http://www.bbc.co.uk/news/science-environment-22556750
Thank you BBC and Pat for our alert.
Friday, 17 May 2013
Tuesday, 14 May 2013
Largest CME of the year
The Sun has unleashed its most powerful eruption of 2013 so far.
The solar flare - a sudden release of radiation - peaked at 1705 BST on Monday, and was associated with a huge eruption of matter.
When these eruptions reach Earth, they can interfere with electronic systems in satellites and those on the ground.
Nasa said this solar explosion - known as a coronal mass ejection (CME) - was not directed at Earth, but it could pass several US spacecraft.
The event on Monday was classified as an "X-class" flare - the most intense type - with a designation of X2.8 (higher numbers denote a stronger flare). It surpassed an X1.7-class flare that occurred 14 hours earlier.
Space Oddity
International Space Station Commander Chris Hadfield has spent the last year charming the earthbound public with his tweets and Tumblr posts from the International Space Station. Now, it turns out he’s got pipes, too: to celebrate the end of his tenure on the I.S.S., he’s recorded a gorgeous and touching tribute to David Bowie’s “Space Oddity.”
He’s also a veteran member of Max Q—an all-astronaut band that’s been playing with rotating lineups since 1987. When Hadfield’s on the ground, he covers bass and lead vocals. And he’s good—really good. As of this morning, the “Space Oddity” video had passed 1.5 million hits, and Bowie’s Facebook page lauded it as “possibly the most poignant version of the song ever created.”
Thursday, 9 May 2013
Large Meteor in the Sky Last Night
A large blue meteor was spotted last night (8th May) travelling across the night sky by people in many parts of England and Wales. Many observers suggested it was a fireball, a brighter-than-usual meteor. The International Astronomical Union defines a fireball as "a meteor brighter than any of the planets" (magnitude −4 or greater).
Watch amateur footage here.
Suzy Buttress, of Basingstoke, described witnessing the meteor as a "once in a lifetime thing".
Space scientist Dr Maggie Aderin-Pocock said the phenomenon was likely to have been debris from Halley's Comet.
Dr Aderin-Pocock explained what could have caused the spectacle.
"Unfortunately I didn't see this meteor myself, but I think what's unusual is the size of this one. With meteor showers people will see a number of meteors over an hour, so let's say six or 10 an hour.
"It seems that this one was particularly large and particularly bright, which is why it's caught so much attention.
"It's quite likely to be part of the Eta Aquarids, which is the debris left by Halley's Comet.
"And twice a year we pass through the debris left behind by the comet and when this happens we see more of these shooting stars but there must have been a large lump left behind which is what caused such a bright meteor to be seen."
Tuesday, 7 May 2013
Herschel finds hot gas on the menu for Milky Way’s black hole
ESA’s Herschel space observatory has made detailed observations of surprisingly hot molecular gas that may be orbiting or falling towards the supermassive black hole lurking at the centre of our Milky Way galaxy.
Our local black hole is located in a region known as Sagittarius A* – Sgr A* – after a nearby radio source. It has a mass about four million times that of our Sun and lies around 26 000 light-years away from the Solar System.
Even at that distance, it is a few hundred times closer to us than any other galaxy with an active black hole at its centre, making it the ideal natural laboratory to study the environment around these enigmatic objects.
Vast amounts of dust lie in the plane of the Milky Way between here and its centre, obscuring our view at visible wavelengths. But at far-infrared wavelengths, it is possible to peer through the dust, affording Herschel’s scientists the chance to study the turbulent innermost region of our Galaxy in great detail.
Our local black hole is located in a region known as Sagittarius A* – Sgr A* – after a nearby radio source. It has a mass about four million times that of our Sun and lies around 26 000 light-years away from the Solar System.
Even at that distance, it is a few hundred times closer to us than any other galaxy with an active black hole at its centre, making it the ideal natural laboratory to study the environment around these enigmatic objects.
Vast amounts of dust lie in the plane of the Milky Way between here and its centre, obscuring our view at visible wavelengths. But at far-infrared wavelengths, it is possible to peer through the dust, affording Herschel’s scientists the chance to study the turbulent innermost region of our Galaxy in great detail.
Herschel has detected a great variety of simple molecules at the Milky Way’s heart, including carbon monoxide, water vapour and hydrogen cyanide. By analysing the signature from these molecules, astronomers have been able to probe some of the fundamental properties of the interstellar gas surrounding the black hole.
“Herschel has resolved the far-infrared emission within just 1 light-year of the black hole, making it possible for the first time at these wavelengths to separate emission due to the central cavity from that of the surrounding dense molecular disc,” says Javier Goicoechea of the Centro de Astrobiología, Spain, and lead author of the paper reporting the results.
The biggest surprise was quite how hot the molecular gas in the innermost central region of the Galaxy gets. At least some of it is around 1000ºC, much hotter than typical interstellar clouds, which are usually only a few tens of degrees above the –273ºC of absolute zero.
