n.33 dvorak captured-trojans
DESCRIPTION
Talk of the "International Workshop on Paolo Farinella (1953-2000): the Scientists, the man", Pisa, 14-16 June 2010TRANSCRIPT
International Workshop on Paolo FARINELLA
Pisa, 14-16 June 2010
Rudolf Dvorak and Richard Schwarz Rudolf Dvorak and Richard Schwarz AstroDynamicsGroupAstroDynamicsGroup
Institute for Astronomy, University of ViennaInstitute for Astronomy, University of Vienna
C A P T U R E D
T R O J A N S
Trojans are asteroids known to orbit around the Lagrange points of a planet:
We observe Trojans around
Jupiter and Neptune and also Mars
(5261) Eureka 1990 MB L5 1.425 1.622 1998 VF31 L5 1.371 1.677 1999 UJ7 L4 1.465 1.584 2007 NS2 L5 1.441 1.606
2001 QR322 L4 29.404 31.330 2004 UP10 L4 29.354 31.209 2005 TN53 L4 28.252 32.236 2005 TO74 L4 28.727 31.782 2006 RJ103 L4 29.320 30.975 2007 VL305 L4 28.132 32.105
L4 point = 2603 L5 point = 1473. JUPITER:
NEPTUNE:
MARS:
The five Lagrange points SUN + PLANET
x
Eccentricity of the primaries: 0.05, 0.1, 0.2, 0.3
Thersites is jumping from L_5
to L_4
I could not find any other orbit having such interesting
dynamics
Can the terrestrial planets
Venus, Earth and Mars capture Trojans ?
N-body simulations in the Newtonian dynamical model
Sun, Venus –
Saturn + 100 massless asteroids
4 different regions
Regions a (VeTe): 0.72 < a < 0.98
Regions b (TeMa): 1.02 < a < 1.50
Regions c (MaJu1): 1.54 < a < 2.20
Regions d (MaJu2): 2.2 < a < 2.5
0
50
100
150
200
1 2 3 4 5semimajor axis [AU]
Mercury Venus Earth Mars Jupiter
3:1 8:3
5:2
1:1
3:2Hildas
Trojans
2:1
4:1
Hungarias
ATENs AMORsAPOLLOs
NEAs
Near Earth Asteroids and mainbelt asteroids
a b dc
N-body simulations in the Newtonian dynamical model
Sun, Venus –
Saturn + 100 massless fictitious asteroids
Regions a (VeTe): 0.72 < a < 0.98
For different inclinations 0<i<20 degrees
For some selected orbits for verifications –
MeNe
100 fictitious Trojans between Venus and the Earth
100 fictitious asteroids between Venus and Earth for 10^7 years
Capture into 1:1 MMR ?
100 fictitious asteroids between Venus and Earth for 10^7 years
Capture into 1:1 MMR ?
Test for capture into the 1:1 MMR with Venus for the 100 asteroids
Venus captures into Trojans
L_4
L_5 HORSESHOE
360 deg
0
360 deg
0
360 deg
0
360 deg
0 degree
Captures by the EARTH360 deg
0 degree
L5-Trojan->L4-Trojan->Horshoe-orbit->escape
Conclusions (Work in progress)
- Captures into the 1:1 MMR for Venus, Earth and Marsare not rare events
- Captures into Trojan orbits also are possible but not so often
Jumping orbits are to observe for all terrestrial planets
- For larger inclinations more captures
Results only for region between Venus and Earth
Goal:
statistics about captures for all 4 regions dependant on inclination and eccentricities
Statistics of jumps and duration of a capture