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ASTEROIDS@HOME
Project Asteroids@home. Asteroids@home is a volunteer distributed computing project developed at the Astronomical Institute, Charles University in Prague, in cooperation with Radim Vančo from CzechNationalTeam.The project is directed by Josef Durech.It runs on the Berkeley Open Infrastructure for Network Computing software platform and uses power of volunteers' computers to solve theASTEROIDS@HOME
Asteroids are small bodies of the solar system. Most of them orbit between Mars and Jupiter in the so-called main belt. Some of them, however, have orbits that come close to the Earth's orbit or even cross it. These are called near-Earth asteroids. Asteroids can be described as irregular solid bodies without any atmosphere or coma. ASTEROIDS@HOMESEE MORE ON ASTEROIDSATHOME.NETASTEROIDS@HOME
In total, about ~330,000 asteroids with enough data were processed in the framework of A@H. The number of data points per asteroid and their photometric quality in general decrease with the order number of asteroid (asteroids with higher numbers were discovered later). Therefore, we have much more models for asteroids with numbers <10,000 than
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FIND A TEAM
Find a team. Search criteria (use one or more) Key words. Find teams with these words in their names or descriptions. Country. --- None International Afghanistan Albania Algeria American Samoa Andorra Angola Anguilla Antarctica Antigua and Barbuda Argentina Armenia Aruba Australia Austria Azerbaijan Bahamas, The Bahrain Bangladesh Barbados ALL TASKS FOR COMPUTER 678180 Task click for details Show names Work unit click for details Sent Time reported or deadline explain Status Run time (sec) CPU time (sec)Credit
ASTEROIDS@HOMETRANSLATE THIS PAGE Projekt Asteroids@home. Asteroids@home je projekt distribuovaných výpočtů vyvinutý na Astronomickém ústavu Univerzity Karlovy v Praze ve spolupráci s Radimem Vančem z CzechNationalTeam.Projekt je veden Josefem Ďurechem.Projekt je založen na softwarové platformě Berkeley Open Infrastructure for Network Computing a využívá výpočetního výkonu počítačů ASTEROIDS@HOMETRANSLATE THIS PAGE Asteroidy typu M se nacházejí ve středních oblastech hlavního pásu. Jak je patrné, příliš slunečního světla žádný z typů asteroidů neodráží, což komplikuje jejich objevování a pozorování. Trojané (Trojans) - pás asteroidů, nacházející se přímo v prostoru oběžné dráhy Jupiteru (5,2 AU).ASTEROIDSATHOME.NET
Bctusbdu BtufspjetAipnf)iuuq;00btufspjetbuipnf/ofu*jtb wpmvouffs.dpnqvujoh qspkfduuibuvtftbo pqfo.tpvsdfCPJOD )CfslfmfzPqfo JogsbtusvduvsfgpsOfuxpslDpnqvujohASTEROIDS@HOME
Project Asteroids@home. Asteroids@home is a volunteer distributed computing project developed at the Astronomical Institute, Charles University in Prague, in cooperation with Radim Vančo from CzechNationalTeam.The project is directed by Josef Durech.It runs on the Berkeley Open Infrastructure for Network Computing software platform and uses power of volunteers' computers to solve theASTEROIDS@HOME
Asteroids are small bodies of the solar system. Most of them orbit between Mars and Jupiter in the so-called main belt. Some of them, however, have orbits that come close to the Earth's orbit or even cross it. These are called near-Earth asteroids. Asteroids can be described as irregular solid bodies without any atmosphere or coma. ASTEROIDS@HOMESEE MORE ON ASTEROIDSATHOME.NETASTEROIDS@HOME
In total, about ~330,000 asteroids with enough data were processed in the framework of A@H. The number of data points per asteroid and their photometric quality in general decrease with the order number of asteroid (asteroids with higher numbers were discovered later). Therefore, we have much more models for asteroids with numbers <10,000 than
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FIND A TEAM