While some of the heating is down to the fierce ultraviolet radiation pouring from a cluster of massive stars that live very close to the Galactic Centre, they are not enough to explain the high temperatures alone.
In addition to the stellar radiation, Dr Goicoechea’s team hypothesise that emission from strong shocks in highly-magnetised gas in the region may be a significant contributor to the high temperatures. Such shocks can be generated in collisions between gas clouds, or in material flowing at high speed from stars and protostars.
“The observations are also consistent with streamers of hot gas speeding towards Sgr A*, falling towards the very centre of the Galaxy,” says Dr Goicoechea. “Our Galaxy’s black hole may be cooking its dinner right in front of Herschel’s eyes.”
Tuesday, 30 April 2013
Giant Hurricane on Saturn
NASA's Cassini spacecraft has provided scientists the first close-up, visible-light views of a behemoth hurricane swirling around Saturn's north pole.
Thin, bright clouds at the outer edge of the hurricane are traveling 330 mph(150 meters per second). The hurricane swirls inside a large, mysterious, six-sided weather pattern known as the hexagon.

This spectacular, vertigo inducing, false-color image from NASA's Cassini mission highlights the storms at Saturn's north pole. The angry eye of a hurricane-like storm appears dark red while the fast-moving hexagonal jet stream framing it is a yellowish green. Low-lying clouds circling inside the hexagonal feature appear as muted orange color. A second, smaller vortex pops out in teal at the lower right of the image. The rings of Saturn appear in vivid blue at the top right.
The images were taken with Cassini's wide-angle camera using a combination of spectral filters sensitive to wavelengths of near-infrared light. The images filtered at 890 nanometers are projected as blue. The images filtered at 728 nanometers are projected as green, and images filtered at 752 nanometers are projected as red. At Saturn, this scheme means colors correlate to different altitudes in the planet's polar atmosphere: red indicates deep, while green shows clouds that are higher in altitude. High clouds are typically associated with locations of intense upwelling in a storm. These images help scientists learn the distribution and frequencies of such storms. The rings are bright blue in this color scheme because there is no methane gas between the ring particles and the camera.
The view was acquired at a distance of approximately 261,000 miles (419,000 kilometers) from Saturn and at a sun-Saturn-spacecraft, or phase, angle of 94 degrees. Image scale is 13 miles (22 kilometers) per pixel.
For more information about the Cassini-Huygens mission visit http://www.nasa.gov/cassini and http://saturn.jpl.nasa.gov. The Cassini imaging team homepage is at http://ciclops.org.
The enormous hurricane raging at Saturn's north pole has an eye 2,000km (1,250mi) across - big enough to cover the UK 12 times over.
This spectacular, vertigo inducing, false-color image from NASA's Cassini mission highlights the storms at Saturn's north pole. The angry eye of a hurricane-like storm appears dark red while the fast-moving hexagonal jet stream framing it is a yellowish green. Low-lying clouds circling inside the hexagonal feature appear as muted orange color. A second, smaller vortex pops out in teal at the lower right of the image. The rings of Saturn appear in vivid blue at the top right.
The images were taken with Cassini's wide-angle camera using a combination of spectral filters sensitive to wavelengths of near-infrared light. The images filtered at 890 nanometers are projected as blue. The images filtered at 728 nanometers are projected as green, and images filtered at 752 nanometers are projected as red. At Saturn, this scheme means colors correlate to different altitudes in the planet's polar atmosphere: red indicates deep, while green shows clouds that are higher in altitude. High clouds are typically associated with locations of intense upwelling in a storm. These images help scientists learn the distribution and frequencies of such storms. The rings are bright blue in this color scheme because there is no methane gas between the ring particles and the camera.
The view was acquired at a distance of approximately 261,000 miles (419,000 kilometers) from Saturn and at a sun-Saturn-spacecraft, or phase, angle of 94 degrees. Image scale is 13 miles (22 kilometers) per pixel.
For more information about the Cassini-Huygens mission visit http://www.nasa.gov/cassini and http://saturn.jpl.nasa.gov. The Cassini imaging team homepage is at http://ciclops.org.
Wednesday, 24 April 2013
Partial Lunar Eclipse
A partial lunar eclipse will take place on April 25, 2013, the first of three lunar eclipses in 2013. Only a tiny sliver of the Moon will be covered by the Earth's umbral shadow at maximum eclipse, but the entire northern half of the Moon will be darkened from being inside the penumbral shadow. This is the second shortest partial eclipse of the Moon for the 21st century, lasting 27 minutes. On September 29, 2042, a partial eclipse of just 0.3% lasting just 12 minutes will be visible.

This partial eclipse will only graze the southern border of the Earth's umbra.
This partial eclipse will only graze the southern border of the Earth's umbra.
Contact
| Time UTC |
|---|---|
| Penumbral Eclipse Begins |
18:03:38
|
Partial Eclipse Begins
|
19:54:08
|
Greatest Eclipse
|
20:07:30
|
Partial Eclipse Ends
|
20:21:02
|
Penumbral Eclipse Ends
|
22:11:26
|
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