PPT-Planetary Orbits Recall eccentricity e defined by:

The semimajor axis is represented by a and the semiminor axis is b Therefore e0 for a circular orbit   Question Use the sheet of information below to summarize the list of planets in order of. udles Nacho L57524opez Departament de Matematica Universitat de Lleida 25001 Lleida Spain email nlopezmatematicaudles Abstract The eccentricity of a vertex in a strongly connected digraph is the maximum distance from The eccentricity sequence of a Topic:. Orbital dynamics and. the restricted 3-body problem. Lecture by: C.P. Dullemond. Objects of the Solar System. Kuiper Belt. (30-50 AU). 10 AU. 1 AU. Earth. Mars. 1 AU. 1.38-. 1.67 AU. e. = 0.1. geometric . fluctuations of the . Glauber. model make specific predictions for . a dipole and triangle terms in the observed azimuthal distribution of particles. Preliminary . results on . the v. 1. Understanding Planetary Migration. Norio Narita. National Astronomical Observatory of Japan. Relation to Prof. Miyama. Based on “Astronomer’s family tree in Japan”. Prof. Miyama was “brother” of Prof. Katsuhiko Sato. Planet A most likely represents. a) Earth b) Venus c) Saturn d) Uranus. Do Now – Regents Question. Planet Revolution. Planets in our solar system . revolve . around the sun in . elliptical. orbits. . Eccentricity – . The ratio of distances. . It basically tells how close a conic section is to being a circle.. In a parabola: . . e. . = 1. In an ellipse or hyperbola:. The . ratio between the foci and the vertices. Motions of the Planets. The ancient astronomers believed that the Universe was made up of spheres (orbs). The sphere that contained all of the objects seen in space was the Celestial Sphere. The sphere rotated around the earth making it appear as if all celestial objects were revolving around the earth. In this image you can see the stars and the Sun look as if they’re attached to the sphere Where is the person in the image trying to get to?. We have so far discussed the basics of an ellipse. Specific type of conic section. “Oval”. Major . vs. Minor Axis. Locations of foci. Graphing; centered at origin or somewhere else. Skinny Factor. Grades are posted on course website. Average = . 127/180, . s.d. . = . 26 (Section 1). 132/180, . s.d. . = 24 (Section 4). Highest . 180/. 180. Scores below 100 => “serious concerns”. Planetary Migration of Jovian . Exoplanets. Norio Narita. National Astronomical Observatory of Japan. Outline. Brief review of orbits of Solar System bodies. Introduction of . exoplanets. and migration models. – Recall Recall Date: March __ , 2014 Recall Number: 14 - DRAFT FOR CLEARANCE BedHead Pajamas Recalls Children’s Pajama s Due to Violation of Federal Flammability Standard WASHINGTON, Systems . The New Science of Distant Worlds. © 2018 Pearson Education, Inc.. 10.1 Detecting Planets Around Other Stars. Our goals for learning:. How do we detect planets around other stars?. © 2018 Pearson Education, Inc.. A Study in Simplifying Models. Anthony Ko. Motivation (Why this is important):. Despite popular belief, a significant amount of satellites experience drag, which causes them to fall to Earth and gain eccentricity . Getting the Audience’s Attention. LPI Education and Public Engagement. August 22, 2018. Online Participants. Joining online? . Please share your thoughts and responses. throughout the session in the chat box..