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April 2, 2008

The UK's National Astronomy Meeting

This week is the annual Royal Astronomy Society's NAM week - the UK's National Astronomy Meeting.

It is an opportunity for astronomers to showcase the latest astronomical research being carried out all around the UK. In 2007 it was been held at the University of Central Lancashire, in 2006 at the University of Leicester, and in 2005 at the University of Birmingham.

This year, we are at the historical Queen's University Belfast, with an attendance of over 600 astronomers from all around the UK, from the students studying to get their doctorates to their professors. There are so many talks on such a wide variety of subjects that there are six different lectures running simultaneously!

I hope to post my highlights of the meeting over the next few days...

Ten more planets...

What a start to this years' NAM!

The day began with the announcement (by Don Pollacco, Queen's University Belfast) that the UK Super-WASP project has discovered a staggering 10 new planets orbiting distant stars! (see the BBC News coverage)

We call such planets exoplanets. The new planets were discovered by looking at a vast number of stars every night and seeing if the brightness of any of those stars dipped for a few hours - the tale-tale sign that a planet had just passed in front of its parent star. It took astronomers 8 years to discover the first 23 planets using this method - but WASP has discovered an addition 10 in just 6 months! The next few years look very exciting for planet finders... but astronomers are already planning the next generation to WASP which would be sensitive to smaller harder-to-spot planets.

Astronomers now know of nearly 300 planets orbiting distant stars.

Astronomers: the next generation

The Astronomy Education and Outreach session at this weeks NAM revealed lots of exciting events to look forward to over the next few years!

Iwan Williams (University of London) began the session by being happy that a small number of students were now beginning to get low grades in GCSE astronomy...! (The majority of GCSE students are 14-16 year old school children)

But why was Iwan happy about this? Well, it proves that a huge cross-section of school children with a wide range of abilities now have the chance to do GCSE astronomy in 'normal' schools, and not just the very best students in private schools. Some 1400 students did the GCSE Astronomy exams in the UK this year, up from 1200 students in the previous year.

Jacquie Milligan (Glenlola Collegiate Girls School) introduced us to how the Faulkes Telescopes are being used in her science lessons, even though she is a biologist. But rather than tell us herself how the project went, Jacquie's students came along and told us what they did for themselves! When two young schoolgirls speak so confidently about their work in front of an audience of experienced research astronomers, it gives great confidence in the future of UK science.

Paul Roche (Cardiff University) told us how big an asteroid was required to remove Aberystwyth from the map whilst leaving Snowdonia intact - by using an asteroid impact simulator! You can do the same for yourself at the Down2Earth website. And when the Deep Imact mission blasted a crater in an asteroid in 2004, school children were the first to take images of the event using the Faulkes Telescope. Paul also recommended using Google Earth to study asteroid impacts on the Earth. Can you find any? Meteor crater in Arizona is a good place to start looking...

Astronomers: the next generation 2

There is so much going on here at NAM about astronomy outreach that I have had to spread the news over two posts!

Lars Christensen indicated some of the many world-wide events that will be taking place to celebrate the International Year of Astronomy in 2009, while Steve Owen highlighted some of the UK plans. Events include the 100 hours of astronomy on April the 2nd-5th 2009, the cosmic diary blog, and the spring and autumn moon watches.

Douglas Pierce-Price highlighted the involvement of the European Southern Observatory, and asked everyone to vote for their favourite picture at the Catch a Star competition website. Douglas also announced that the astronomer's hotel at the European Southern Observatory at Paranal in Chile (below) will feature in the next James Bond film - as the baddies lair!

To end the session, Rita Tojeiro highlighted the fun that was had in Scotland, during the Dark Sky Scotland series of events. Over 5000 people attended 35 events - even the occasional bad weather did not dampen the enthusiasm of visitors! Rob Hill finished the session encouraging people to attend the 2009 European Conference on Light Pollution, to be held in Armagh, Northern Ireland.

And finally, it was a announced that a gallery of images will be on display in Liverpool in June 2008 titled From Earth to the Universe.

April 4, 2008

Yet more Exosolar Planets

12 years ago, we didn't even know planets could exist around distant stars. Today, we know of almost 300 of them!

The exosolar planet session here at this year's NAM began with the announcement by Rachael Smith (Institute of Astronomy, University of Cambridge) of the astonishing discovery of two asteroid belts orbiting the star eta Tel.

