Team D: Kaniesha Stern Charles Ammon Jowers III Tracy Diggs Exo means outside of and Planet means Wanderer Exoplanets are planets outside of our solar system Alex Wolszczan discovered the first exoplanet 51 Peg was the second exoplanet discovered Kepler Satellite Mission 450 exoplanets have been confirmed Find habitable Planets Find signs of other life forms What else may we find in the universe • Kepler’s First Law: The orbit of every planet is an ellipse with the sun at one of its foci • Kepler’s Second Law: P2=a3 • Kepler’s Third Law: A planet moves the fastest when it’s closest to a star and Slowest when its furthest away from it’s star 51 Peg 4.23 0.62 0.24 1.88 1.0 84.0 11.86 164.8 29.46 Introduction of Our Solar System Transit detection is a way of discovering Exoplanets by viewing them at the moment of an eclipse Imaging is another way of discovering exoplanets by using a camera to take a picture Radial Velocity is used to determine Doppler Shift Doppler effect is the shift in frequency and wavelength of a wave Spectrographs are used for this method Wien’s Law states that hotter bodies emit at shorter wavelengths, and a higher frequency; cooler bodies emit at longer wavelengths and a lower frequency If a body emits in the blue, would you expect it to be hotter or colder than a body that emits in the red? Object: Cool star Sun Hot star Temperature: 4,000 K 5,777 K 50,000 K There are five variables that we used to describe planetary orbits, which are: • Mean Anomaly • Mass • Period • Eccentricity • Longitude of Periastron Spectroscopy interaction of matter and radiation. Spectrographs instruments designed to perform spectroscopy, by dispersing light. Emission Lines Absorption Lines Behaviors of Light Refraction Reflection Diffraction Earth has a blue sky and green grass … Why is the sky blue? Answer: The sky scatters more blue light than it does red light Different Types of Grass Acetone (CH3)2CO Spectrograph Measured what would appear on the absorption spectrum Why is the grass green? Answer: Chlorophyll reflects yellow and green light infrared light; but absorbs blue and red light Red Edge and How it can be used to detect life? Red edge is the signature of vegetation on earth Astronomers will look for red edge on other planets to see if they may have life —Image courtesy NASA/Johns Hopkins University Applied Physics Laboratory/Carnegie Institution of Washington Search for life outside of our Solar System has begun Besides Earth, there is no life on other planets in our Solar System Radial Velocity and Doppler effect, Transit Detection and Imaging are detection methods used to discover exoplanets Red edge is a signature of life on a planet, a characteristic that our planet has ; which will allow astronomers to find life on other planets. SEECoS and the Eberly College of Science Norman Freed-Dean of Eberly College of Science Ms. Jody Markley -UBMS Director Mr. Derek James -UBMS Assistant Director Suvrath Mahadevan -Assistant Professor Arpita Roy -Research Assistant Mr. Eric Speight –Teacher AND…. All the UBMS Staff and Faculty