Find a team. Search criteria (use one or more) Key words. Find teams with these words in their names or descriptions. Country. --- None International Afghanistan Albania Algeria American Samoa Andorra Angola Anguilla Antarctica Antigua and Barbuda Argentina Armenia Aruba Australia Austria Azerbaijan Bahamas, The Bahrain Bangladesh Barbados ALL TASKS FOR COMPUTER 678180 Task click for details Show names Work unit click for details Sent Time reported or deadline explain Status Run time (sec) CPU time (sec)Credit
ASTEROIDS@HOMETRANSLATE THIS PAGE Projekt Asteroids@home. Asteroids@home je projekt distribuovaných výpočtů vyvinutý na Astronomickém ústavu Univerzity Karlovy v Praze ve spolupráci s Radimem Vančem z CzechNationalTeam.Projekt je veden Josefem Ďurechem.Projekt je založen na softwarové platformě Berkeley Open Infrastructure for Network Computing a využívá výpočetního výkonu počítačů ASTEROIDS@HOMETRANSLATE THIS PAGE Asteroidy typu M se nacházejí ve středních oblastech hlavního pásu. Jak je patrné, příliš slunečního světla žádný z typů asteroidů neodráží, což komplikuje jejich objevování a pozorování. Trojané (Trojans) - pás asteroidů, nacházející se přímo v prostoru oběžné dráhy Jupiteru (5,2 AU).ASTEROIDSATHOME.NET
Bctusbdu BtufspjetAipnf)iuuq;00btufspjetbuipnf/ofu*jtb wpmvouffs.dpnqvujoh qspkfduuibuvtftbo pqfo.tpvsdfCPJOD )CfslfmfzPqfo JogsbtusvduvsfgpsOfuxpslDpnqvujohLOG IN
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CPU PERFORMANCE
CPU model Number of computers Avg. cores/computer GFLOPS/core GFLOPs/computer; Intel(R) Core(TM) i7-5775R CPU @ 3.30GHzFIND A TEAM
Find a team. Search criteria (use one or more) Key words. Find teams with these words in their names or descriptions. Country. --- None International Afghanistan Albania Algeria American Samoa Andorra Angola Anguilla Antarctica Antigua and Barbuda Argentina Armenia Aruba Australia Austria Azerbaijan Bahamas, The Bahrain Bangladesh BarbadosBOINC@TAIWAN
Team info; Description: For all BOINCers who love Taiwan. Created: 19 Jun 2012: Total credit: 434,631,960: Recent average credit: 283,701:Cross-project stats
ERROR TASKS FOR COMPUTER 679309 Task click for details Show names Work unit click for details Sent Time reported or deadline explain Status Run time (sec) CPU time (sec)Credit
WORKUNIT 146124122
Task click for details Computer Sent Time reported or deadline explain Status Run time (sec) CPU time (sec) Credit Application; 337795901:710230
ERROR TASKS FOR COMPUTER 670521 Task click for details Show names Work unit click for details Sent Time reported or deadline explain Status Run time (sec) CPU time (sec)Credit
CATHOLICS
log in: Catholics. Team info; Created: 24 Jul 2018: Web site: http://http:abortionno.com INVALID TASKS FOR COMPUTER 679309 Task click for details Show names Work unit click for details Sent Time reported or deadline explain Status Run time (sec) CPU time (sec)Credit
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ASTEROIDS@HOME
Project Asteroids@home. Asteroids@home is a volunteer distributed computing project developed at the Astronomical Institute, Charles University in Prague, in cooperation with Radim Vančo from CzechNationalTeam.The project is directed by Josef Durech.It runs on the Berkeley Open Infrastructure for Network Computing software platform and uses power of volunteers' computers to solve theASTEROIDS@HOME
Asteroids are small bodies of the solar system. Most of them orbit between Mars and Jupiter in the so-called main belt. Some of them, however, have orbits that come close to the Earth's orbit or even cross it. These are called near-Earth asteroids. Asteroids can be described as irregular solid bodies without any atmosphere or coma. ASTEROIDS@HOMESEE MORE ON ASTEROIDSATHOME.NETASTEROIDS@HOME
Asteroids@home - A BOINC distributed computing project for asteroid shape reconstruction (2015) Asteroid models derived so far: KWSN-Gemjunkie , ..:: Thor ::.. Here λ and β are ecliptic longitude and latitude of the spin axis direction and P is the rotation period. Usually, there are two possible pole directions andcorresponding shape
ASTEROIDS@HOME
