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Naar Contents Back to Part 5 To Part 7 Comet Oumuamua 6 Application to the Pioneers In March 1972, the Pioneer 10
spacecraft was launched. Just over a year later – in April 1973 – Pioneer
11 followed. Both described orbits in the plane of the ecliptic, which took
them past Jupiter and other planets, ultimately leaving our solar system in
opposite directions. They
generated a vast amount of research data about the solar system. One of the
goals of the projects was to better understand the gravitational field in the
solar system. The measurements of the spacecraft's accelerations were
exceptionally precise, measuring them with an accuracy of 10–10
m/s2. However, this precision presented a new problem that remains
unresolved.
The measured anomalous
acceleration of the Pioneer is found by adding the acceleration the
Pioneer experiences due to the anomalous acceleration in the sun's
gravitational field, measured from Earth, to the acceleration the Earth
experiences in the opposite direction, as seen from the Pioneer. This
therefore occurs between Earth and the spacecraft.
Together, this should yield 9.44x10–10
m/s² near Jupiter. However, measurements near Jupiter could not yet be
performed because the manoeuvres were still ongoing.
If we limit ourselves to Newtonian gravitational acceleration, we can
derive Pioneer's acceleration from the calculations by subtracting the
acceleration experienced by the Earth relative to the Sun from Pioneer's
measured acceleration. This yields Pioneer's gravitational acceleration. However, the measurements measure not only the normal gravitational
acceleration, but also the anomalous acceleration. Therefore, to find
Pioneer's acceleration, we must also subtract the anomalous acceleration from
the measurements. If we don't do this, the correction is insufficient we are
left with the sum of the anomalous accelerations at Pioneer and Earth. That's the mistake NASA made. Therefore, at the end of the calculation,
they should find an acceleration of Pioneer of at least 9.37x10–10
m/s² towards Earth. The reason the anomalous acceleration wasn't noticed until beyond Jupiter
is likely related to the occasional accelerations Pioneer had to undergo
before reaching Jupiter to steer it in the right direction. This prevented a
usable, continuous series of measurements. Beyond Jupiter, this was possible,
but initially, no anomaly was found. This can be explained by the fact that the Pioneer was steered past
Jupiter in such a way that it could make optimal use of the speed gain due to
Jupiter's gravitational assistance. This velocity gain is optimal when the Pioneer is flung away in a
tangential direction relative to the distance r from the sun. The
measured radial velocity relative to the Earth at j
=90 degrees is zero at that moment. The Pioneer then no longer has any radial
velocity relative to the Earth, so the anomalous velocity and anomalous
acceleration can not occur. Pioneer's acceleration measurement then yields the
traditional value of the sun's gravitational field at that location. The
anomalous acceleration is then zero.
Fig.
2 The orbits that the Pioneers described in the solar system
The sharp angles that the orbits exhibit upon encountering Jupiter are
the result of the orbit being deflected by Jupiter's gravitational pull, which
also results in a gain in speed. The result of the calculations is also shown in a graph (Fig
3).
Table 1 The anomalous acceleration at the distances
beyond Jupiter .
Figure
3 The anomalous acceleration of Pioneer 10 in the solar system according to
the obstruction theory
Figure
4 The anomalous acceleration as measured on Pioneers 10 and 11 |