Such a system may sound familiar to you... that is because we have two asteroid belts in our own solar system! In our solar system, one is between the orbits of Mars and Jupiter (the asteroid belt) and one is at the very edge of our solar system (the Kuiper-Edgeworth belt, of which Pluto appears to be the closest and largest member).

However, eta Tel is a very young system, only 12 million years old (our solar sytem is 4,500 million years old), and so eta Tel reminds us of how our solar system must have looked long ago, before Jupiter and Saturn formed. In fact, the asteroid belts in eta Tel may began to stick together to form two large planets in the future.


Artist's impression of newly discovered planets around the star Ogle-2006-BLG-109 (Credit: KASI/CBNU/ARCSEC)

Following on with the same theme, Martin Dominik (University of St Andrews) described a system called Ogle-2006-BLG-109, which contained two Jupiter-sized planets at 2.3 & 4.6 times the Sun-Earth separation - again, very similar to the planets Jupiter & Saturn in our solar system. In total, astronomers now know of 26 multiple planet systems, and 4 of these planets are in habitable zones - the location around a star that is neither too hot or too cold for life.

Astronomer Elain Simpson of the Queen's University Belfast announced the discovery of 5 more planets using SuperWASP, with 2 more suspect planets. Elain initially discovered 44 possible planets, and by observing each and every one in more detail using the Nordic Optical Telescope, she discovered the 5 planets. All these planets are hot Jupiters - large planets, very close to their parent star.

It makes us all wonder when the first Earth-like planet will be found - This year? There is a European Space Agency mission being planned called Darwin which has the aim of finding traces of water, ozone & carbon dioxide around some of these distant planets, helping us to identify Earth-like planets in the very near future.

Exosolar planet atmospheres

One of the newest topic in astronomy presented at this year's NAM was the atmosphere's in exosolar planets session. I find it staggering that astronomers can now study the atmospheric composition of planets orbiting distant stars!

The ultimate aim is to find an atmosphere around a planet that could sustain life. That has not been found yet, but it is only a matter of time...

There are two ways to study the atmosphere of a distant exoplanet. If the planet ever passes in front of the parent star, some starlight is blocked by the planet itself, but some of the star-light is absorbed by the planet's atmosphere - and by looking at what wavelength's of starlight is absorbed by the planet's atmosphere, you can work out what chemicals are present in the planet's atmosphere. Also, when the planet moves around to the far side of the star, it can reflect starlight in our direction, and by looking at that reflected starlight astronomers can work our what chemicals are doing the reflection.

Doing this in reality is incredibly difficult, due to the parent star being so bright, and the planets being so small and faint.

An artist depicts the extrasolar planet, TrES-1, and its host star. Courtesy Jeffrey Hall and Lowell Observatory.

The highlight of the session was the research done by Tommi Koskinen at the University College London, on a planet called HD17156b. This planet was actually discovered by amateur astronomers! It is very impressive what new science can be achieved by experienced amateur astronomers. In this example, the planet moved in front of its parent star, hiding 0.6% of the light coming from the star - and this is enough for skilled amateur astronomers to detect the planet.

While amateurs monitor the entire sky, professionals scrutinise individual objects, and this is exact what Tommi and his colleagues have done. They discovered that the orbit of the planet around the parent star is very elliptical (strongly oval shaped), and so the temperature of the planet can vary by a staggering 1000oC depending on where it is in its orbit. They also discovered that when the planet is close to the star it rotates at the same rate at which it orbits, but when it is further away from the star it rotates quicker.

April 6, 2008

100 years since the Tunguska Event

Prof. Mark Bailey's (Armagh Observatory) public lecture at NAM 2008 celebrated the 100th anniversary of the Tunguska event, when a large meteoroid exploded 5 miles above a remote region of Siberia.

The eyewitness reports of the event are, quite frankly, terrifying.

...the sky split in two and fire appeared high and wide over the forest. The split in the sky grew larger, and the entire Northern side was covered with fire. At that moment I became so hot that I couldn't bear it, as if my shirt was on fire;

Then I saw a wonder: trees were falling, the branches were on fire, it became mighty bright, how can I say this, as if there was a second sun, my eyes were hurting, I even closed them.

The event was even observed from Northern Ireland, some 3,500 miles away from Tunguska. The astronomer working at the Armagh Observatory that night noted a "nocturnal glow" in the log book (even though the Moon was not present), which was bright enough to read a newspaper and play cricket, even after midnight!

Fortunately, a Tunguska type event is only expected to occur, on average, once every century. And a meteor crater type impact is only expected once per million years.

