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标题: 每日科技报告第106期 A New Way to Weigh Planets [打印本页]

作者: 张立涛 时间: 2010-10-24 14:41
标题: 每日科技报告第106期 A New Way to Weigh Planets
本帖最后由张立涛于 2010-10-24 14:42 编辑

A New Way to Weigh Planets

An international CSIRO-led team of astronomers has developed a new way to weigh the planets in our Solar System -- using radio signals from the small spinning stars called pulsars.

The Sun, Earth and Jupiter orbit a common barycentre. (Credit: D. Champion, MPIfR)

"This is first time anyone has weighed entire planetary systems -- planets with their moons and rings," said team leader Dr David Champion from Germany's Max-Planck-Institut für Radioastronomie.

"And we've provided an independent check on previous results, which is great for planetary science."

Measurements of planet masses made this new way could feed into data needed for future space missions.

Until now, astronomers have weighed planets by measuring the orbits of their moons or of spacecraft flying past them. That's because mass creates gravity, and a planet's gravitational pull determines the orbit of anything that goes around it -- both the size of the orbit and how long it takes to complete.

The new method is based on corrections astronomers make to signals from pulsars -- small spinning stars that deliver regular 'blips' of radio waves.

The Earth is travelling around the Sun, and this movement affects exactly when pulsar signals arrive here.

"This is first time anyone has weighed entire planetary systems -- planets with their moons and rings," says Dr David Champion from Germany's Max-Planck-Institut für Radioastronomie.

To remove this effect, astronomers calculate when the pulses would have arrived at the Solar System's centre of mass, or barycentre, around which all the planets orbit.

Because the arrangement of the planets around the Sun changes all the time, the barycentre moves around too.

To work out its position, astronomers use both a table (called an ephemeris) of where all the planets are at a given time, and the values for their masses that have already been measured.

CSIRO Astronomy and Space Science (CASS) researcher, Dr Dick Manchester, says that if these figures are slightly wrong, and the position of the barycentre is slightly wrong, then a regular, repeating pattern of timing errors appears in the pulsar data.

"For instance, 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," Dr Manchester said.

"But if the mass of Jupiter and its moons is corrected, the timing errors disappear. This is the feedback process that the astronomers have used to determine the planets' masses."

Data from a set of four pulsars have been used to weigh Mercury, Venus, Mars, Jupiter and Saturn with their moons and rings. Most of these data were recorded by CSIRO's Parkes radio telescope in eastern Australia, with some contributed by the Arecibo telescope in Puerto Rico and the Effelsberg telescope in Germany.

The masses were consistent with those measured by spacecraft. The mass of the Jovian system, 9.547921(2) x 10-4 times the mass of the Sun, is significantly more accurate than the mass determined from the Pioneer and Voyager spacecraft, and consistent with, but less accurate than, the value from the Galileo spacecraft.

The new measurement technique is sensitive to a mass difference of two hundred thousand million million tonnes -- just 0.003 per cent of the mass of the Earth, and one ten-millionth of Jupiter's mass.

CASS scientist Dr George Hobbs says that, in the short term, spacecraft will continue to make the most accurate measurements for individual planets.
"But the pulsar technique will be the best for planets not being visited by spacecraft, and for measuring the combined masses of planets and their moons," Dr Hobbs said,

Repeating the measurements would improve the values even more. If astronomers observed a set of 20 pulsars over seven years they'd weigh Jupiter more accurately than spacecraft have. Doing the same for Saturn would take 13 years.

The head of the 'Fundamental Physics in Radio Astronomy' research group at the Max-Planck-Institut für Radioastronomie, Professor Michael Kramer, says astronomers need this accurate timing because they are using pulsars to hunt for gravitational waves predicted by Einstein's general theory of relativity.

"Finding these waves depends on spotting minute changes in the timing of pulsar signals, and so all other sources of timing error must be accounted for, including the traces of Solar System planets," Professor Kramer said.

作者: 画个圈圈 时间: 2010-10-24 15:40
好啊顶~~~~~~~~~~~~~~~~~~~~~~~~~

作者: 1124629740 时间: 2010-10-24 15:51

作者: moonandwind604 时间: 2010-10-24 16:05
基于脉冲星（以有规律的周期发出无线电波的一种小天体）
相关知识：
（摘自大英百科）
脉冲星从表面发出的带电粒子进入星体磁场，磁场将它们加速，使得它们产生辐射，从磁极处以强粒子束释放出来。辐射束的方向与脉冲星自转轴方向不一致，因此当星体自旋时，辐射束像灯塔般来回摆动，看起来就像是脉冲。已经证明无线电脉冲星一直在减速，典型的减慢速度为每年百万分之一秒。经计算得知约1,000万年后当脉冲星的磁场变得足够弱时，脉冲星就会“熄灭”。

作者: phinlot 时间: 2010-10-25 13:31