In total, about ~330,000 asteroids with enough data were processed in the framework of A@H. The number of data points per asteroid and their photometric quality in general decrease with the order number of asteroid (asteroids with higher numbers were discovered later). Therefore, we have much more models for asteroids with numbers <10,000 than
FIND A TEAM
Find a team. Search criteria (use one or more) Key words. Find teams with these words in their names or descriptions. Country. --- None International Afghanistan Albania Algeria American Samoa Andorra Angola Anguilla Antarctica Antigua and Barbuda Argentina Armenia Aruba Australia Austria Azerbaijan Bahamas, The Bahrain Bangladesh BarbadosPROJECT STATUS
project1: IBM x3550 M4 (1 x Intel Xeon E5-2620 2.00 GHz, 96 (12 x 8) GB RAM (1333 MHz) 8 x 600 GB IBM SAS 10000 rpm (RAID5) OS Debian Jessie) project2: IBM x3550 M4 (1 x Intel Xeon E5-2620 2.00 GHz, 64 (4 x 16) GB RAM (1333 MHz) 3 x 600 GB IBM SAS 10000 rpm (RAID5) OS DebianJessie)
ASTEROIDS@HOMETRANSLATE THIS PAGE Projekt Asteroids@home. Asteroids@home je projekt distribuovaných výpočtů vyvinutý na Astronomickém ústavu Univerzity Karlovy v Praze ve spolupráci s Radimem Vančem z CzechNationalTeam.Projekt je veden Josefem Ďurechem.Projekt je založen na softwarové platformě Berkeley Open Infrastructure for Network Computing a využívá výpočetního výkonu počítačů ASTEROIDS@HOMETRANSLATE THIS PAGE Asteroidy typu M se nacházejí ve středních oblastech hlavního pásu. Jak je patrné, příliš slunečního světla žádný z typů asteroidů neodráží, což komplikuje jejich objevování a pozorování. Trojané (Trojans) - pás asteroidů, nacházející se přímo v prostoru oběžné dráhy Jupiteru (5,2 AU).ASTEROIDSATHOME
Bctusbdu BtufspjetAipnf)iuuq;00btufspjetbuipnf/ofu*jtb wpmvouffs.dpnqvujoh qspkfduuibuvtftbo pqfo.tpvsdfCPJOD )CfslfmfzPqfo JogsbtusvduvsfgpsOfuxpslDpnqvujohASTEROIDS@HOME
Project Asteroids@home. Asteroids@home is a volunteer distributed computing project developed at the Astronomical Institute, Charles University in Prague, in cooperation with Radim Vančo from CzechNationalTeam.The project is directed by Josef Durech.It runs on the Berkeley Open Infrastructure for Network Computing software platform and uses power of volunteers' computers to solve theASTEROIDS@HOME
Asteroids are small bodies of the solar system. Most of them orbit between Mars and Jupiter in the so-called main belt. Some of them, however, have orbits that come close to the Earth's orbit or even cross it. These are called near-Earth asteroids. Asteroids can be described as irregular solid bodies without any atmosphere or coma. ASTEROIDS@HOMESEE MORE ON ASTEROIDSATHOME.NETASTEROIDS@HOME
Asteroids@home - A BOINC distributed computing project for asteroid shape reconstruction (2015) Asteroid models derived so far: KWSN-Gemjunkie , ..:: Thor ::.. Here λ and β are ecliptic longitude and latitude of the spin axis direction and P is the rotation period. Usually, there are two possible pole directions andcorresponding shape
ASTEROIDS@HOME
In total, about ~330,000 asteroids with enough data were processed in the framework of A@H. The number of data points per asteroid and their photometric quality in general decrease with the order number of asteroid (asteroids with higher numbers were discovered later). Therefore, we have much more models for asteroids with numbers <10,000 than
FIND A TEAM
Find a team. Search criteria (use one or more) Key words. Find teams with these words in their names or descriptions. Country. --- None International Afghanistan Albania Algeria American Samoa Andorra Angola Anguilla Antarctica Antigua and Barbuda Argentina Armenia Aruba Australia Austria Azerbaijan Bahamas, The Bahrain Bangladesh BarbadosPROJECT STATUS
project1: IBM x3550 M4 (1 x Intel Xeon E5-2620 2.00 GHz, 96 (12 x 8) GB RAM (1333 MHz) 8 x 600 GB IBM SAS 10000 rpm (RAID5) OS Debian Jessie) project2: IBM x3550 M4 (1 x Intel Xeon E5-2620 2.00 GHz, 64 (4 x 16) GB RAM (1333 MHz) 3 x 600 GB IBM SAS 10000 rpm (RAID5) OS DebianJessie)
