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Saturday, December 11, 2010

Transcript: "Is the Universe Infinite?"


Is the Universe Infinite?

Since ancient times, we’ve looked into the night skies and wondered:

How far do the stars stretch out into space?

And what’s beyond them?

In modern times, we built giant telescopes that have allowed us to cast our gaze deep into the universe.

Astronomers have been able to look back to near the time of its birth.

They’ve reconstructed the course of cosmic history in astonishing detail.

From intensive computer modeling, and myriad close observations, they’ve uncovered important clues to its ongoing evolution.

Many now conclude that what we can see, the stars and galaxies that stretch out to the limits of our vision, represent only a small fraction of all there is.

Does the universe go on forever? Where do we fit within it?

And how would the great thinkers have wrapped their brains around the far-out ideas on today’s cutting edge?

To begin to get a handle on infinity, we’re going to need some perspective on the numbers and scales that define our universe.

One place to start is a narrow side street in Charles Dickens’ London.

A Curiosity Shop, fictional to be sure.

Here you can find an unparalleled collection of stuff.

Old shrunken heads, manuscripts, newspapers, books, and rare examples of impressively large numbers.

From Zimbabwe comes a 100 trillion dollar note. In late 2008, with that nation battered by hyperinflation, it was worth about a dollar fifty US.
(http://en.wikipedia.org/wiki/Zimbabwean_dollar)

Go up two orders of magnitude to something decidedly more useful. The fastest supercomputer in history will soon hum along at 20 thousand trillion calculations per second, a twenty followed by 15 zeroes.

You’ll have to run it about a day and a half for your calculations to equal the number of grains of sand on all the world’s beaches. That’s around a sextillion, a ten followed by 22 zeroes.
(http://www.newton.dep.anl.gov/askasci/ast99/ast99215.htm)

That’s roughly the number of stars in the visible universe.

Atoms in the visible universe? That’s upwards of 10 to the 78th power, a 10 with 78 zeroes.
(http://www.universetoday.com/36302/atoms-in-the-universe/)
(http://g42.org/MiscInfo/numbers.html)

Cubic centimeters? A mere ten to the 84th, a septvigintillion.
(http://spacemath.gsfc.nasa.gov/weekly/2page9.pdf)

To go up from there, we turn to no less a source than the Guinness Book of World Records. The largest named number in regular decimal notation: the Buddhist time period Asamkhyeya is ten to the 140th years, or 100 quinto-quadragintillions.

Then there’s the largest number ever used. Graham’s number is a calculation of angles in a type of hypercube.
(http://math.ucsd.edu/~fan/ron/images/guiness.jpg)

If you divided the visible universe into the smallest units known, called Planck volumes, the total of those units wouldn’t get you anywhere close to Graham’s number.
(http://en.wikipedia.org/wiki/Graham's_number)

But it’s still nowhere close to the ultimate ceiling: infinity.

For those who find infinity hard to grasp, even troubling, you’re not alone. It’s a concept that has long tormented even the best minds.

Over two thousand years ago, the Greek mathematician Pythagoras and his followers saw numerical relationships as the key to understanding the world around them.

But in their investigation of geometric shapes, they discovered that some important ratios could not be expressed in simple numbers.
(Aczel, Amir, “The Mystery of the Aleph: Mathematics, the Kabbalah, and the Search for Infinity,” p. 4.)

Take the circumference of a circle to its diameter, called Pi.

Computer scientists recently calculated Pi to 5 trillion digits, confirming what the Greeks learned: there are no repeating patterns and no ending in sight.
(http://www.numberworld.org/misc_runs/pi-5t/details.html)

The discovery of the so-called irrational numbers like Pi was so disturbing, legend has it, that one member of the Pythagorian cult, Hippassus, was drowned at sea for divulging their existence.
(Aczel, Amir, “The Mystery of the Aleph: Mathematics, the Kabbalah, and the Search for Infinity,” p. 5.)

A century later, the philosopher Zeno brought infinity into the open with a series of paradoxes: situations that are true, but strongly counter-intuitive.

In this modern update of one of Zeno’s paradoxes, say you have arrived at an intersection. But you are only allowed to cross the street in increments of half the distance to the other side. So to cross this finite distance, you must take an infinite number of steps.

In math today, it’s a given that you can subdivide any length an infinite number of times, or find an infinity of points along a line.

What made the idea of infinity so troubling to the Greeks is that it clashed with their goal of using numbers to explain the workings of the real world.

To the philosopher Aristotle, a century after Zeno, infinity evoked the formless chaos from which the world was thought to have emerged: a primordial state with no natural laws or limits, devoid of all form and content.
(Wallace, David Foster, “Everything and More: A Compact History of Infinity” p. 44)

But if the universe is finite, what would happen if a warrior traveled to the edge and tossed a spear? Where would it go?

