This is the Hubblecast!
News and images from the NASA/ESA Hubble Space Telescope.
Travelling through time and space with our host Doctor J, a.k.a. Dr. Joe Liske.
Welcome to the sixth special episode of the Hubblecast celebrating the International Year of Astronomy in 2009.
In the fifth episode, we saw how some telescopes study parts of the universe that we can’t see with our eyes.
This time, we will see how telescopes in space have revolutionised almost every field in astronomy.
The Hubble Space Telescope.
Is by far the most famous telescope in history. And for good reason.
Hubble has revolutionised so many fields in astronomy.
By modern standards, Hubble’s mirror is actually quite small.
It only measures about 2.4 metres across.
But its location is literally out of this world.
High above the blurring effects of the atmosphere, it has an exceptionally sharp view of the Universe.
And what’s more, Hubble can see ultraviolet and near-infrared light.
This light just cannot be seen by ground-based telescopes because it is blocked by the atmosphere.
Cameras and spectrographs, some as big as a telephone booth, dissect and register the light from distant cosmic shores.
Just like any ground-based telescope, Hubble is upgraded from time to time.
Spacewalking astronauts carry out servicing missions.
Broken parts get refurbished and older instruments get replaced with newer and state-of-the-art technology.
Hubble has become the powerhouse of observational astronomy.
And it has transformed our understanding of the cosmos.
With its keen eyesight, Hubble observed seasonal changes on Mars...
a cometary impact on Jupiter...
an edge-on view of Saturn’s rings...
and even the surface of tiny Pluto.
It revealed the life cycle of stars, from their very birth and baby days in a nursery of dust-laden clouds of gas,
all the way to their final farewell:
as delicate nebulae, slowly blown into space by dying stars,
or as titanic supernova explosions that almost outshine their home galaxy.
Deep in the Orion Nebula, Hubble even saw the breeding ground of new solar systems:
dusty discs around newborn stars that may soon condense into planets.
The space telescope studied thousands of individual stars in giant globular clusters, the oldest stellar families in the Universe.
And galaxies, of course.
Never before had astronomers seen so much detail.
Majestic spirals, absorbing dust lanes, violent collisions.
Extremely long exposures of blank regions of sky
even revealed thousands of faint galaxies billions of light-years away.
Photons that were emitted when the Universe was still young.
A window into the distant past, shedding new light on the ever-evolving cosmos.
Hubble is not the only telescope in space.
This is NASA’s Spitzer Space Telescope, launched in August 2003.
In a way, it is Hubble’s equivalent for the infrared.
Spitzer has mirror that is only 85 centimetres across.
But the telescope is hiding behind a heat shield that protects it from the Sun.
And its detectors are tucked away in a dewar filled with liquid helium.
Here the detectors are cooled down to just a few degrees above absolute zero making them very, very sensitive.
Spitzer has revealed a dusty Universe.
Dark, opaque clouds of dust glow in the infrared when heated from within.
Shock waves from galaxy collisions sweep up dust in telltale rings and tidal features,
new sites for ubiquitous star formation.
Dust is also produced in the aftermath of a star’s death.
Spitzer found that planetary nebulae and supernova remnants are laden with dust particles,
the prerequisite building blocks of future planets.
At other infrared wavelengths, Spitzer can also see right through a dust cloud,
revealing the stars inside, hidden in their dark cores.
Finally, the space telescope’s spectrographs have studied the atmospheres of extrasolar planets –
gas giants like Jupiter, that race around their parent stars in just a few days.
So what about X-rays and gamma rays?
Well, they are completely blocked by the Earth’s atmosphere.
And so without space telescopes, astronomers would be totally blind to these energetic forms of radiation.
X-ray and gamma ray space telescopes reveal the hot, energetic and violent Universe
of galaxy clusters, black holes, supernova explosions, and galaxy collisions.
They are very hard to build, though.
Energetic radiation passes right through a conventional mirror.
X-rays can only be focused with nested mirror shells made of pure gold.
And gamma rays are studied with sophisticated pinhole cameras,
or stacked scintillators that give off brief flashes of normal light when struck by a gamma ray photon.
In the 1990s, NASA operated the Compton Gamma Ray Observatory.
At the time, it was the largest and most massive scientific satellite ever launched.
A fully fledged physics lab in space.
In 2008, Compton was succeeded by GLAST:
the Gamma Ray Large Area Space Telescope.
It will study everything in the high-energy Universe from dark matter to pulsars.
Meanwhile, astronomers have two X-ray telescopes in space.
NASA’s Chandra X-ray Observatory
and ESA’s XMM-Newton Observatory are both studying the hottest places in the Universe.
This is what the sky looks like with X-ray vision.
Extended features are clouds of gas,
heated to millions of degrees by shock waves in supernova remnants.
The bright point sources are X-ray binaries:
neutron stars or black holes that suck in matter from a companion star.
This hot, in falling gas emits X-rays.
Likewise, X-ray telescopes reveal supermassive black holes in the cores of distant galaxies.
Matter that spirals inward gets hot enough to glow in X-rays
just before it plunges into the black hole and out of sight.
Hot but tenuous gas also fills the space between individual galaxies in a cluster.
Sometimes, this intracluster gas is shocked and heated even more by colliding and merging galaxy clusters.
Even more exciting are gamma ray bursts, the most energetic events in the Universe.
These are catastrophic terminal explosions of very massive, rapidly spinning stars.
In less than a second, they release more energy than the Sun does in 10 billion years.
Hubble, Spitzer, Chandra, XMM-Newton and GLAST are all versatile giants.
But some space telescopes are much smaller and have much more focused missions.
Take COROT, for example.
This French satellite is devoted to stellar seismology and the study of extrasolar planets.
Or NASA’s Swift satellite,
a combined X-ray and gamma ray observatory designed to unravel the mystery of gamma ray bursts.
And then there’s WMAP, the Wilkinson Microwave Anisotropy Probe.
In just over two years in space, it had already mapped the cosmic background radiation to unprecedented detail.
WMAP gave cosmologists the best view yet of one of the earliest phases of the Universe,
more than 13 billion years ago.
Opening up the space frontier has been one of the most exciting developments in the history of the telescope.
So what’s next?
Thank you for joining me in this sixth episode of the special series.
Next time we will see the new and amazing telescopes of the future that are currently being planned.
This is Dr. J. signing off for the Hubblecast.
Once again nature has surprised us beyond our wildest imagination.