PPT-Building a comet

Whats a Comet Made of dirty snowball model Composed of Ices water CO 2 and others Gases water CO 2 CO O 2 and some simple organics Tiny dust particles organic and inorganic. ISON . OBSERVING . CAMPAIGN . (=CIOC) SBAG Update Jan – Jul 2013 . CIOC . Team. established Jan 2013 at SBAG-8. . Team has a mix of experiences, skillsets, and research specialties. . Abundant contributions from early- and mid. European Space Agency (ESA). Launched 10 years ago, 5 Earth flybys to save fuel and weight. Rosetta Explores a Comet. Comet 67P or . Churyumov-Gerasimenko. (after who found it). 4x4.5 km – here with Los Angeles for scale. Andrew Cheng . (JHU/APL; andrew.cheng@jhuapl.edu). Steve Arnold . (. JHU/APL). Pietro. . Bernasconi. . (JHU/APL). Karl . Hibbitts. . (JHU/APL). Eliot . Young. . (. SwRI. ). Tibor. . Kremic. . (GRC). Comets. one of the most glorious things to see in the sky is a comet.. May be visible for only days, weeks, or months. Comet. : chunks of ice and dust whose orbits are very long, narrow ellipses.. Think of them as a “dirty snowball”. COMET. μ-e conversion search from . muonic. . aluminium. J-PARC pulsed proton beam to produce pulsed . muon. beam. Forbidden in the Standard Model .  clue to the new physics beyond the Standard Model. In this lesson, we are . going to be comparing comets, meteors, and asteroids which are found . in the Solar System. . Essential Question:. What is the difference between a comet, meteor, . and asteroid?. . Shahzeb Siddiqui - sms5713@psu.edu. Software Systems Engineer. Office: 222A Computer Building. Institute of . CyberScience. . May . x. th. . 2015 . System Overview. Comet is one of the XSEDE cluster designed by Dell and SDSC that delivers 2.0 PFLOPS of performance. . Challenger Tragedy. Francis . Scobee. , Michael . Smith, Ronald McNair, Ellison . Onizuka. , Judith . Resnik. , . Gregory Jarvis, and Christa . McAuliffe. First time a teacher was on . board the Space Shuttle.. muon. particle physics . programmes. at J-PARC. Mu_01. Satoshi MIHARA. IPNS, KEK. FKPPL-FJPPL workshop, . Yonesei. Univ.. Outline. Introduction. Physics motivation. J-PARC facility. France-Japan collaboration in the COMET experiment at J-PARC. (. Danio. . rerio. ) . as a model. Chris A. . McCabe. 1. , Chris W. Theodorakis. 2. , Theodore B. Henry. 1. and Mark G. J. . Hartl. 1. Introduction . Environmental stressors can damage the DNA of aquatic organisms. The Oort Cloud. What is the Oort Cloud?. Spherical area between 5,000 and 100,000 AU from the sun (Kuiper belt ends at 55 AU). Proxima Centauri is 270,000 AU from sun. Contains between 0.1 and 2 trillion comets. dust tail. - A long, wide tail buffeted by photons emitted from the Sun, but it curves slightly due to the comet's motion.. hydrogen envelope. - Hydrogen gas that surrounds the coma of the comet and trails along for millions of miles (it is usually between the ion tail and the dust tail). The hydrogen envelope is about 10 million km across at the nucleus of the comet and about 100 million km long.. Akiva Bar-Nun and Diana Laufer . Dept. of Geosciences, Tel Aviv University. Thanks to the OSIRIS team. 1. The comet is chaotic since it was formed by agglomeration of fluffy ice balls at low speeds, followed by violent gas release events on the comet.. November 12, 2014:. First-Ever Soft Landing on a Comet. (Comet 67P/. Churyumov-Gerasimenko. ). The Rosetta Mission. Launched in 2004: 10 Years in the Making. Graphic: . Time. Magazine, Nov. 17, 2014.