Star Formation and the Era of Reionization

Star Formation and the Era of Reionization

This text discusses the process of star formation, focusing on how main sequence stars burn hydrogen and the significance of the Era of Reionization.

About Star Formation and the Era of Reionization

PowerPoint presentation about 'Star Formation and the Era of Reionization'. This presentation describes the topic on This text discusses the process of star formation, focusing on how main sequence stars burn hydrogen and the significance of the Era of Reionization.. The key topics included in this slideshow are star formation, main sequence stars, nuclear fusion, Era of Reionization, protostars,. Download this presentation absolutely free.

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1. Star Formation Szydagis 03.30.2015 1/12

2. For most of their lives, main-sequence stars burn _______, converting it into _______ via nuclear fusion. A. Carbon, hydrogen B. Hydrogen, helium C. Oxygen, hydrogen D. Helium, nitrogen All stars begin their lives as protostars that are initially ______. A. Much hotter B. The same size C. Smaller in size D. Bigger in size 2/12

3. The Era of Reionization About ~500 million years after the Big Bang, stars began to form for the first time, and universe ceased being dark in the optical (visible) wavelengths, since stars shine This event is called reionization . Why? The universe stopped being ionized after recombination , but now with the formation of stars ions return because a star is hot enough to ionize atoms of gas making up the universe The first stars were huge, and when they exploded at the ends of their lives, casting off their outer layers, they thus seeded the cosmos with the material necessary to make the next generation of (smaller) stars we know and love Also left behind supermassive black holes as galaxy cores 3/12

4. Protostars A gas cloud (mainly of hydrogen and helium) can become Jeans unstable , by being massive and/or large enough to collapse (symmetrically into sphere, with gravity), heating up as shrinking Collapse ceases when fusion ignited, pressure building up Protostars can come in different sizes. Bigger ones become bigger stars, and the bigger they are, the faster they fall (faster they burn out: living fast and dying young) 4/12

5. Dwarf Stars Still-born stars are brown dwarfs . Not heavy/big enough to become stars. Just giant balls of gas, like planet Jupiter, except even more vast (couple of orders of magnitude) Dont collapse further because even without fusion gas certainly has an intrinsic pressure, can balance out gravity, especially if not much mass, producing not much force On the other hand, red dwarfs are between brown dwarfs and our sun in mass. They are cool and burn hydrogen very slowly, living for billions / trillions of years in theory Possibly most common star in the Milky Way, but faint Out of H? Become blue dwarf stars, but universe still too young to have seen any. Eventually, blue->white->black 5/12

6. Nebular Nurseries Gigantic dusty clouds of gaseous atoms and molecules often many light years across within even larger nebulae (hundreds or thousands ly) constitute stellar nurseries It takes thousands of years (cosmic blink of an eye) Radio, infrared, x-rays can penetrate the curtain of dust Coldness of space actually aids in star formation (that is why the universe had to cool down before birth of stars, to <~100 degrees Kelvin, to prevent hot diffusion) Lack of heat means gravity can do its work, and not have gas pressure disperse the particles attracting each other Joke: 6/12

7. Chandra X-ray Observatory NGC 604 in galaxy M33 Astro Systeme Austria N12 f/3.5 astrograph 7/12

8. Star Clusters Stars automatically like to form in groups because they develop from immense clouds with enough material for many stars: the formal term for their bunches is cluster Young, loose, irregular clusters are called open (or, galactic) clusters, while old, dense, symmetric clusters are known as globular clusters, found everywhere Open clusters still have loose gas, while globular ones, with more stars, have used it all up (to make new stars) Not all stars observed in clusters. During gravitational collapse of gas and stars to form a cluster, through random motion some stars attain escape velocity, leave 8/12

9. (Some globular clusters are failed galaxies, with black holes) Jewel Box (open) cluster University of Oregon a.k.a. M13 Time permitting: a return to the kitchen cosmos 2513005/behold-the-cosmos-created-from-the- contents-of-a-kitchen?sc=ipad?f=1001 (slides 2, 7, and 10 this time) 9/12

10. An Activity (Sorting) Two categories minimum, and you cant put everything into its own category Something can only be in one category, not multiple, and you should try and reach a consensus with your group 10/12

11. On the main sequence, larger stars are _______ than/as smaller stars, in general. A. The same temperature B. Colder C. Hotter D. Darker With the exceptions of the red giants and supergiants, the larger stars are also _______. A. Brighter B. Dimmer C. Faster-rotating D. Younger 11/12

12. Homework and Quotes Re-read text and plot about the main sequence and the H-R diagram Read again carefully, with understanding I hope the light reading loads mean that everyone finishes them on time! Turn in homework #7 now to Steven. You can pick up #8 in the back Special due date Original illustration by Sidney Paget 12/12