OPEN STAR CLUSTER M11 Rosalina Bonilla Jennifer Hsieh Mary Lou Juanatas Cluster 7: Stars, Sight, and Science OUTLINE Background of Star Clusters Description of project Messier 11 Ideal Gas Law Star Formation Stellar Evolution Observation & data collection of M11 Data analysis Results & conclusions What are open star clusters? Group of stars born at the same time Cluster contains Hot Young stars Found in the disk of spiral galaxies Metallicity – how much heavy elements are in the object Open cluster have lots of metals MAIN OBJECTIVES How old is M11? How do we know? Why does it matter? Fun Facts about M11 Nick Name: The Wild Duck Cluster One of the richest and most compact of open cluster Discovered in 1681 by Gottfriend Kirch 3000 stars Ideal Gas Law P= pressure V= volume n= number of particles T= temperature R= gas constant P V= n RT Star Formation Protostar – dust and gas collapses under gravity Pressure balances the forces of gravity Molecules in the protostar radiate allowing it to shrink Stellar Structure/Evolution Main sequence – hydrogen fuses into helium in the core Red giants swell up, causing the outer layers to cool which makes them red This happens when the core runs out of hydrogen OBSERVATION DATA ANALYSIS CONCLUSION M11 is 90 million years old with an ± of 10 million years Using the isoplot program we estimated the age of our M11 Open star clusters help us determine the metallicity of our universe The metalllicity of the universe is important because we’re made of metals ACKNOWLEDGEMENTS Advisors Vision Science Gabriel, Gene, Jason P., Jim, Joy, & Maribell Astronomy Jason Melbourne Nick Konidaris David, Elinor, Jason, Lynne, Marla, Nick, Scott Sea., Scott Sev. Teacher Fellow / Sci. Comm. Gary / Pascha REFERENCES WWW.ANTWRP.GFSC.NASA.GOV Http://antwrp.gsfc.nasa.gov/apod/astropix.ht ml (Astronomy Pic. of the Day) Http://mthamilton.ucolick.org/ (Lick observatory) www.tcho.la.asu.edu/ www.soral.as.arizona.edu/ www.ctio.noao.edu/ www.star.le.ac.uk/ www.physics.nwu.edu/ QUESTIONS?????