aegis 2008 annual assembly 11 december 2008 propel – asteroid proper elements bojan novaković and...

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A c a d e m i c a n d E d u c a t i o n a l G r i d I n i t i a t i v e o f S e r b i a A E G I S AEGIS 2008 Annual Assembly 11 December 2008 PROPEL – Asteroid proper elements Bojan Novaković and Zoran Knežević Astronomical Observatory Belgrade Serbia bnovakovic @aob.bg.ac. yu , zoran @ aob . bg .ac. yu

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Page 1: AEGIS 2008 Annual Assembly 11 December 2008 PROPEL – Asteroid proper elements Bojan Novaković and Zoran Knežević Astronomical Observatory Belgrade Serbia

Acad

em

ic a

nd E

ducat ional Gr id Init iat ive o

f Serbia

A E G I S

AEGIS 2008 Annual Assembly

11 December 2008

PROPEL – Asteroid proper elements

Bojan Novaković and Zoran Knežević

Astronomical Observatory Belgrade

Serbia

[email protected], [email protected]

Page 2: AEGIS 2008 Annual Assembly 11 December 2008 PROPEL – Asteroid proper elements Bojan Novaković and Zoran Knežević Astronomical Observatory Belgrade Serbia

A E G I S

11 December 2008

PROPEL – Asteroid proper elements

Proper elements are quasi integrals of N-body equations of motion. They are nearly constant in time and represent average characteristics of motion over very long time spans, up to hundreds of millions of years. They are used to:

study long term dynamical evolution of asteroids study evolution of the asteroid belt through their classification

into the collisional families assess the stability of their motion identify transport mechanisms at work in the Solar system.

Page 3: AEGIS 2008 Annual Assembly 11 December 2008 PROPEL – Asteroid proper elements Bojan Novaković and Zoran Knežević Astronomical Observatory Belgrade Serbia

A E G I S

11 December 2008

Importance of Grid for PROPEL

Why grid makes a difference for PROPEL? Computation of asteroid proper elements

requires numerical integrations of thousands of orbits over time spans on the order of millions of years. This is computationally complex, CPU intensive and time consuming procedure. Since it can be simply parallelized by grouping similar orbits into independent batches, it is perfectly suitable for the grid.

The need to speed up the time consuming computations and make them more efficient is justified by the large increase of observational data expected from the next generation all sky surveys.

Page 4: AEGIS 2008 Annual Assembly 11 December 2008 PROPEL – Asteroid proper elements Bojan Novaković and Zoran Knežević Astronomical Observatory Belgrade Serbia

A E G I S

11 December 2008

Gridification topics

Software Installation Management Running Jobs Data Management Data Access Application-Level Monitoring  Benchmarking Installation of appropriate FORTRAN compiler Optimisation for platforms based on both AMD

and Intel Processors Preparation of SEE-GRID-2 wiki pages about

Software installation management Execution and data collecting automation

Launching of PROPEL web site

Page 5: AEGIS 2008 Annual Assembly 11 December 2008 PROPEL – Asteroid proper elements Bojan Novaković and Zoran Knežević Astronomical Observatory Belgrade Serbia

A E G I S

11 December 2008

PROPEL statistics

Page 6: AEGIS 2008 Annual Assembly 11 December 2008 PROPEL – Asteroid proper elements Bojan Novaković and Zoran Knežević Astronomical Observatory Belgrade Serbia

A E G I S

11 December 2008

AstDys databaseScreenshot of the AstDys’ statistics: country of visitors’ origin and number of visits.http://hamilton.dm.unipi.it/astdys/

Page 7: AEGIS 2008 Annual Assembly 11 December 2008 PROPEL – Asteroid proper elements Bojan Novaković and Zoran Knežević Astronomical Observatory Belgrade Serbia

A E G I S

11 December 2008

List of contributors

Zoran Knežević Bojan Novaković Branko Marović Milan Potočnik Branimir Acković Antun Balaž Vladimir Bajčeta Edi Bon