ASTEROIDS@HOMETRANSLATE THIS PAGE Projekt Asteroids@home. Asteroids@home je projekt distribuovaných výpočtů vyvinutý na Astronomickém ústavu Univerzity Karlovy v Praze ve spolupráci s Radimem Vančem z CzechNationalTeam.Projekt je veden Josefem Ďurechem.Projekt je založen na softwarové platformě Berkeley Open Infrastructure for Network Computing a využívá výpočetního výkonu počítačů ASTEROIDS@HOMETRANSLATE THIS PAGE Asteroidy typu M se nacházejí ve středních oblastech hlavního pásu. Jak je patrné, příliš slunečního světla žádný z typů asteroidů neodráží, což komplikuje jejich objevování a pozorování. Trojané (Trojans) - pás asteroidů, nacházející se přímo v prostoru oběžné dráhy Jupiteru (5,2 AU).ASTEROIDSATHOME
Bctusbdu BtufspjetAipnf)iuuq;00btufspjetbuipnf/ofu*jtb wpmvouffs.dpnqvujoh qspkfduuibuvtftbo pqfo.tpvsdfCPJOD )CfslfmfzPqfo JogsbtusvduvsfgpsOfuxpslDpnqvujohFIND A TEAM
Find a team. Search criteria (use one or more) Key words. Find teams with these words in their names or descriptions. Country. --- None International Afghanistan Albania Algeria American Samoa Andorra Angola Anguilla Antarctica Antigua and Barbuda Argentina Armenia Aruba Australia Austria Azerbaijan Bahamas, The Bahrain Bangladesh Barbados TOP HOSTS - ASTEROIDS@HOME Computer info Rank Owner Recent average credit Total credit BOINC version CPU GPU Operating system; ID: 466432 Details | Tasks: 1: Anonymous: 145,381.56: 25,208,160 ALL TASKS FOR COMPUTER 686851 Task click for details Show names Work unit click for details Sent Time reported or deadline explain Status Run time (sec) CPU time (sec)Credit
WORKUNIT 147130352
Task click for details Computer Sent Time reported or deadline explain Status Run time (sec) CPU time (sec) Credit Application; 339875153:713293
WORKUNIT 145840258
Task click for details Computer Sent Time reported or deadline explain Status Run time (sec) CPU time (sec) Credit Application; 337228160:622514
WORKUNIT 145955844
Task click for details Computer Sent Time reported or deadline explain Status Run time (sec) CPU time (sec) Credit Application; 337459528:652430
WORKUNIT 144770893
Task click for details Computer Sent Time reported or deadline explain Status Run time (sec) CPU time (sec) Credit Application; 334830803:222761
WORKUNIT 146079487
Task click for details Computer Sent Time reported or deadline explain Status Run time (sec) CPU time (sec) Credit Application; 337706847:519828
WORKUNIT 147136883
Task click for details Computer Sent Time reported or deadline explain Status Run time (sec) CPU time (sec) Credit Application; 339888642:652430
ERROR TASKS FOR COMPUTER 679309 Task click for details Show names Work unit click for details Sent Time reported or deadline explain Status Run time (sec) CPU time (sec)Credit
ASTEROIDS@HOME
Project Asteroids@home. Asteroids@home is a volunteer distributed computing project developed at the Astronomical Institute, Charles University in Prague, in cooperation with Radim Vančo from CzechNationalTeam.The project is directed by Josef Durech.It runs on the Berkeley Open Infrastructure for Network Computing software platform and uses power of volunteers' computers to solve theASTEROIDS@HOME
Asteroids are small bodies of the solar system. Most of them orbit between Mars and Jupiter in the so-called main belt. Some of them, however, have orbits that come close to the Earth's orbit or even cross it. These are called near-Earth asteroids. Asteroids can be described as irregular solid bodies without any atmosphere or coma. ASTEROIDS@HOMESEE MORE ON ASTEROIDSATHOME.NETASTEROIDS@HOME
In total, about ~330,000 asteroids with enough data were processed in the framework of A@H. The number of data points per asteroid and their photometric quality in general decrease with the order number of asteroid (asteroids with higher numbers were discovered later). Therefore, we have much more models for asteroids with numbers <10,000 than
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APPLICATIONS
