Oumuamua – Non-Gravitational
Acceleration Observed but Probably not Alien Tech
Observation of Non-Gravitational Acceleration
A recent paper in Nature has shown (Non-gravitational acceleration in the trajectory of 1I/2017 U1 (‘Oumuamua)),
via a comprehensive analysis of multiple observations, that Oumuamua has
deviated from a purely gravitational track, on its way through the solar
system. In other words, its trajectory
has been influenced by some other push than the gravity of the major bodies of
the solar system. The effect is very
small, so it took a lot of observational data to detect the anomalous motion.
In the graph below, Oumuamua’s non-gravitational component
is shown, and can be compared to solar system bodies (it’s the black vertical
line). As you can see, it is within the
range for solar system comets, in this respect, though rather far into the right
tail of the distribution. So, relative
to “normal” solar system comets, its non-gravitational acceleration is actually
quite large, even if it is small in an absolute sense.
Just as a reminder, Oumuamua appeared in our skies in 2017,
and has been tracked with large ground-based telescopes as well as the Hubble
Space Telescope. Its velocity (26
km/second, which is more than the escape velocity from the solar system) and
trajectory (highly hyperbolic eccentricity=1.3) indicate that it must have
originated from outside of our solar system, probably from somewhere in the
constellation Lyra.
Lyra contains the bright star Vega, which is easy to find,
as it is one of the stars of the asterism The Summer Triangle. It is also an interesting coincidence for SF
fans that Vega is the star that was featured in the novel and movie “Contact”,
as the home planet of the alien civilization that sent the instructions to
build a wormhole device.
Some 177 ground-based and 30 space-based (Hubble)
observations were analysed, to determine Oumuamua’s track through the solar
system with great precision. Various
mathematical models were then produced, and compared to the actual data, using standard
statistical techniques, such as Chi-square goodness-of-fit tests.
The analysis showed that the arc of the body’s path could
not be explained by a solely gravitational model, even if the sun, eight
planets, moon, Pluto and the 16 largest asteroid were included in the model. Many of the observations deviated from
prediction by 3 to 5 standard deviations (about 35 in all did so). Furthermore, there appeared to be a clear
trend to the offsets, so this was not likely due to random observational
errors.
Below is a copy and paste graph from the paper, showing the
model residuals, using a purely gravitational model (a) vs a model that also
includes an extra push from some non-gravitational source (b). The residuals are what is left over after
subtracting the observational data points from the predictions of the model at the
location that those observations were made (in declination and right ascension,
which are sky coordinates somewhat similar to latitude and longitude). Basically, a good model will tend to have low
deviations from predictions, and the deviations will be randomly scattered
throughout the dataset. Using those
criterial, one can see that model b gives a better fit with observational data.
The model with the extra push includes a term that provides
a small positive impetus that varies with a 1/r**2 (or 1/r) term, with r being
distance from the sun. In other words,
the push is stronger when the body is closer to the sun, and it seems to vary
with something that falls off as one over R squared, as do radiation levels
from the sun.
Off-Gassing Explanation of Non-Gravitational Acceleration
So, does this mean that Oumuamua is actually a spacecraft of
some sort, under alien control? Not too
likely, according to the paper. Their hypothesis
is that Oumuamua is actually an extra-solar comet, rather than an extra-solar
asteroid, and that the slight non-gravitational changes in the object’s track
through our solar system are caused by off-gassing from the comet (primarily
the sublimation of water ice, carbon dioxide ice or carbon monoxide ice). The level of off-gassing will tend to fall
off with distance from the sun, as it is the sun’s radiation that produces the
off-gassing, and the strength of that falls off with distance, in a 1/R**2
manner.
Off-gassing and related dust basically creates the tail and/or
halo of a comet. By a simple application
of Newton’s laws, you can see that this off-gassing will also provide a push to
an object, much like a rocket does for a spacecraft (though obviously a much
smaller effect).
Some nice closeup pictures of a comet off-gassing were taken
by the ESA Rosetta probe, a few years ago.
Also shown, is an image of comet dust, as Rosetta made a close approach
to Comet 67/P.
