Great Day for Cosmology

Exciting times for cosmology. It’s Nobel Prize week again, and in the first bit of good news for the day, the Physics Nobel was awarded to Saul Perlmutter, Adam Riess and Brian Schmidt. These three scientists were leaders in the studies of type Ia supernovae that led to the discovery of dark energy in 1998 [here's a primer on the science by Schmidt] – the mysterious phenomenon that causes the Universe to expand at a faster rate than we had previously thought.

Truly groundbreaking new results don’t happen very often in science – in fact, trying to think of those that are is quite a fun exercise. Of the last few decades, the discovery of dark energy from observations of distant supernovae is by far the most prominent groundbreaker I can ever think of. So it’s really no surprise that they are now receiving one of the highest honours, and it’s much deserved. (Of course so many physicists are deserving of big prizes, and these things are notoriously hard to predict.)

The second bit of good news for cosmologists is that ESA have officially selected the Euclid mission as one of its next medium-sized mission. Scheduled for launch in 2019, Euclid’s main objective is to study the nature of dark energy by measuring shapes and redshifts of a huge number of objects in the Universe over the entire sky. It’s a fascinating mission, both scientifically and technically, that we’re also involved in at MPIA. Great news for everyone involved.

We know so little about dark energy, a huge targeted survey like Euclid is bound to throw up some really intriguing new questions – perhaps even some answers? If you combine that with the fascinating stuff that’s going on in particle physics, faster than light neutrinos and such, it’s safe to say that cosmology is heading towards some really fun times!

[Very little blogging in recent weeks..... I'm having an exceptionally busy time at work at the moment, with proposal deadlines, and instrument deadlines, and the handover of MIRI to NASA on the immediate horizon. My Rule #1 for blogging is that blogging cannot cause me any extra stress - so for now it's on the backburner. More activity soon!]

 

Credit where it’s due?

The Andromeda Galaxy in optical, IR and X-ray

Earlier this week, this amazing image of M31, the Andromeda galaxy, was splashed all over the media and the inernet. The image is a composite of optical, infrared and X-ray data, with the infrared image coming from the Herschel space telescope, launched in 2009. The picture has been featured and discussed in the media all week – rightly so, as it’s stunning. With Herschel, we can finally showcase far-infrared and submillimetre images that are just as beautiful as those produced at shorter wavelengths with Hubble, or VLT on the ground. Moreover, observing galaxies at these wavelengths at the level of detail enabled by Herschel is opening some big new windows onto the physics that governs the Universe, from right on our doorstep to billions of lightyears away. What I’m saying, if that wasn’t yet clear, is that this telescope is something to be very proud of.

The Daily Mail, however, decided to take a different approach – one that both misses the point, and is plain wrong. It sets the Herschel image side by side with an optical image of Andromeda, taken by British amateur astronomer Steve Loughran, and asks:

“One of these pictures was taken in a British back garden by an amateur using kit worth £10,000 – the other cost Nasa millions. But can you tell the difference?”

Herschel looks into the Heart of Darkness

Star formation in Gould's Belt

Last week a big conference took place at the European Space Agency hub ESTEC, down the road in Noordwijk. The town was inundated with the lucky scientists who got to play with the first data from the new infrared space observatory Herschel and were finally allowed to talk about it to the rest of the world. And now that the conference is over, as expected, science from Herschel is everywhere!

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20 Years of Hubble

Source: Hubblesite.org. Credit: NASA, ESA, and M. Livio and the Hubble 20th Anniversary Team (STScI)

Today we celebrate the 20th anniversary of the launch of the Hubble Space Telescope. Hurrah! Although it’s clearly impossible, as I haven’t aged more than, oh, 10 years since then.

The folks at NASA and ESA have released a set of gorgeous new images and videos of the Carina Nebula, a region of active star formation in our Galaxy.

The European Hubble team have also taken the occasion to launch a rather nice looking new website, check it out here.

The same team are organising a competition to find the most artistic, funniest, weirdest, largest and smallest manifestations of Hubble and its images in popular culture – that’s a fun idea. Anyone can join the Flickr group and submit images, and the category winners get some cool prizes. Read more here.

Google joined in the celebration with a lovely doodle for the day:

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Oh My Herschel

Herschel stares into Aquila

Herschel stares into Aquila

Scientists have gathered in Madrid this week to discuss for the first time the data they have received from the new infrared telescope Herschel that was launched in May of this year. Some fantastic images have been produced as part of the first observing programmes, like the one above of an active star forming region in the constellation Aquila. The region was known as a ‘dark cloud’ – meaning that dust was blocking any visible or near-infrared radiation coming from its interior. Until Herschel came along, and switched on the lights. Observing at longer infrared wavelengths, the telescope is sensitive to radiation from cooler and dusty material, allowing it to peer into the cloud’s interior. The image, created from data from two of Herschel’s images, PACS and SPIRE, shows up to 700 dense pockets of cold and dusty material that may eventually condense into stars; around 100 of them have progressed to the protostellar stage where they begin to resemble a young forming star.

ESA has launched a new site to showcase the Herschel images. A little sparsely populated so far, but the first postings are very promising indeed.

Image credit: ESA and the SPIRE & PACS consortia, Ph. André (CEA Saclay) for the Gould’s Belt Key Programme Consortia