Dark matter: The stuff that possesses mass, yet refuses to interact with
radiation, so we can't 'see' it. Its nature has eluded scientists for
decades, but there could be a reservoir of the stuff sitting right on
our doorstep — if the weird measurements made by Global Positioning
System (GPS) satellites are proven to be caused by a halo of the
so-called non-baryonic matter around our planet
During a presentation at the American Geophysical Union (AGU)
conference in San Francisco in December, GPS expert Ben Harris (of the
University of Texas at Arlington) described some tricky measurements of
the Earth’s mass using the armada of GPS satellites that are in orbit
around our planet. He noticed a mass discrepancy when compared with
“official” mass measurements as quoted by the International Astronomical
Union (IAU).
“The nice thing about GPS satellites is that we know their
orbits really, really well,” said Harris. This orbital knowledge helped
Harris calculate the Earth’s vital statistic to a very high degree of
precision. After analyzing 9 months of data from the GLONASS, GPS and
Galileo satellite systems, he found that his measurement of Earth’s mass
came in at between 0.005 and 0.008 percent larger than the IAU
measurement.
What does this mean? Well, it could indicate some unforeseen
error in data collection or analysis (in the GPS or IAU measurements),
but there is another more intriguing possibility.
ANALYSIS: How Low Can a Dark Matter Halo Go?
This mass discrepancy could be the influence of a halo, or
ring, of dark matter surrounding Earth. By Harris’ reckoning, to explain
his measurements, the invisible planetary dark matter halo would need
to straddle the equator and be 191 kilometers (119 miles) thick by
70,000 kilometers (43,500 miles) wide.
As noted by New Scientist’s Anil Ananthaswamy, Harris has yet to factor in the effects of relativity and gravitational interactions with the sun and moon.
This research highlights the gaps in our knowledge dark matter.
Non-baryonic matter is believed to account for 85 percent of all matter
in the universe, but we have yet to directly observe this elusive form
of matter, let alone create it in immense particle accelerators like the
Large Hadron Collider. We know it’s out there, however, bulking-out
galactic clusters and warping spacetime. Through indirect means, such as
gravitational lensing and orbital motions, we can detect the stuff and
this most recent GPS measurements provide another tantalizing means of
understanding the subtle mass effects on a potential Earth-dark matter
coupling.
ANALYSIS: Dark Matter Matters, Especially When You Can’t Find It
Interestingly, the hypothetical presence of dark matter could
have another subtle effect on our planetary neighborhood. During
measurements of spacecraft flybys of Earth, very slight anomalies in
spacecraft speed have been detected. For example, NASA’s NEAR asteroid
spacecraft used our planet for a gravitational speed assist in January
1998. During the flyby, in addition to the extra velocity the flyby
provided, there was an additional mystery boost of 13
millimeters/second. This tiny boost, which has been spotted in other
spacecraft flybys, is known as a “flyby anomaly,” and one of the
contributing factors could be the gravity exerted on the spacecraft by
an invisible halo of dark matter.
The most recent flyby, however, of NASA’s Juno Jupiter mission in November, has yet to revel any velocity anomaly, only adding to the mysterious nature of flyby anomalies.
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