It would not fly off on an infinite journey, Aristotle said. Rather, it would join the motion of the stars in a crystalline sphere that encircled the Earth.
(http://www.jb.man.ac.uk/~jpl/cosmo/infinity.html)

To preserve the idea of a limited universe, Aristotle would craft an historic distinction.

On the one hand, Aristotle pointed to the irrational numbers such as Pi. Each new calculation results in an additional digit, but the final, final number in the string can never be specified. So Aristotle called it “potentially” infinite.
(Wallace, David Foster, “Everything and More: A Compact History of Infinity” p. 65.)

Then there’s the “actually infinite,” like the total number of points or subdivisions along a line. It’s literally uncountable. Aristotle reserved the status of “actually infinite” for the so-called “prime mover” that created the world and is beyond our capacity to understand.
(http://csep10.phys.utk.edu/astr161/lect/retrograde/aristotle.html)

This became the basis for what’s called the Cosmological, or First Cause, argument for the existence of God.
(http://www.allaboutphilosophy.org/cosmological-argument.htm)

Another century later, Archimedes incorporated “actual infinity” into measurements of curved lines and volumes.

His method boils down to a process of summation. Place a triangle inside a circle. Turn it into a square, then a pentagon, and so on. As the number of sides increases, to infinity, their combined lengths equal the circumference of the circle.  

By slicing and dicing curves into an infinite number of straight lines, he was able to compare a variety of curves, areas, and volumes.
(http://www.archimedespalimpsest.org/scholarship_netz2.html)

Archimedes anticipated techniques developed two thousand years later.

And yet, his ideas on infinity did not carry forward, due to what the author David Foster Wallace described as a mathematical allergy to the concept that developed in response to Aristotle’s “potential infinity.”
(Wallace, David Foster, “Everything and More: A Compact History of Infinity” p. 68.)

It was Aristotle’s ideas that passed into the Christian era along with his cosmology, with Earth seated firmly at the center.

That view was not universal. Islamic, Hindu, and even some western thinkers posed alternate views that included infinite space.
(http://veda.wikidot.com/hindu-cosmology)

In European circles, the issue of infinity resurfaced during the Renaissance.

In 1543, the Polish astronomer Nikolas Copernicus argued that Earth orbits the Sun, not the other way around.

The old Greek spheres began to fall by the wayside when a distant supernova, then a comet, were spotted by the astronomer Tycho Brahe. These objects seemed to behave independently of the other stars.

A monk named Giordanno Bruno inflamed the issue by traveling Europe at the height of the Inquisition to proclaim an infinite universe. In the year 1600, he was burned at the stake for this and other heresies.
(http://www.theosophy-nw.org/theosnw/world/modeur/ph-holli.htm)

Just nine years later, in 1609, Galileo Galilee used the first astronomical telescope to show that the universe is much larger than we thought. In later writings, he even sought to discredit the distinction between potential and actual infinity.

Galileo was forced to recant his views, and the old Aristotelian view held sway. Any attempt to assign a value to infinity, in numbers or in nature, was doomed, for that was the unique province of God.
(Dauben, Joseph Warren, “Georg Cantor: His Mathematics and Philosophy of the Infinite.” P. 123)

Finally, at the end of the 19th century, the mathematician Georg Cantor sought once and for all to divorce metaphysics from the abstract pursuit of math.

Infinity, he wrote, had to be studied without “arbitrariness and prejudice.”
(Dauben, Joseph Warren, “Georg Cantor: His Mathematics and Philosophy of the Infinite.” P. 125)

He became known for folding finite and infinite numbers into a unified theory of number sets, considered a foundation of modern math.

One of his defenders used a paradox to show how infinite sets are subject to concrete comparisons.

Say you’ve come to stay at this grand hotel.
(Pickover, Clifford A., “The Math Book: From Pythagoras to the 57th Dimension” p. 354)

You’re in luck, because here there is an infinite number of rooms.

Oddly enough, you learn there are “No Vacancies.”

Fortunately, the manager says: I can still check you in. He assigns you to room #1 and directs you down the corridor. Then, he goes to work, shifting the guest in room 1 to room 2 -- room 2 to 3 -- 3 to 4 -- and so on.

So in this hotel, there’s a number set that includes an infinite number of guests and rooms. Then there’s that same set plus you… two infinite sets, yet one is a subset of the other.

Being able to use infinite sets of different sizes allowed mathematicians to design equations describing continuous motion and change over time.

Echoing Aristotle, a critic of the new set theory suggested that the end of the corridor is still only a potential infinity, with God representing the only actual infinity.

For those who pine for humble accommodations, we’ll recommend an alternative later on.

Even as mathematicians embraced infinity, astronomers in the early 20th century still saw a limited universe… centered on the galaxy, a flat disk of stars.

