Showing posts with label cosmology. Show all posts
Showing posts with label cosmology. Show all posts
Wednesday, March 19, 2014
Explaining the New Discovery about the Big Bang
As you may have heard, a large team of scientists (from many universities and labs) has used a telescope at the South Pole to make ground-breaking measurements of the very first instants oftime after the Big Bang. There's been a lot of media interest in the discovery, and this morning I was part of a team of scientists (including string theorist Brian Greene) who tried to explain the measurements and the ideas behind them on KQED's Forum program with Michael Krasny. You can hear the full hour at:http://www.kqed.org/a/forum/R201403190900
In the photo, you can see the Dark Sector Lab, a research facility just 3/4 of a mile from the Earth's South Pole. It was the antenna at left (BICEP2) that detected and measured microwaves that are the "afterglow" of the big bang.
For decades, physicists have explained some of the most intriguing large-scale properties of the universe by suggesting that, a tiny fraction of time after the big bang, the cosmos underwent a period of tremendous "inflation" (like blowing up a balloon with the breath of a million people, instead of just with your own lung-power.) That sudden increase in the size of the universe can help us to understand many things about cosmic conditions today, some 14 billion years after the big bang.
But did this "inflation" really happen? That's what the experiment at the South Pole set out to discover. If it did, it would have left very subtle imprints on the "cosmic background radiation" (the afterglow of the big bang) which today comes to us in the form of cool microwaves. (Cool here meaning less energetic waves than the light from the screen on which you are reading this post.)
The imprint of inflation was so delicate that it took several years of observations and even more years of massaging the data to tease it out of the microwave maps we make. One of the leaders of the team said during the show that the effect was 1 part in 30 million. But if it's confirmed by other experiments, this will stand as a milestone in our study of the universe. It's a remarkable wedding between the small scale world of atoms and waves (gravity waves making tiny ripples in the fabric of space-time) and the large-scale world of the entire universe.
It's one more piece of evidence that we now live at a time of "precision cosmology" -- being able to measure the properties of the entire cosmos with laboratory accuracy.
Labels:
astronomy,
astrophysics,
BICEP2,
big bang theory,
Brian Greene,
cosmic background radiation,
cosmology,
gravity waves,
inflation,
KQED Forum,
microwave telescope,
physics,
science,
science news,
south pole
Wednesday, February 19, 2014
Crisis at the Historic Lick Observatory
Lick Observatory, which went into operation in 1888 and was the first mountain-top observatory, is threatened by the budget axe at the University of California. The University President's Office has said that, by 2017-18, it will have to close the still-active observatory (which played a key role in the discovery of the acceleration of the universe, an observation that won the 2011 Nobel Prize in physics.)
You can read the full story in the alumni magazine for the U. of California: http://alumni.berkeley.edu/california-magazine/just-in/2014-02-19/not-licked-yet-fight-keep-iconic-uc-observatory-open
But those of you in the San Francisco Bay Area next week can hear Prof. Alex Filippenko, the President of the Lick Observatory Council, give a free public talk about the latest situation (and what is being discovered at Lick). The talk is Wednesday evening, Feb. 26th, at 7 pm in the Smithwick Theater at Foothill College in Los Altos.
It's part of the Silicon Valley Astronomy Lecture Series, which I have had the pleasure of organizing and moderating for the last 14 years. For more information about the talk and the speaker, and for directions, see:http://www.foothill.edu/news/newsfmt.php?sr=2&rec_id=3270
From its early discovery of the fifth moon of Jupiter's to the recent findings of planets orbiting other stars, the Lick Observatory has a rich history of astronomical work. Plus, it's a premier educational facility, training young astronomers and welcoming tens of thousands of visitors to its spectacular site.
If you don't live in the area, but would like to know more or would like to help, check out the "Save Lick" website:
http://www.ucolick.org/SaveLick/
(The attached photo, taken by Rick Baldridge of the Peninsula Astronomical Society, shows Lick's oldest building in front of the rising full moon.)
I have a special fondness for the Lick Observatory because its first director helped ound the Astronomical Society of the Pacific, where I was the executive director for 14 years. Plus it's a Bay Area treasure, and its closing would be a tremendous loss for Bay Area astronomy.
Monday, January 20, 2014
The Death of Two Iconoclasts in Astronomy
This past week brought us news of the death of two very different
members of the astronomical community who became known for thinking far “outside
the box” – astronomer Halton “Chip” Arp and amateur astronomer and telescope
designer John Dobson. I got to know both
of them through my work with the Astronomical Society of the Pacific (ASP.)
Chip Arp, trained at Harvard and Caltech, was an astronomer at the Hale
Observatories who specialized in the study of the great islands of stars we
call galaxies. He was particularly
interested in those galaxies that had an unusual appearance or characteristics,
and, in 1966, he put together a collection of images of over 300 of these,
which he called his “Atlas of Peculiar Galaxies.” At the time, they seemed mysterious, but today
we understand that many of them look odd because two or more galaxies have
collided or passed too close (or are in the process of doing so). Such collisions are now known to be far more
common among galaxies than astronomers first thought.
