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6 409 (0,127s) •

Project

Early dynamics of planets and analysis of asteroid populations (GA25-16507S)

also plan to study populations of Trojans, Hilda and Thule asteroids, resonantly coupled to Jupiter. Explaining their striking differences may shed light onto Jupiter's late orbital evolution, and/or these pop...

Astronomy (including astrophysics,space science)

  • 2025 - 2027
    • •
  • 10 555 tis. Kč
    • •
  • 9 583 tis. Kč
    • •
  • GA ČR
Project

Chaos and resonances in the dynamics of asteroids (GA205/02/0969)

-body resonances Jupiter-asteroid-Saturn, but also in resonances with Mars. More of the Kirkwood gaps in the asteroid belt located at orbital resonances of low orders with Jupiter as the ...

BN - Astronomie a nebeská mechanika, astrofyzika

  • 2002 - 2004
    • •
  • 1 350 tis. Kč
    • •
  • 372 tis. Kč
    • •
  • GA ČR
Project

The origin of asteroids inside gravitational resonances and the dynamics of meteoroids with the Yarkovsky/YORP effect included (GP205/08/P196)

Stable populations of asteroids, which are influenced by gravitational resonances with Jupiter, are important source of information about the evolution of the whole Solar System. Their origin, observed distribution...

BN - Astronomie a nebeská mechanika, astrofyzika

  • 2008 - 2010
    • •
  • 558 tis. Kč
    • •
  • 558 tis. Kč
    • •
  • GA ČR
Project

The Yarkovsky and YORP effects in translational and rotational motion of asteroids (GA205/05/2737)

Orbital and rotational motion of asteroids has been thought for a long time nongravitationa]effects played important role in the past evolution of the asteroid belt. Structure of asteroid families, asteroid

BN - Astronomie a nebeská mechanika, astrofyzika

  • 2005 - 2007
    • •
  • 667 tis. Kč
    • •
  • 667 tis. Kč
    • •
  • GA ČR
Project

The Yarkovsky and YORP effects in translational and rotational dynamics of asteroids (GA205/08/0064)

Orbital and rotational motion of asteroids has been thought for a long time to be a pure example of massless(test)-bodies dynamics in gravitational field of planets. During the last decade, however, novel ideas arose indicating that...

BN - Astronomie a nebeská mechanika, astrofyzika

  • 2008 - 2012
    • •
  • 1 501 tis. Kč
    • •
  • 1 501 tis. Kč
    • •
  • GA ČR
Project

The effect of resonances on the asteroid belt structure (GA205/95/0184)

BN - Astronomie a nebeská mechanika, astrofyzika

  • 1995 - 1997
    • •
  • 332 tis. Kč
    • •
  • 332 tis. Kč
    • •
  • GA ČR
Project

Regular and chaotic trajectories in the asteroid belt (GA205/98/1102)

The study of chaos for the asteroids in the asteroid belt. The possibilities applied to asteroidal orbits. At least seven planets will be taken into account in numerical integration of asteroidal orbits. Results wi...

BN - Astronomie a nebeská mechanika, astrofyzika

  • 1998 - 2000
    • •
  • 623 tis. Kč
    • •
  • 364 tis. Kč
    • •
  • GA ČR
Project

Mapping the asteroid population - physical models of asteroids from sparse photometric data (GP205/07/P070)

part of the asteroid population is to use photometric data from all-sky asteroid-STARRS is the asteroid photometric and astrometric survey project of the University of asteroids, the first observations ar...

BN - Astronomie a nebeská mechanika, astrofyzika

  • 2007 - 2009
    • •
  • 669 tis. Kč
    • •
  • 669 tis. Kč
    • •
  • GA ČR
Project

Properties of meteoroids from different classes of parent bodies (GAP209/11/1382)

-asteroid transition objects? Is comet 2P/Encke a Jupiter family comet by origin? What on asteroidal orbits in different size ranges?......

BN - Astronomie a nebeská mechanika, astrofyzika

  • 2011 - 2015
    • •
  • 7 684 tis. Kč
    • •
  • 7 684 tis. Kč
    • •
  • GA ČR
Project

Thermal effects in the orbital and rotational dynamics of small solar systém bodies (GA205/02/0703)

in the long-term dynamics of small solar system objects (meteoroids, small asteroids) understanding originof the small near-Earth asteroids, iii) modeling the long-term diffusion processes in the asteroid families, and/or ...

BN - Astronomie a nebeská mechanika, astrofyzika

  • 2002 - 2004
    • •
  • 946 tis. Kč
    • •
  • 496 tis. Kč
    • •
  • GA ČR
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