Project
Jupiter
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.
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