Wolfram Demonstrations Project
Astrophysics
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Demonstrations 21 - 40 of 105
Restricted Three-Body Problem in 3DBinding Energies of IsotopesEffective Potential of a Black Hole MetricTidal ForcesDixon Model for Magnetic Field of a Neutron Star
Restricted Three-Body Problem in 3D
Binding Energies of Isotopes
Effective Potential of a Black Hole Metric
Tidal Forces
Dixon Model for Magnetic Field of a Neutron Star
The Zeeman Effect in the Interstellar Medium2D Sine-Gaussian Lissajous FiguresBroadcasting Satellite in a Geocentric Kepler OrbitRelativistic Effects on Satellite Clock as Seen from EarthGravitational Redshift
The Zeeman Effect in the Interstellar Medium
2D Sine-Gaussian Lissajous Figures
Broadcasting Satellite in a Geocentric Kepler Orbit
Relativistic Effects on Satellite Clock as Seen from Earth
Gravitational Redshift
Gravitational Waves from Non-precessing Spinning Binary Black Hole CoalescenceGeodesics in Schwarzschild SpaceFitting an Ellipse to the Orbit of a Star near the Galactic CenterEarth's Magnetosphere and the Solar WindRestricted Three-Body Problem in a Plane
Gravitational Waves from Non-precessing Spinning Binary Black Hole Coalescence
Geodesics in Schwarzschild Space
Fitting an Ellipse to the Orbit of a Star near the Galactic Center
Earth's Magnetosphere and the Solar Wind
Restricted Three-Body Problem in a Plane
Egg-Shaped Orbits of Non-Uniform OscillatorsDoppler EffectPlanetary Tunnels with Coriolis EffectRadius and Temperature of Main Sequence StarsBlackbody Curves and Telescope Sensitivity
Egg-Shaped Orbits of Non-Uniform Oscillators
Doppler Effect
Planetary Tunnels with Coriolis Effect
Radius and Temperature of Main Sequence Stars
Blackbody Curves and Telescope Sensitivity

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