Data Analysis on Contour Probe Marisa Briones Milton Diaz Maurice Fernandez Danny Gunawan Project • Overview on Contour Probe • Compute the distances of the perigee and apogee to the center of the earth • Simulate trajectory of the probe • Design a sequence of speed changes in the apogee and perigee which will result in a circular orbit of radius 100,000 km. Mission NASA’s Contour Probe To explore the nucleus of two, possibly three comets. Probe and Comet Contour Probe INSTRUMENTS Four scientific instruments will take images and spectral maps of the nucleus of comets and analyse the surrounding gas and dust, providing the most detailed data on these mysterious, dynamic, and ancient keepers of the solar systems original material. Contour Remote Imaging Spectrograph (CRISP) Contour Forward Imager (CFI) The Neutral Gas and Ion Mass Spectrometer The Neutral Gas and Ion Mass Spectrometer will measure the abundance and isotope ratios for many neutral and ion species in the coma of each comet during the flyby Contour Dust Analyzer (CIDA) Contour Dust Analyzer (CIDA) The mission plan called for the probe to meet up with comet Encke in 2003, Schwassman-Wachmann 3 in 2006 and perhaps comet d'Arrest in 2008. • Launch: July 3, 2002 at 2:27 a.m. EDT Lost Aug. 15, 2002 Scientists believe this picture shows Contour broken in two pieces Equations • • • • • • • • x=rcosf y=rsinf h=(GMa(1-e^2))^.5 p=a(1-e^2) r=p/(1+e) x*=(-h/p)sinf y*=(h/p)(e+cosf) r=(x^2+y^2)^.5 • v=(vx^2+vy^2)^.5 • v=(GM/a(1-e^2))^.5 *(1+e^2+2ecosf)^.5 • at apogee f = 180 • at perigee f = 0 • final velocity v=(2GM/r)^.5 where r=100,000km Calculations Using the orbital elements we calculated the following in 1,000km/1,000s: • • • • • • • • T=150s M=6.2262rad E=5.8603 f=4.8213 r=11.365km p=1.2466km h=70491km e = 0.8915936 • • • • • • x=.81547km y=9.8432km z=-5.6222km vx=-6.519km/s vy=-4.2446km/s vz=1.7541km/s Apogee & Perigee • • • • apogee=p/(1-e)=115km perigee=p/(1+e)=6.5902km distances to the center of the earth: apogee - radius of earth = 115km - 6.378km = 108.6 km • perigee - radius of earth = 6.5902km 6.378km = .212 km Orbital Simulation • Using Dr. Varadi’s Orbital Simulation Software we investigated the trajectory of the Contour Probe. • We used the original x, y, z values and velocity values to simulate an orbit but the software did not produce an orbit. • We set y, z, vx, vz equal to 0 and the values for x & y equal to: x=apogee & Vy=v=(GM/a(1e^2))^.5*(1+e) • • x=-115 km y=0 Vx=0 Vy=-0.33825 km/s • z=0 Vz=0 Sequence of Speed Changes • • • • We used the planar values for x, y, z, vx, vy, vz. x=1.2353km y=11.298 km z=0 vx=5.6212 km/s vy=5.6563 km/s vz=0 We decreased the planar values for vx & vy by 97.2% because the absolute values were larger than the escape velocity of the earth, which is 7.9km/s: vx=0.15739 km/s vy=0.15838 km/s • At the apogee we increased the velocity through a sequence of speed changes to create new perigees and apogees until the ellipse had a radius of 100,000 km. Sequences • vx=0.01km/s • vy=-0.4km/s • We tripled the initial values: • vx=0.03km/s • vy=-0.12km/s • We did a 25% increase: • vx=0.0325km/s • vy=-0.13km/s • We did a 0.65% decrease: • vx=0.032435km/s • vy=-0.1274km/s • These velocities gave the absolute values of x and y to equal to a radius of 100,000 km. Vx = -0.0484 Vy = 0.02488 Circular Orbit of Radius 100,000 km • When we reached an ellipse with the absolute value of x and y equal to 100,000 km, we tried to create a circular orbit with this radius. The final velocity according to the equation: v=(2GM/100)^.5 is 0.089286 km/s. • We took the absolute value of v x and vy and divided the final velocity by this value to get k=1.63972. Final Values • • • • x= -87.2773528989 km y=-50.5478705216 km By trial and error: vx= -0.037164 km/s By k * vy: vy=0.04081 km/s Conclusion • The contour probe was lost August 15, 2002. • From its orbital elements, there was no true orbit. • Through a sequence of speed changes, a circular orbit of radius 100,000 km can be simulated, but still problems with the software do not produce the correct simulation. Acknowledgments • Dr. Horn • Dr. Varadi • Dr. Shubin