Applications. Period Search Application. Platform. Version. Created. Average computing. Microsoft Windows (98 or later) running on an Intel x86-compatible CPU. 102.00 (cuda55) 10FIND A TEAM
Find a team. Search criteria (use one or more) Key words. Find teams with these words in their names or descriptions. Country. --- None International Afghanistan Albania Algeria American Samoa Andorra Angola Anguilla Antarctica Antigua and Barbuda Argentina Armenia Aruba Australia Austria Azerbaijan Bahamas, The Bahrain Bangladesh Barbados ASTEROIDS@HOMETRANSLATE THIS PAGE Projekt Asteroids@home. Asteroids@home je projekt distribuovaných výpočtů vyvinutý na Astronomickém ústavu Univerzity Karlovy v Praze ve spolupráci s Radimem Vančem z CzechNationalTeam.Projekt je veden Josefem Ďurechem.Projekt je založen na softwarové platformě Berkeley Open Infrastructure for Network Computing a využívá výpočetního výkonu počítačů ASTEROIDS@HOMETRANSLATE THIS PAGE Asteroidy typu M se nacházejí ve středních oblastech hlavního pásu. Jak je patrné, příliš slunečního světla žádný z typů asteroidů neodráží, což komplikuje jejich objevování a pozorování. Trojané (Trojans) - pás asteroidů, nacházející se přímo v prostoru oběžné dráhy Jupiteru (5,2 AU).ASTEROIDSATHOME
Bctusbdu BtufspjetAipnf)iuuq;00btufspjetbuipnf/ofu*jtb wpmvouffs.dpnqvujoh qspkfduuibuvtftbo pqfo.tpvsdfCPJOD )CfslfmfzPqfo JogsbtusvduvsfgpsOfuxpslDpnqvujohASTEROIDS@HOME
Project Asteroids@home. Asteroids@home is a volunteer distributed computing project developed at the Astronomical Institute, Charles University in Prague, in cooperation with Radim Vančo from CzechNationalTeam.The project is directed by Josef Durech.It runs on the Berkeley Open Infrastructure for Network Computing software platform and uses power of volunteers' computers to solve theASTEROIDS@HOME
Asteroids are small bodies of the solar system. Most of them orbit between Mars and Jupiter in the so-called main belt. Some of them, however, have orbits that come close to the Earth's orbit or even cross it. These are called near-Earth asteroids. Asteroids can be described as irregular solid bodies without any atmosphere or coma. ASTEROIDS@HOMESEE MORE ON ASTEROIDSATHOME.NETASTEROIDS@HOME
In total, about ~330,000 asteroids with enough data were processed in the framework of A@H. The number of data points per asteroid and their photometric quality in general decrease with the order number of asteroid (asteroids with higher numbers were discovered later). Therefore, we have much more models for asteroids with numbers <10,000 than
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APPLICATIONS
Applications. Period Search Application. Platform. Version. Created. Average computing. Microsoft Windows (98 or later) running on an Intel x86-compatible CPU. 102.00 (cuda55) 10FIND A TEAM
Find a team. Search criteria (use one or more) Key words. Find teams with these words in their names or descriptions. Country. --- None International Afghanistan Albania Algeria American Samoa Andorra Angola Anguilla Antarctica Antigua and Barbuda Argentina Armenia Aruba Australia Austria Azerbaijan Bahamas, The Bahrain Bangladesh Barbados ASTEROIDS@HOMETRANSLATE THIS PAGE Projekt Asteroids@home. Asteroids@home je projekt distribuovaných výpočtů vyvinutý na Astronomickém ústavu Univerzity Karlovy v Praze ve spolupráci s Radimem Vančem z CzechNationalTeam.Projekt je veden Josefem Ďurechem.Projekt je založen na softwarové platformě Berkeley Open Infrastructure for Network Computing a využívá výpočetního výkonu počítačů ASTEROIDS@HOMETRANSLATE THIS PAGE Asteroidy typu M se nacházejí ve středních oblastech hlavního pásu. Jak je patrné, příliš slunečního světla žádný z typů asteroidů neodráží, což komplikuje jejich objevování a pozorování. Trojané (Trojans) - pás asteroidů, nacházející se přímo v prostoru oběžné dráhy Jupiteru (5,2 AU).ASTEROIDSATHOME
Bctusbdu BtufspjetAipnf)iuuq;00btufspjetbuipnf/ofu*jtb wpmvouffs.dpnqvujoh qspkfduuibuvtftbo pqfo.tpvsdfCPJOD )CfslfmfzPqfo JogsbtusvduvsfgpsOfuxpslDpnqvujohAPPLICATIONS