One problem with this hypothesis, is that earlier
observations seemed to have ruled out the body being a comet. There had been no optical signs of a coma, dust,
nor spectroscopic evidence of gas emissions.
Basically, it looked like an inactive body, corresponding more to an
asteroid than a comet, when compared to objects native to our solar
system.
On the other hand, a comet always seemed like a more likely
explanation than an asteroid, as theory said that interstellar comets would be
brighter, and therefore easier to detect than interstellar asteroids. So there’s that.
So, why wasn’t the evidence of off-gassing and dust seen in
earlier optical and spectroscopic measurements?
One possibility for the lack of dust is that Oumuamua has an atypical dust-grain
size distribution, with fewer small dust particles than usual. Solar radiation pressure would thereby not be
able to create a significant dust halo, as large dust particles won’t be
affected much by solar radiation pressure.
It is also possible that Oumuamua simply had a low dust to ice ratio, so
there wasn’t much dust to create a dust halo.
Perhaps the long journey through interstellar space had produced this
low dust-ice ratio, via a thin isolating mantle or the journey had changed the
surface in some other relevant way.
Other Possible Explanations
Some other physical models that might produce a
non-gravitational acceleration were discussed.
For fun, I have included a Science Fiction possibility, which I have
called SF response, where possible:
- 1. Solar Radiation Pressure, such as that which drives a light-sail spacecraft. This was rejected on the basis that the object would have to have an unrealistically low density, three or four orders of magnitude lower than natural solar system objects.
- SF response – what if actually was a solar sail?
- 2. Yarkovsky Effect. This is another subtle effect, based on anisotropic thermal emission of photons from a rotating body. As with solar radiation, this effect is far too small to produce the acceleration detected.
- 3. Friction or Drag. Drag from collisions with small particles would tend to have a negative acceleration (slow Oumuamua down), whereas the observed acceleration was positive.
- 4. Single Impulsive Change in Velocity. An example of this would be a collision with some other solar system body (or the firing of a retro rocket :)). However, the observations seemed to indicate that the acceleration was constant and in a radial direction (away from the sun).
- SF response – what about the slow firing of a rocket, or other impulsive force (ion thruster?), perhaps energized by solar power, which would account for the 1 over R squared form of the acceleration?
- 5. Fragmented Object. If the object was fragmented, with the center of mass following a different trajectory than the detected (brighter) part of the object, it could appear to be following a non-gravitational track, while its center of mass was actually following a gravitational track. But no secondary object has been detected, and it would have to be very small to escape detection, which would mean it wouldn’t affect the apparent path enough to account for the observations.
- SF response – How about a small, reflective craft that left the mother ship?
- 6. Odd Surface Brightness. If one end of Oumuamua was very bright (and therefore detected) while the rest of the object was very dark, it could look as if Oumuamua was following a non-gravitational track. But it would have to be extremely long and thin for that effect to account for the observational discrepancies.
- SF Response - Oumuamua does appear to be very long and thin, more so than almost all natural bodies in our solar system (about 10 to 1). However, it still seems to be far too small to account for the anomalies.
- 7. Strong Magnetic Field. If Oumuamua had a very strong magnetic field, then interaction with the solar wind could change its motion. But that effect would be orders of magnitude too small (about 10,000 times), even if the object was fairly highly magnetized, for a natural body.
- SF Response - Interestingly enough, a ferromagnetic body (e.g. iron) has about 100,000 times more magnetic susceptibility than even the strongest magnetized rocks (according to my text of Applied Geophysics, by Telford et al). So, how about an inactive spacecraft, perhaps built into a natural body?
Summary
So, it appears that the enigmatic interstellar visitor is
best explained as a comet that was ejected from another solar system, somewhere
in the vicinity of Vega. But, its
peculiar elongated shape, and now its non-gravitational motion, render it a
fascinating object for speculation, whether scientific or science fiction.
Sources:
Non-gravitational acceleration in the trajectory of 1I/2017 U1 (‘Oumuamua),
Marco Micheli, et
al, Nature 27 June 2018
Applied Geophysics, Telford et al
Now that you
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The Zoo Hypothesis or The News of the World: A Science Fiction Story
Summary
In the field known as Astrobiology, there is a research program
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The Magnetic Anomaly
Summary
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