Near Earth Objects Near-Earth Objects (NEOs) are comets and asteroids that have been nudged by the gravitational attraction of nearby planets into orbits.

Slides:



Advertisements
Similar presentations
Chapter 8 Formation of the Solar System
Advertisements

Unt4: asteroid part 2. Comets Comet Ikeya-Seki in the dawn sky in 1965.
7.5 Other Objects In the Solar System (Pages ) Homework: Page 306 # 1, 3, 7, 8 Key Concepts: (Page 306)
Structure & Formation of the Solar System
MOST - Moving Object Search Tool for NEOWISE and IRSA Kevin Yau 6/11/2010.
Statistical Analysis of Near Earth Objects By Danielle Bisordi and Kristin Buckley Professor Florescu MA 331 December 3, 2009.
Solar System. What is the Solar System? Consists of a star, (like the sun) and all of the planets, moons and other bodies that travel around it. Planets.
Space Flight to the Stars. Celestial Objects “ Celestial” means sky Objects we can see in the sky such as the Sun, Moon, Earth and other planets are all.
Comets, Asteroids, and Meteors
Comets, Asteroids and Meteors
3 rd Grade. The Sun is a star. The Sun is the center of the solar system.
The Solar System Section 23.1 Pg
Class 2 : The Structure and Formation of the Solar System Basic constituents of the solar system The formation of the solar system What are the facts.
Solar System 3 rd Grade Katonya Beaubouef. Solar System The sun and all the objects that orbit around it.
Part 1: The evolution of the solar system. Origin of the Universe Lesson 1.
Vocabulary.  Our solar system includes the sun, the planets and many smaller objects.
National College Iasi Near Space Objects. National College Iasi Learn about NEOs Near-Earth Objects (NEOs) are comets, meteorids and asteroids that have.
WARM UP What two things determine the strength of an object’s gravitational force?
Astrophysics on the OSG (LIGO, SDSS, DES) Astrophysics on the OSG (LIGO, SDSS, DES) Kent Blackburn LIGO Laboratory California Institute of Technology Open.
Chapter 8, Astronomy. Identify planets by observing their movement against background stars. Explain that the solar system consists of many bodies held.
Solar System A group of objects in space that move around a central star.
An Introduction to Astronomy Part VI: Overview and Origin of the Solar System Lambert E. Murray, Ph.D. Professor of Physics.
The Origin of the Solar System Lecture 13. Homework 7 due now Homework 8 – Due Monday, March 26 Unit 32: RQ1, TY1, 3 Unit 33: RQ4, TY1, 2, 3 Unit 35:
JOURNAL #17 – THE SOLAR SYSTEM 1.What is the order of the planets from the Sun outward? 2.If during a solar eclipse the moon must be between the Sun and.
Solar Nebula Theory How to make a solar system: 1.Start with nebula = a large cloud of dust and gas. 2.A nearby star explodes (supernova) or the nebula.
Nothing travels faster than the speed of light.
Survey of the Solar System
Lecture Outlines Physical Geology, 14/e Copyright © The McGraw-Hill Companies, Inc. Permission required for reproduction or display. Plummer, Carlson &
THE SOLAR SYSTEM. The solar system Formed 4.6 billion years ago from a nebula a cloud of dust and gas The hot center from this nebula, shrinking and spinning,
The Solar System Science Third Grade The solar system is the sun and the objects that orbit around it.
TA19B –Teach About Planets, Asteroids, Meteors and Comets Use with BrishLab ES19B Done By: Coach.
Welcome to Science 12/13/10 Open your books to page and use these pages to begin completing the outline you just received. Today’s Schedule 1.
Big Bang theory Parts of our solar system Planet characteristics Galaxies Constellations Nebulas.
Created by, Morgan, Liz, Megan According to scientific theory, over fifteen thousand million years ago, the universe came into existence with a huge.
Survey of the Solar System. Introduction The Solar System is occupied by a variety of objects, all maintaining order around the sun The Solar System is.
Space Asteroids Raynaldo 6B.
Section 4 Minor Members of the Solar System
Universe Eighth Edition Universe Roger A. Freedman William J. Kaufmann III CHAPTER 7 Our Solar System CHAPTER 7 Our Solar System.
1 Ch. 23: “Touring Our Solar System” 23.4: “Minor Members of the Solar System”
14 billion years ago: start of the known universe… …but a rapid expansion of material known as the “Big Bang” Not really an “explosion”… The element ‘Hydrogen’
© 2010 Pearson Education, Inc. Formation of the Solar System.
Comets, Asteroids, and Meteors Section Standard  6.e. Students know the appearance, general composition, relative position and size, and motion.
 Meteoroid – a chunk of rock or dust in space. (these come from comets or asteroids)  Meteor – a chunk of rock or dust that enters our atomosphere and.
Formation of the Solar System
What causes day and night? (Please get this right…) What causes day and night? (Please get this right…) Do you see different stars at night here than you.
Planets, Solar Systems, and Galaxies…..Oh my!
The Solar System. The Solar System Contains: One star (the sun). Nine planets (well now there’s eight planets and 3 dwarf planets). 157 moons (at last.
EARTH IN SPACE. DAY AND NIGHT The Earth completes one rotation on its axis every 24 hours. The rotation of the Earth on its axis is responsible for day.
Chapter 8 Survey of Solar Systems
Solar System Formation Solar System Comprised of a star and the planets that orbit the star Binary – Two stars at center of system –Eclipsing is when.
2 nd Law of Thermodynamics 1 st Law – conservation of energy 2 nd Law – no cyclic process which converts heat entirely into work is possible. Can’t build.
Astronomy and Cosmology Where does the Earth fit in?
Comets, Asteroids, and Meteoroids Section Comets Loose collections of ice, dust, and small rocky particles whose orbits are usually very long, narrow.
What they are Where the are They and Us.  Comet – A body that produces a coma of gas and dust; a small, icy body that orbits the Sun  Made of ice and.
Solar System Video: 1 How it Formed.
Bodies in the solar system that orbit the Sun. Typically made of rock and metal but can also contain organic compounds.
Certain images included in this presentation fall under the Fair Use exemption of the U.S. Copyright Law. They have been prepared according to the educational.
Warmup  What is the line of latitude that cuts through the center of the earth?  What is ZERO degrees longitude?  What is 180 degrees longitude?
Introducing The Solar System WHAT’S IN IT? HOW DID IT FORM?
Formation of the Solar System Transparency for Activity From Messenger Activity.
The Asteroid Belt and Beyond!
Pegasus WMS Extends DAGMan to the grid world
“Don’t make me read, make me understand “
Survey of the Solar System
Our Solar System.
Chapter 2 Lesson 2 The Solar System
Characteristics of the Solar System
Dwarf Planets Spherical object that orbits the Sun
The Structure of the Solar System
Frieda meets Pegasus-WMS
Presentation transcript:

Near Earth Objects Near-Earth Objects (NEOs) are comets and asteroids that have been nudged by the gravitational attraction of nearby planets into orbits that allow them to enter the Earth's neighborhood. Composed mostly of water ice with embedded dust particles, comets originally formed in the cold outer planetary system while most of the rocky asteroids formed in the warmer inner solar system between the orbits of Mars and Jupiter. The scientific interest in comets and asteroids is due largely to their status as the relatively unchanged remnant debris from the solar system formation process some 4.6 billion years ago. 37 Near Earth Object candidates are identified in Sloan Digital Sky Survey imaging data. The objects have apparent magnitudes r=19 – 21 and proper motions of 1.3 to 18 degrees per day. The earth collision rate for this population (size greater than 20 m) is estimated to be one per century.

How To Find NEOs SDSS imaging data consist of 6 strips called “camcols”. The above image is a small portion of a “run” that extends for 800 fields. Camcols Fields Near Earth Objects show up as streaks in 3 colors

Why OSG ? Experience tells us that Grid is more suitable for CPU Intensive Jobs. Neo Jobs are Data Intensive but also need fair amount of CPU time. Also, to achieve PARALLELISM …  More Jobs…finish sooner  Running locally would limit the number of jobs run simultaneously  On OSG, can run several run-rerun and camcols within a run-rerun in parallel Current Workflow also will facilitate further analysis

Job Statistics Run-Rerun Avg: 150 Fields camcol 1camcol 2camcol3 camcol4camcol5 camcol6 6 Tar balls Avg: 1.5*6=9 GB Neo-$run-$camcol-Input.tar Neo-Executable 6 Neo Par Files Avg: 2*6=12 K neo-00$run-$camcol-$rerun.par Total Jobs 180 Total Input Data 9*180=1620 GB Total Output Data12*180=2160 K

OSG- Site SDSS Cluster TAM Cluster GFS DiskLocal Disk RLS Server on TAM VDL Generation VDL2XML Abstract DAX Creation Concrete DAG Creation Condor Submit DAG Compute Node Local Disk Register Input Files Query RLS to Create Condor Submit File NEO WORKFLOW Copy Input to Local Disk Copy Output Back Register Output Files Transfer Output Back to TAM

Future EAG Grid Projects… In the coming year Experimental Astrophysics Group ( EAG ) has 4 projects planned for the Open Science Grid  The simulation effort for the DES  Genetic algorithm fitting of SDSS quasar spectra  Search for near Earth asteroids in the SDSS imaging data  The coaddition of the SDSS southern stripe.  Thankyou