Applications. Period Search Application. Platform. Version. Created. Average computing. Microsoft Windows (98 or later) running on an Intel x86-compatible CPU. 102.00 (cuda55) 10LOG IN
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PROJECT STATUS
Database schema version: 27013 Hosts project1: IBM x3550 M4 (1 x Intel Xeon E5-2620 2.00 GHz, 96 (12 x 8) GB RAM (1333 MHz) 8 x 600 GB IBM SAS 10000 rpm (RAID5) OS Debian Jessie) project2: IBM x3550 M4 (1 x Intel Xeon E5-2620 2.00 GHz, 64 (4 x 16) GB RAM (1333 MHz) 3 x 600 GB IBM SAS 10000 rpm (RAID5) OS Debian Jessie) Computing status TOP HOSTS - ASTEROIDS@HOME Computer info Rank Owner Recent average credit Total credit BOINC version CPU GPU Operating system; ID: 466432 Details | Tasks: 1: Anonymous: 145,381.56: 25,208,160CPU PERFORMANCE
CPU model Number of computers Avg. cores/computer GFLOPS/core GFLOPs/computer; Intel(R) Core(TM) i7-5775R CPU @ 3.30GHz ALL TASKS FOR COMPUTER 516899 Task click for details Show names Work unit click for details Sent Time reported or deadline explain Status Run time (sec) CPU time (sec)Credit
ALL TASKS FOR COMPUTER 670521 Task click for details Show names Work unit click for details Sent Time reported or deadline explain Status Run time (sec) CPU time (sec)Credit
Home | Project Asteroids@home| DAMIT database
| Basics about
asteroids | Scientific results PROJECT ASTEROIDS@HOME Asteroids@home is a volunteer distributed computing project developed at the Astronomical Institute , Charles University in Prague , in cooperation with RadimVančo from
CzechNationalTeam . The project is directed by Josef Durech. It
runs on the Berkeley Open Infrastructure for Network Computing (BOINC ) software platform and uses power of volunteers' computers to solve the lightcurve inversion problem formany asteroids.
WHY DISTRIBUTED COMPUTING? With huge amount of photometric data coming from big all-sky surveys as well as from backyard astronomers, the lightcurve inversion becomes a computationaly demanding process. In the future, we can expect even more data from surveys that are either already operating (PanSTARRS ) or under construction(Gaia , LSST
). Moreover, data from surveys are often _sparse in time_, which means that the rotation period - the basic physical parameter - cannot be estimated from the data easily. Contrary to classical lightcurves where the period is "visible" in the data, a wide interval of all possible periods has to be scanned densely when analysing sparse data. This fact enormously enlarges the computational time and the only practical way to efficiently handle photometry of hundreds of thousands of asteroids is to use distributed computing. Moreover, the problem is ideal for parallelization - the period interval can be divided into smaller parts that are searched separately and then the results are joined together. WHY TO STUDY ASTEROIDS? * The large discrepancy between the huge number of all known asteroids and the small number of those with known basic physical parameters (shape, spin, period) is a strong motivation for furtherresearch.
* Knowing the physical properties of a significant part of the asteroid population is necessary for understanding the origin and evolution of the whole solar system. * Thermal emission of small asteroids can significantly change their orbit (Yarkovsky efect ), which can be crucial for predicting the probability of their collision with the Earth. To be able to compute how the thermal emission affects the orbit, we have to know the spin (and also the shape, to a certain extent) of theobject.
SCIENTIFIC OBJECTIVES The aim of the project is to derive shapes and spin for a significant part of the asteroid population. As input data, we use any asteroid photometry that is available. The results are asteroid convex shape models with the direction of the spin axis and the rotation period. The models will be published in peer-reviewed journals and then madepublic in the DAMIT
database.
2017 Asteroids@homeDetails
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