But it is really difficult to estimate precisely how frequently such events occur. If you were to ask an astronomer in 1993 what the chance was of a large comet hitting Jupiter, they would have said maybe once every 100 million years... but just a year later, Comet Shoemaker-Levy 9 did hit Jupiter.

And astronomers are discovering new Near-Earth Objects (asteroids with orbits that come relatively close to the earth) all the time, as the graph below shows (courtesy NASA/JPL).

Impact frequency

But, while such events may scare us, Mark pointed out that our entire existence was dependent on the impact that wiped out the dinosaurs. If that collision had not have happened, we would not be here today.

The asteroid that wiped out the dinosaurs originated in the outer solar system, where a chance gravitational tug from another asteroid set it on a collision course with Earth. If that tug had been slightly different by a minuscule amount, the asteroid would have missed Earth, the dinosaurs would have continued their reign, and tiny mammals (from which we evolved) would never have got started - and so humans would not be here today.

Prof. Bailey then began to discuss the financial implications of ignoring the asteroid threat. If the Tunguska impact was centred on London, it would have destroyed everything within the M25, killing millions. If it hit anywhere else in the UK, it would have still killed tens of thousands. If we are lucky, and such an asteroid strikes land just once every ten attempts, that is still a major town disappearing every thousand years.

But the real risk is from the small, more frequent asteroids. We expect a 10m meteoroid to hit every year, causing a 100m crater. Maybe only 1 in ten would hit a populated area - but considering the average density of England, that once-a-decade strike could still kill 12 people.

Mark argued that this represents an intolerable risk, and using economic reasoning suggested that significant investment is required in order to research the threat posed.

Today, almost a hundred years after the event, little can be seen of the aftermath in Tunguska. Only a few felled trees remain visible, and even the small rise at the epicentre (upon which a totem pole to the Siberian fire god Agby stands) will be flat in a decade. One member of the audience suggested that, even though the fallen trees have almost disappeared, new growth may follow the lines of fertiliser provided by the fallen trees, providing at least some evidence to what happened nearly a century ago.

NAM 2008

This years National Astronomy Meeting at the Queen's University Belfast came to a close on Friday, after 4 days of talks on the latest breakthroughs in UK astronomical research.

There were so many excellent talks this year, that it was impossible to keep up blogging about them! So expect a few more blogs to appear from me over the next week.

Many press articles were released during the week, including...

At the end of the meeting, it was announced that next year's National Astronomy Meeting is to be held at the University of Hertfordshire. Many of us are looking forward to it already!

April 9, 2008

The Sky Tonight - April 2008

Spring is here, so it is time to say goodbye to Orion until next winter! By the end of April, it will by hidden by the glare of the Sun, and during June the Sun will be directly above Orion.

The Sun is setting later and later, setting now at 8pm summer time. In fact, the Sun is setting 40 minutes later at the end of the month than at the start. Although the nights are getting shorter, making it more difficult for observing, it is also getting warmer - a welcome relief to anyone who has been observing in sub-zero temperatures this winter!

The Moon is a wonderful sight in the evening for the first few weeks of April, but the full Moon is on the 20th, making it very difficult to see any but the brightest stars. Last quarter is on the 28th of April, so that is another good opportunaty to observe the fainter objects this month.

The only planets visible in the evening this month are Mars (look west for a red object all evening, although it gets very low in the sky after midnight), and Saturn (high in the south at sunset, and setting in the west at 3am).

Saturn is easy to spot this month since it is so close to the bright star Regulus, in the constellation of Leo (Saturn is the slightly fainter of the two). On the night of the 14th of April, the Moon is just to the right of the pair, and on the following night, the Moon is just below the pair.

If you have never seen the rings of Saturn before, then those two nights are the best time to be amazed by the sight, with the Moon acting as a very helpful guide, and Saturn being at its highest point in the sky at sunset in the evening - very convenient!

We know summer is rapidly approaching, because the summer triangle is once again visible in the evening sky, rising during April at around 10pm.

And for those staying up really late, Jupiter is very bright indeed. Just look towards the south-east to see Jupiter rising at 3am. If you have binoculars, take a closer look and you may be able to see up to 4 moons orbiting around Jupiter.

April 15, 2008

Cosmic Visions

Cosmic visions is a European Space Agency initiative to plan missions to be launched between 2015-2025. And there is no shortage of ideas!

