1 / 5

Section 2

Section 2. The sun. The sun’s layers. The Sun is a huge ball of gas that makes energy by fusing hydrogen into helium Photosphere-often called the surface of the sun. Temp is about 6000K Above photosphere is the chromosphere

eyad
Download Presentation

Section 2

An Image/Link below is provided (as is) to download presentation Download Policy: Content on the Website is provided to you AS IS for your information and personal use and may not be sold / licensed / shared on other websites without getting consent from its author. Content is provided to you AS IS for your information and personal use only. Download presentation by click this link. While downloading, if for some reason you are not able to download a presentation, the publisher may have deleted the file from their server. During download, if you can't get a presentation, the file might be deleted by the publisher.

E N D

Presentation Transcript


  1. Section 2 The sun

  2. The sun’s layers • The Sun is a huge ball of gas that makes energy by fusing hydrogen into helium • Photosphere-often called the surface of the sun. Temp is about 6000K • Above photosphere is the chromosphere • Corona is outermost layer. Largest layer, temps are as high as 2 million K

  3. Surface features • Sunspots – appear dark because they are cooler than other areas • Sunspots prove that the sun rotates • Sunspots are not permanent features

  4. Prominences and flares • Prominences are huge, arching columns of gas that can blast materials into space • Solar flares come from sun spots that shoot outward suddenly

  5. The Sun-an average star • Our sun is middle aged • Many stars orbit each other in a binary or triple star system. Our system has only one star • Some stars move through space as a cluster of stars

More Related