Alas, at one point in his research, Arp decided that the way we measure
distances to galaxies (Hubble’s rule that the faster the galaxy is moving away
from us, the farther it is from us) was not always correct. He thought he saw several pairs of galaxies
that were moving at different speeds, and thus should be separated by vast
distances, but seemed on his photos to be physically connected – a contradiction. Eventually, he decided that these connections
challenged the notion that our universe is expanding smoothly from a “big bang”
beginning. When other astronomers
investigated his best cases with better instruments, he turned out to be wrong
-- many of his “connections” were really just chance alignments of different
objects on early photographs.
As few other astronomers joined him in his ultimately quixotic attempt
to undercut the big bang idea, he slowly became embittered and felt persecuted. But I knew him back when he was Vice-President
and then President of the ASP from 1979 to 1983 (and I was the Society’s
Executive Director). Having been a
champion fencer and a bon vivant, he cut a dramatic figure, arguing with genially
with Board member Allan Sandage, charming our donors and members, and still
full of energy in fighting the “establishment.” Although he turned out to be wrong, Arp was
a useful figure in making astronomers re-measure and re-check their assumptions
about galaxies and the universe. Science
always needs a few well-trained “trouble-makers” and “dissenters” to keep us
from taking our “party-line” views for granted.
John Dobson, on the other hand, was mostly self-taught in astronomy,
but invented a new way of building amateur telescopes that helped make astronomy
as a hobby more accessible. Today, many
serious amateur astronomers build or buy telescopes with “Dobsonian mounts.” (His original inspiration, developed while
being trained as a monk in a Vedanta Monastery, was to find a way to build
telescopes cheaply for those who could not afford them. His first mirrors were made from the glass
of discarded ship portholes.)
After he left the Monastery, he founded the San Francisco Sidewalk
Astronomers, whose mission was to show the public the night sky by bringing
telescopes to the streets. The sidewalk
astronomy movement spread to other cities, and has influenced many amateur
astronomy clubs to hold public events in settings where there may be more
light, but there are also significant crowds of people who have never looked
through a telescope.
Unfortunately, along the way, Dobson decided that both Einstein’s and
Hubble’s work was wrong and that our modern view of the universe was fatally
flawed. Instead of restricting his
dynamic lectures and workshops to helping amateurs and the public appreciate
astronomy (a subject where he excelled), he could not resist offering seminars
on abstract issues in the science of the universe (where he had no particular
expertise.) I remember one meeting of
the ASP, where noted astronomer Margaret Burbidge sat for a long time with John
Dobson, patiently explaining to him where his views collided with known facts
about the universe – but no avail. I too tried in a small way to help him
understand the power of Einstein’s theories, but he was by then too enmeshed in
his own views to see clearly.
Still, we can celebrate that many, many thousands of people owe their
exposure to astronomy to Dobson’s enthusiasm, and that there are several
generations of California amateur astronomers who were inspired and helped by
Dobson’s unfailing enthusiasm for sharing the sky. They continue to do “sidewalk astronomy” and
to make new friends for our science.
The illustration above shows entry number 142 in Arp’s catalog, seen not in
black and white, but with the full power of the Hubble Space Telescope. The two colliding galaxies have influenced
each other’s structure (and just happen right now to resemble a penguin
standing guard over an egg.) For more,
see the short video at: http://www.spacetelescope.org/videos/heic1311a/
Below is a snapshot I took of Chip Arp during his time as ASP President.
Sunday, October 21, 2012
Extremely Deep View of the Universe
Last month, the Hubble Space Telescope released one of the most impressive astronomical images ever taken and I wanted to share it with you. Called the Hubble Extremely Deep Field, it shows a tiny, tiny portion of the sky in the constellation of Fornax -- a portion about the same size (angle) in our sky as one of the smaller dark splotches (maria) you can see on the Moon.
Between 2002 and 2012, a team of astronomers kept photographing this same bit of sky over and over again for 2 million seconds (almost 23 days) and the results, as you can see, are spectacular. Almost every bit of light you see on the accompanying picture is a galaxy (a collection of millions and, more likely, billions of stars). Some are so far away, light from them is estimated to take 13 billion YEARS to reach us!
This means that when you look at the faintest objects in this picture you are looking almost back to the beginning of time (the Big Bang is estimated to have taken place 13.7 billions years ago.) Some 5,500 galaxies are visible in the small frame of this image and they range in distance and time over billions of lightyears and years. In such images, which are like core samples in geology, astronomers can study the history of structure and matter in the universe.
This means that when you look at the faintest objects in this picture you are looking almost back to the beginning of time (the Big Bang is estimated to have taken place 13.7 billions years ago.) Some 5,500 galaxies are visible in the small frame of this image and they range in distance and time over billions of lightyears and years. In such images, which are like core samples in geology, astronomers can study the history of structure and matter in the universe.
The Hubble scientists have done this before, taking previous sets of deep images called the Hubble Deep Field and then the Hubble Ultra-deep Field. But the current image (above) shows by far the deepest view (seeing the faintest galaxies and light from longest ago.)
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