion, Pegasus.  It is important to note that the stars are at varying distances away.

4. How a Star Is Born  All stars form inside a collapsing nebula, a cloud of dust and gases.  A nebula’s collapse can be triggered by gravitational attraction of a nearby star or the shockwave from an exploding star.  The area with the largest mass starts to pull more mass in. The matter pulled in has excess energy which causes the central ball of material to begin to spin. Extremely high pressures build up inside the ball, which in turn causes the tightly packed atoms to heat up. As the temperature climbs, the core begins to glow. This is a protostar

5.  A protostar is a star in its first stage of formation. Eventually, the temperature of the spinning protostar rises to millions of degrees Celsius. This is hot enough for nuclear reactions to start. Over tens of thousands of years, the energy from the core gradually reaches the star’s outside. When that occurs, the fully formed star “switches on” and begins to shine.

6. The Life Cycle of Stars - Star Mass and Evolution  Astronomers describe stars in three general mass categories: low, medium, and high.

7. The Life Cycle of Stars - Star Mass and Evolution Low Mass Stars  Low mass stars use their nuclear fuel much more slowly than more massive stars do. Low mass stars burn so slowly that they can last for 100 billion year. This is due to less gravity and thus less pressure. The light from a red dwarf starts dim and gradually grows dimmer.  Eventually they collapse under their own gravity.  Over time a red dwarf will turn into a white dwarf.

8. Medium Mass Stars  Medium mass stars burn their fuel faster than low mass stars do, using their hydrogen up in about 10 billion years. When the fuel starts to run out the star slowly collapses under its own gravity. This raises the temperature enough to cause the fusion of helium and reignites the star. The star expands rapidly to a red giant. The fuel then runs out and the star slowly burns out.

9. High Mass Stars  High mass stars are those that are more than 10 times the mass of the Sun. In a high mass star, as gravity pulls matter into the centre of the star and squeezes the core, the nuclear reactions accelerate. As a result, a high mass star is hotter, brighter, and bluer than other stars.  After a fuel runs out the star cycles through collapsing and using another fuel. The star will become a supergiant like Polaris and Betelgeuse.

10.  Betelgeuse is so large that if it was in place of our sun it would reach Jupiter

11. Supernovas: The Violent End of High Mass Stars  After a star cycles through different fuels it eventual reaches iron. When all of the other fuels burn out, the star will essentially go out. The star then collapses with so much energy that it heats up to over a few million degrees and explodes. (Supernova)

12. High Mass Stars  The explosion is strong enough to create every element in the periodic table through fusion. Some of the fragments are sent far out into space while other debris may be made into new nebulae.  The star’s remaining core after a supernova explosion faces one of two outcomes, depending on the mass of the original star:

13. High Mass Stars  Neutron stars (mass between 10 and 40 times the mass of the Sun). A supernova explosion is directed not only outward, but also inward. This force causes the atoms in the star’s core to compress and collapse.  When an atom collapses, it forms neutrons, particles that are at the centre of most atoms already. When the star’s core becomes little more than a ball of neutrons only about 15 km across, it is called a neutron star. Neutron stars are made of the densest material known

14. High Mass Stars  Black holes — If the star was more than 40 times the mass of the Sun, it will become a black hole.  After exploding as a supernova, the star’s core is under so much gravitational force that nothing can stop its collapse, not even the formation of neutrons. In this case, the effect of gravity is so great that space, time, light, and other matter all start to fall into a single point.

15. The life Cycle of a Star  http://www.youtube.com/watch?v=PM9CQDlQI0A http://www.youtube.com/watch?v=PM9CQDlQI0A

16. The Hertzsprung-Russell Diagram he stars are arranged by three classifications. 1. By colour – Red stars are plotted on the right, and blue stars are plotted on the left. Other stars, such as the yellow Sun, are plotted in between. 2. By luminosity – The brightest stars are plotted at the top, and the dimmest stars are plotted at the bottom. A star with a luminosity of 100 is 100 times brighter than the Sun. 3. By surface temperature – The hottest stars are plotted on the left, and the coolest stars are plotted on the right.

17. The Hertzsprung-Russell Diagram

18. Homework  Read pp. 294 – 301  Answer # 1 – 6, 8, 9, 11 - 13