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Eugene Lanning
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 Project Jupiter
XIII-B. Processed Data Representation

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Abstract
I. Purpose
II. Background
III. Orbits
IV. Period  Determination
V. Methods
VI. Kepler's Laws
VII. Observing Suggestions
VIII. Data Gathering
IX. Data Processing
X. Observer's Data Results
XI. Other Quad-A Results
XII. Conclusions


This Project Jupiter Report was prepared by
Mizar Consulting
Eugene A. Lanning
130 Hillside Terrace
Nebraska City, NE
68410-3740
ealanni@alltel.net
Member of AAAA


AAAA
The American Association of Amateur Astronomers
P.O. Box 7981
Dallas, TX
75209-0981
e-Mail:
aaaa@astromax.com

www.AstroMax.com


Project Jupiter

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XIII. Attachments

Attachment B: Processed Data Representations

In this representation, the vertical distance is the observed distance of Callisto from the center of Jupiter. The red dots represent the distances recorded by Tim, and the blue line represents equation that best fits the data. One parameter of the equation is the period of the curve, and is the orbital period of Callisto. Tim’s observations yielded an equation period that has within10.5 minutes (0.0% difference) when compared to NASA data for Callisto of nearly 17 days!


In this representation, the vertical distance is the observed distance of Ganymede from the center of Jupiter. The red dots represent the distances recorded by Tim, and the orange line represents equation that best fits the data. On the graph the days on the x-axis represent the number of days since midnight on September 2, 2002 (GMT), the date that Tim logged his first JD estimate. Tim’s observations yielded an equation period that has a 0.6% difference when compared to NASA data for Ganymede!


In this representation, the vertical distance is position of Europa from the center of Jupiter. The red dots represent the distances recorded by Tim, and the pink line represents equation that best fits the data. Tim’s observations yielded an equation period that has 0.2% difference when compared to NASA data for Europa!


In this representation, the red dots represent the distances recorded by Tim, and the green line represents equation that best fits the data. To find the best equation for Jupiter’s moon Io requires that the observations be accurate. Tim’s observations yielded an equation period that has 0.1% difference when compared to NASA data for Io!


The next representation is concerning the distance from the red dots to the colored lines, i.e., how close the observations fit to the equations for the motions that were developed. In the below chart the observation-equation differences were placed into 0.36 JD wide groups. By far the largest number of observations are in the 0.33 JD group, meaning 11 of Tim’s 29 observations were accurate to between 0.54 and 0.18 JD. Tim attained a high degree of accuracy in estimating the Jupiter-moon separations. The observations outside the 0.33 and -0.03 JD groupings lie in a statistically expected pattern.


In the above representation Tim’s data for the moon Callisto is compared to observation data from four other Quad-A members, all data from the Fall of 2002. The observational data represented is from CCD measurements, Astrometric measurements and other observers using the JD estimating method. We have normalized the data to a consistent amplitude for comparison purposes. Tim’s JD estimates are very consistent with measurements taken by others. For this graph the zero days point is August 30, 2002, a change from other graphs in this section so that all available data can be represented.


[Home]
[Abstract]
[I. Purpose]
[II. Background]
[III. Orbits]
[IV. Period  Determination]
[V. Methods]
[VI. Kepler's Laws]
[VII. Observing Suggestions]
[VIII. Data Gathering]
[IX. Data Processing]
[X. Observer's Data Results]
[XI. Other Quad-A Results]
[XII. Conclusions]
[XIII. Attachments]
[Up]
[XIII-A. Data Sheets]
[XIII-B. Processed Data Representation]
[XIII-C. Press Release]
[XIII-D. Weighing Jupiter]
[XIII-E. Galileo Galilei Discovers Jupiter’s Moons]
[XIII-F. Practice JD estimating sessions]
[XIII-G. Earth-Jupiter Distance Effects]

 

The image of Jupiter on the Project Jupiter cover page is courtesy of AAAA member Charlie Warren of Texas. Used by permission. Jupiter and three of its moons - right to left are the moons Europa, Io and Ganymede. Callisto is not on the image. CCD Image taken February 2, 2002.

AAAA
The American Association of Amateur Astronomers
P.O. Box 7981
Dallas, TX 75209-0981
e-Mail: aaaa@astromax.com

www.AstroMax.com