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The
image shows an impression by David A. Hardy of a possible scene from a
moon orbiting the extra-solar planet in orbit around the star HD70642.
The planet has a mass about twice that of Jupiter and orbits the star
in roughly six years, with a nearly circular orbit of more than three
times the Earth-Sun distance. The star HD70642 is a 7th magnitude star
in the southern constellation Puppis, and has properties very similar
to that of our sun. The similarity in appearance of the extra-solar
planet to Jupiter arises because the planets have a similar mass. The
possible existence of the moons has been inferred from our knowledge of
the planets in our own solar system and from theories of planetary
formation—they have not actually been detected.
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The ‘orbit’ diagram shows the size and shape of the
star HD70642 orbit compared with the orbits of planets in our own Solar
System
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Illustration of the
Doppler Wobble Technique.
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Astronomers looking for planetary systems
that resemble our own solar system have found the most similar formation
so far. British astronomers, working with Australian and American
colleagues, have discovered a planet like Jupiter in orbit round a
nearby star that is very like our own Sun. Among the hundred found so
far, this system is the one most similar to our Solar System. The
planet’s orbit is like that of Jupiter in our own Solar System,
especially as it is nearly circular and there are no bigger planets
closer in to its star.
“This planet is going round in a nearly circular orbit three-fifths
the size of our own Jupiter. This is the closest we have yet got to a
real Solar System-like planet, and advances our search for systems that
are even more like our own,” said UK team leader Hugh Jones of Liverpool
John Moores University.
The planet was discovered using the 3.9-metre Anglo-Australian
Telescope [AAT] in New South Wales, Australia. The discovery, which is
part of a large search for solar systems that resemble our own, will be
announced today (Thursday, July 3rd 2003) by Hugh Jones (Liverpool John
Moores University) at a conference on “Extrasolar Planets: Today and
Tomorrow” in Paris, France.
“It is the exquisite precision of our measurements that lets us
search for these Jupiters – they are harder to find than the more exotic
planets found so far. Perhaps most stars will be shown to have planets
like our own Solar System”, said Dr Alan Penny, from the Rutherford
Appleton Laboratory.
The new planet, which has a mass about twice that of Jupiter,
circles its star (HD70642) about every six years. HD70642 can be found
in the constellation Puppis and is about 90 light years away from Earth.
The planet is 3.3 times further from its star as the Earth is from the
Sun (about halfway between Mars and Jupiter if it were in our own
system).
The long-term goal of this programme is the detection of true
analogues to the Solar System: planetary systems with giant planets in
long circular orbits and small rocky planets on shorter circular orbits.
This discovery of a -Jupiter- like gas giant planet around a nearby star
is a step toward this goal. The discovery of other such planets and
planetary satellites within the next decade will help astronomers
assess the Solar System’s place in the galaxy and whether planetary
systems like our own are common or rare.
Prior to the discovery of extrasolar planets, planetary systems were
generally predicted to be similar to the Solar System – giant planets
orbiting beyond 4 Earth-Sun distances in circular orbits, and
terrestrial mass planets in inner orbits. The danger of using
theoretical ideas to extrapolate from just one example – our own Solar
System – has been shown by the extrasolar planetary systems now known to
exist which have very different properties. Planetary systems are much
more diverse than ever imagined.
However these new planets have only been found around one-tenth of
stars where they were looked for. It is possible that the harder-to-find
very Solar System-like planets do exist around most stars.
The vast majority of the presently known extrasolar planets lie in
elliptical orbits, which would preclude the existence of habitable
terrestrial planets. Previously, the only gas giant found to orbit
beyond 3 Earth-Sun distances in a near circular orbit was the outer
planet of the 47 Ursa Majoris system – a system which also includes an
inner gas giant at 2 Earth-Sun distances (unlike the Solar System). This
discovery of a 3.3 Earth-Sun distance planet in a near circular orbit
around a Sun-like star bears the closest likeness to our Solar System
found to date and demonstrates our searches are precise enough to find
Jupiter- like planets in Jupiter-like orbit.
To find evidence of planets, the astronomers use a high- precision
technique developed by Paul Butler of the Carnegie Institute of
Washington and Geoff Marcy of the University of California at Berkeley
to measure how much a star “wobbles” in space as it is affected by a
planet’s gravity. As an unseen planet orbits a distant star, the
gravitational pull causes the star to move back and forth in space. That
wobble can be detected by the ‘Doppler shifting’ it causes in the
star’s light. This discovery demonstrates that the long term precision
of the team’s technique is 3 metres per second (7mph) making the
Anglo-Australian Planet Search at least as precise as any of the many
planet search projects underway.
[Astronomers
find ‘home from home’ – 90 light years away! ]