Supernovas+-+JV

=Getting Started=
 * **Click on the edit button above to put your own content on this page.**

=Project Documents:=

Rubric: [[file:Space Exploration Adventure Rubric.doc]], [[file:Space Exploration Adventure Rubric.pdf]]

 * Written Information **: As you enter text, the area will expand. Make sure to check the required details of the assignment and review the rubric (see document links) to self-assess your work. Your paragraphs will be in block format, enter one return between paragraphs. The tab key, indent feature will not appear when typing directly into the wiki page.

Visuals Make sure to include the location of your image; add a caption with this information N = mp/(4r3 o/3) = 2 × 1017 kg/m3 ,

**Works Cited** **Sources** : Include the source information for all of the magazine articles, reference sources (encyclopedias) and web site pages that were used to complete your project. The source information for encyclopedias may be found at the end or beginning of each entry in iCONN. When using periodicals, the publication information will be at the beginning or end of the article. This needs to be formatted for MLA standards. If it is not labeled 'Source Citation' it can be formatted appropriately by using EasyBib.com. You should use EasyBib for the web sites. The final Works Cited should be listed in alphabetical order by the first word of the source citation. "Milky Way." //Kids InfoBits Presents: Astronomy//. Gale, 2008. Reproduced in Kids InfoBits. Detroit: Gale, 2012. "The Milky Way." //WMAP's Universe//. NASA, 28 June 2010. Web. 06 Mar. 2012. . Vergano, Dan. "Galaxy Bracketed by Big Bubbles." //USA Today// 10 Nov. 2010: 05A. Web. 6 Mar. 2012.
 * Sample:**

4 Type II Supernova Physics
 * Your Source List:**

**Topic: Research Focus**
 * What is your topic?**
 * State the focus of your research:**

**Notes**

+ 56Fe $. . . ! 13 4He + 4n ;

+ 4He ! 2p + 2n (16)

(ii) Inverse beta decay. When electrons have K > 3.7 MeV then the

following can occur:

e− + 56Fe ! 56Mn + e

and by time we get down to nucleons:

e− + p ! n + e

+ 56Fe $. . . ! 13 4He + 4n ; + 4He ! 2p + 2n (16) (ii) Inverse beta decay. When electrons have K > 3.7 MeV then the following can occur: e− + 56Fe ! 56Mn + e and by time we get down to nucleons: e− + p ! n + e ==== acts that you will use to write your final paper. You may want to label sections of your notes to help you be more organized as you write. As you take notes from a source, you should list the source citation in the Works Cited section above. ====