Pulsar Timing: An Outer System Tool

by Paul Gilster on August 23, 2010

The ways astronomers find to wrest new findings from raw data never ceases to amaze me. This news release from the Max-Planck-Institut für Radioastronomie focuses on a new way to weigh the planets in our Solar System by using signals from pulsars. The method flows out of work on pulsar timing that has been used in the hunt for gravitational waves and has implications not just for the known planets but for detecting hitherto unknown objects in our system.

Pulsar timing supplements earlier ways of weighing planets by measuring their effect on spacecraft flown past them, or extrapolating information from the orbits of their moons. And it seems to be hugely sensitive, to just 0.003 percent of the mass of the Earth and one ten-millionth of Jupiter’s mass.

“This is first time anyone has weighed entire planetary systems – planets with their moons and rings,” says team leader Dr. David Champion (MPIfR). “In addition, we can provide an independent check on previous results, which is great for planetary science.”

So how does this work? The reception of pulsar signals is affected by the Earth’s movement around the Sun, an effect that can be removed by calculating when the pulsar signals would have reached the Solar System’s center of mass, or barycenter, which is the rotation center for all the planets. As you would imagine, the barycenter itself moves as the planetary positions change over time. An ephemeris charting the position of the planets can be used to work out the barycenter’s position according to the values for their masses that have been measured.

Any error in the calculation of the barycenter causes repeating timing errors in the pulsar data. Dick Manchester (CSIRO/Australia) says that “…if the mass of Jupiter and its moons is wrong, we see a pattern of timing errors that repeats over 12 years, the time Jupiter takes to orbit the Sun.” Correct the mass of Jupiter and its moons and the timing error disappears.

Image: Planets in the solar system with their masses determined by means of pulsar timing observations. Credit: David Champion.

Thus far the method has been used to weigh Mercury, Venus, Mars, Jupiter and Saturn (with moons and rings). The mass of the Jovian system can be calculated to a value far more accurate than the best Pioneer and Voyager spacecraft results, though not quite as accurate as the value measured by the Galileo spacecraft. Spacecraft will continue to be the best source of planetary weight measurements, but for planets not being probed by spacecraft, the pulsar measurement will provide accurate data, becoming more accurate as measurements are repeated over time.

This story takes us deep into the Solar System and involves more than the known planets. The kind of data being used may help us with a variety of unknown bodies. From the paper:

The pulsar timing technique is also sensitive to other solar system objects such as asteroids and currently unknown bodies, e.g., trans-Neptunian objects (TNOs). Measurements of anomalous period derivatives and binary period derivatives for a number of millisecond pulsars have already been used to place limits on the acceleration of the Solar System toward nearby stars or undetected massive planets… Pulsar timing array experiments with a wide distribution of pulsars on the sky will be sensitive to the dipolar spatial dependence resulting from any error in the solar system ephemeris, including currently unknown TNOs.

Thus exquisitely sensitive timing data gathered at Parkes, Arecibo and the German Effelsberg instrument, useful in the search for gravitational waves, opens up a new investigative tool for planetary measurement and the hunt for unknown bodies in our system. It’s easy to see why this emerged: The kind of tiny changes in pulsar timing that could flag gravitational waves has to be distinguished from timing error caused by objects in our Solar System. And this is interesting:

Limits for unknown masses have also been placed by spacecraft using deviations from their predicted trajectories. Doppler tracking data from the two Pioneer spacecraft were searched for accelerations due to an unknown planet. The anomalous acceleration detected in these data… is attributed to non-gravitational sources (Anderson et al. 2002) and is not detected in planetary measurements (Folkner 2010).

The paper is Champion et al., “Measuring the Mass of Solar System Planets Using Pulsar Timing,” to be published in The Astrophysical Journal. Also interesting (in terms of distributed science) is Knispel et al., “Pulsar Discovery by Global Volunteer Computing,” Science Express (12 August 2010). Abstract here.

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{ 7 comments }

Tulse August 23, 2010 at 15:25

How large would a TNO have to be to be detectable? Could this methodology identify possible Oort Cloud objects? How about neighbouring brown dwarfs? Or do objects have to have a small enough periodicity to their orbits to be detectable?

Michael Simmons August 23, 2010 at 22:27

>Or do objects have to have a small enough periodicity to their orbits to be detectable?

I imagine that without a number of orbits you can not detect the cyclic nature of the offset and calculate a correction.
So for Neptune you would need several 164 year orbits.
i.e. it would work but not in our lifetimes.

Having very accurate masses for Jupiter and Saturn might help in computing the cause of any detected disturbance in the outer solar system.

bigdan201 August 24, 2010 at 11:24

Cool! I always thought that pulsars would be a good tool for measurement, since they send out such regular signals. I remember reading that when pulsars were first discovered, scientists thought they had found ETI since the signal seemed so mechanical.

Is there any way that pulsars can be used to measure bodies in other solar systems?

Eniac August 24, 2010 at 23:22
Pointless Geometry August 31, 2010 at 0:50

Great to have another tool to find an earth-like planet. Look for a similar sun, similar gas giant planets and now a similar solar system mass; it all helps narrow the field.

walter b marvin September 5, 2010 at 17:11

I found three problems in Anderson’s analysis:

1) The time between inception of life and the rise of self awareness was glossed over. If we take earth’s experience, it took several billions of years for life to get to the complexity of intelligence in order for self awareness to blossom

2) He claims that over time, genetics or machines would break down due to replications errors. This problem has already been solved. It is commonly called RAID 1, RAID 2, RAID 3 etc. Basically data in redundantly stored and when retrieved, it is check and if nescessiary, repaired. Even if you insist on physical immortality, I can see a time in not the too distant future when even basic genitics would be redundantly coded.

3 He claims that there would be an information overload about discovered planets. But do we not now already live with information overloads, (e.g. the internet) I’m shure the most interesting information will get bandwidth, while less interesting stuff will be dropped.

Subzero Kari September 15, 2010 at 14:22

an interesting view of pulsar activity based on plasma experiments
http://public.lanl.gov/alp/plasma/downloads/HealyPeratt1995.pdf

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