First Observation of a Uranian Mutual Event (Forwarded)
- From: Andrew Yee <ayee@xxxxxxxxxxxxxxxxxxxxxx>
- Date: Wed, 16 May 2007 20:46:40 GMT
Armagh Observatory
Armagh, Northern Ireland
FOR FURTHER INFORMATION PLEASE CONTACT:
Apostolos Christou or David Asher
Armagh Observatory
Tel. 028-3752-2928
16 May 2007
First Observation of a Uranian Mutual Event
An international team of astronomers led by Apostolos Christou at Armagh
Observatory has made the first ever observation of one of the satellites
of the planet Uranus passing in front of another. The observation was made
on the night of 4th May by Marton Hidas and Tim Brown, of the Las Cumbres
Observatory Global Telescope, Santa Barbara, California, using the robotic
Faulkes Telescope South at Siding Spring Observatory, Australia. This work
involves a collaboration between scientists at Siding Spring, Las Cumbres,
Armagh and Cardiff University.
When one satellite passes in front of another, the phenomenon is known as
an occultation; when one moves into the shadow of another it is an
eclipse. Collectively, occultations and eclipses are called mutual events.
These provide a means to determine the positions of the satellites with
exceptional precision, better than any optical telescope, but they are
rare. In the case of Uranus, a season of mutual events occurs just once
every 42 years, each individual event lasting just a few minutes. At the
time of the last Uranian mutual event season, Man had yet to walk on the
Moon. Not surprisingly, no-one had successfully recorded any mutual event
involving these extremely faint satellites, which are 3,000 million
kilometres from Earth.
But this situation changed this month, when the Faulkes telescope observed
the satellite Oberon (named after the "King of Shadows and Fairies" in
Shakespeare's "A Midsummer Night's Dream") occulting Umbriel (the "dusky
melancholy sprite" in Alexander Pope's poem "The Rape of the Lock"). As
Oberon's disc encroached upon Umbriel's, gradually blocking off Umbriel¹s
light, the combined brightness of the moons dropped by about a third.
Measurements of such changes in brightness, and comparison with models of
the satellites' motions, allow astronomers to work out the masses of the
moons and the effects of the shape of Uranus on their orbits, and to model
their surface features. The current Uranian mutual-event season is
expected to lead to some of the greatest advances in the study of the
Uranian system since the flyby of the Voyager 2 spacecraft in 1986.
This observation kicks off a campaign extending from now into 2008 to
observe the entire mutual event season. It highlights the value of the
North and South Faulkes telescopes for recording rare, time-critical
events. And because the telescopes have an educational focus, the data
will eventually be used not just by astronomers but also by schools and
schoolchildren worldwide.
[NOTE: Images supporting this release are available at
http://www.arm.ac.uk/press/2007/uranus_event03.html ]
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