Missions include:

  • XEUS - the next generation X-ray telescope, designed to look at the hottest and most violent regions of space
  • LISA - a mission to detect and measure gravity waves, emitted when massive objects violently collide
  • SPICA - a mission to explore how stars and planets form
  • PLATO aims to search for planets orbiting distant stars
  • TANDEM will scrutinise Saturn's moons Titan (an Earth-like organic-rich world) and Enceladus.
  • LAPLACE would explore Jupiter's moon Europa - and world covered in ice but with a water ocean beneath the surface
  • MARCO-POLO is a mission to return a sample from a near-Earth asteroid, which could be key if we ever need to deflect an asteroid in the future
  • CROSS-SCALE plans to study astrophysical plasma's in all regions of space.
  • SPACE - a mission to study how the Universe evolved in infrared wavelengths
  • DUNE - designed to study dark matter and dark energy in the universe

Not all these missions will become reality.

Which ones would you choose?


DUNE
A wide field, visible and near-infrared space imager, with the primary goal of studying dark energy and dark matter with unprecedented precision by using weak gravitational lensing
SPACE
A near-infra-red surveyor dedicated to an all-sky, spectroscopic survey of a large number of galaxies, aiming to obtain information on the evolution of galaxies in the Universe

XEUS
New generation, space based X-ray observatory dedicated to investigations on the evolution of the Universe at higher energies and based on a two spacecraft formation concept

SPICA
European contribution to the Japanese SPICA mission, dedicated to Medium and Far Infrared astronomy and to investigations on the origins of galaxies and planets

PLATO
Ultra-high precision, visible and near-infrared photometry mission, dedicated to investigations on exo-planets transiting in front of a large sample of stars as well as to investigations on the seismic oscillations of these parent stars

Marco Polo
In-situ measurements and sample return from a primitive Near-Earth Object (asteroid or dormant comet) in order to reveal information about the early formation processes of the Solar System and the role of minor bodies in the origin and evolution of life on Earth

TandEM
In-situ exploration of the two Saturn moons: Titan and Enceladus in order to gain knowledge on their geological, chemical and evolutionary history and possibly understand their astrobiological potential

Cross-Scale
Quantifying the coupling in plasmas between different physical scales in order to address fundamental questions such as how shocks accelerate and heat particles or how reconnection converts magnetic energy
LAPLACE
In-depth, quantitative study of the Jupiter system and its moons, which focuses on the formation of the Jupiter System, the way how the Jupiter system works, and whether Europa is habitable
LISA
A three-spacecraft interferometer with an arm length of 5 million kilometres and the primary goal to detect and observe gravitational waves from astronomical sources in a frequency range of 0.0001 to 0.1 Hz

The above banners have been taken from the ESA website.

April 20, 2008

The last big feast of our Milky Way's giant black hole

Using three X-ray space telescopes - ESA's XMM-Newton, JAXA's Suzaku and NASA's Chandra - Japanese astronomers have discovered that the black hole at the centre of our galaxy was much more active 300 years ago, when it gorged on a large feast of nearby stars (for full details, see ESA's press release).

Imagine looking for a black object on a black background, and you will appreciate the difficulty in observing black holes! However, when a star or gas falls in towards a black hole, it gets extremely hot - millions of degrees centigrade hot! Anything at this temperature will give off X-ray radiation. So the best way to find a black hole is to look for X-rays in space - the tell-tell sign of something falling towards a black hole.

Not only that, but those X-rays can reflect off clouds of gas... which is exactly what has been observed. A cloud of gas near the centre of our galaxy suddenly brightened. What astronomers believed happened is that the black hole at the centre of the galaxy had a big feast which released large amounts of X-rays. Those X-rays then travelled for 300 years until they collided with the neighbouring gas cloud and caused it to glow. And now, we are just seeing that gas cloud glow.

This means that, if we had X-ray space telescopes 300 years ago, we would have been able to witness the black hole at the centre of the Milky-way enjoying its feast!

We have seen the super-massive black-hole at the centre of the Milky-way feed before, but the feast 300 years ago was a million times bigger than anything we have seen in recent times.

If you want to know more about black hole, why not watch our planetarium show Black-holes: the other side of infinity?

April 22, 2008

links for 2008-04-22

About April 2008

This page contains all entries posted to Royal Observatory, Greenwich in April 2008. They are listed from oldest to newest.

March 2008 is the previous archive.

May 2008 is the next archive.

Many more can be found on the main index page or by looking through the archives.