Did the limits of our vision, like the horizon at sea, conceal an infinite universe beyond?

Albert Einstein, for one, believed that if that were true, then the night sky would be filled with dense starlight shining from every direction. We’d reel from the effects of infinite gravity.

Arguing for a finite universe, he described a people living on the 2D surface of a sphere.

To them, a beam of light moving through space would appear to go straight, on an infinite journey. In fact, it follows a path determined by the overall gravity of the universe, and curves back around.
(Isaacson, Walter, “Einstein: his life and universe” p. 252)

Like the old Greek spheres, this view of a static and limited universe began to fall by the wayside in the 1920s.

Edwin Hubble and Milt Humason used the new 100” telescope on Mt. Wilson in California to look at mysterious fuzzy patches of sky called “nebulae.” They found that these patches were galaxies like our own, and that some were very far away.

What’s more, they found that most are moving away from us. In fact, the farther out they looked, the faster the galaxies are moving.

This fact, known as Hubble’s law, led to an inescapable conclusion: that the universe is expanding. Furthermore, if you run the clock back on this expansion, it appears that it all began in one singular moment.

That moment has traditionally been described as an explosion… a “Big Bang.”

How large the universe has gotten since then depends on how long it’s been growing, and how quickly.

Using an array of modern telescopes, astronomers have recently narrowed the beginning to 13.7 billion years ago. Taking into account the expansion of space ever since, the radius of the visible universe, the part we can see, has expanded out to 46 billion light years.
(Lineweaver, Charles H. and Davis, Tamara M.  “Misconceptions About the Big Bang,” Scientific American: March 2005.)

These measurements have raised anew the ancient questions: What’s beyond our cosmic horizons? Is there an edge? Or does it somehow go on forever?

A new set of answers has emerged from a theory designed to address questions that arose from the original model of the Big Bang.

For one, how did the universe get so large? The Hubble Deep Field contains images of infant galaxies at less than 10% of the age of the universe, near the edge of our cosmic horizons.

By the time one of those galaxies reached maturity, it would have moved far, far beyond our horizon.

And what of all the galaxies visible at its horizons?

For another, how did the universe get so smooth? In every direction you look, the density of galaxies is the same on large scales.

Astronomers believe that whatever process flung the universe outward, must have also blended it in its earliest moments.

The theory that addresses these questions was based on the discovery that energy is constantly welling up from the vacuum of space in the form of particles of opposite charge, matter and anti-matter.

The idea is that in primordial times, an energy field embedded in this so-called quantum vacuum suddenly moved into a higher energy state, causing space and time to literally inflate, and our universe to burst forth.

If this theory is right, then our universe is incomprehensibly large. Its author, the scientist Alan Guth, wrote that the universe as a whole would have grown to at least ten billion trillion times the size of our visible patch. That’s a ten followed by 23 zeroes.
(Guth, Alan.  The Inflationary Universe, Perseus Publishing: 1997, p. 186)

If you think that’s big.

A variation on the theory describes the origin of our universe as a physical process that exists far beyond it, out into the seemingly infinite void that had confounded Aristotle and other Greek thinkers.

In that case, our universe would have inflated like a bubble, and joined a stream of other bubble universes frothing up and expanding across an endless ocean of time and space.

A related idea theorizes a cosmic landscape unfolding in vast fractal patterns.

These new, more expansive, visions of the cosmos are not without their paradoxes.

Logically speaking, with infinite stars, infinite planets, infinite universes, you will also have infinite possibilities. 

The so-called infinite monkey theorum has its roots in Aristotle’s attempts to illustrate the perils of thinking about infinity.
(http://en.wikipedia.org/wiki/Infinite_monkey_theorem)

Ask a monkey to type, or ask an infinite number of monkeys to type, for an infinite amount of time. You’re sure to get a lot of random letters.

But there is a chance, however small, that somewhere, somehow, you’ll get the full text of Shakespeare’s Hamlet.

It’s clearly absurd.

Then again, consider the increasingly strange nature of our universe, as suggested by some new observations.

This is where we draw your attention from the famous Hotel Infinity -- to a less well-appointed alternative.

You’re sure to get a big welcome at the old Hall of Mirrors.

This ramshackle place would have thrown even the great thinkers for a loop.

It represents a kind of optical illusion that may be present in our view of deep space, according to a new interpretation of data from one of the most important space satellites ever launched.

WMAP was sent out to make precision measurements of radiation left over from a period about 300,000 years after the Big Bang.

It revealed an intricate pattern of hot and cold spots, now thought to represent the seeds of galaxy filaments and walls seen on large scales. The pattern was laid down by pressure waves that ricocheted through the expanding gas of the early universe.

One group of scientists, looking at the sizes of these waves, suggested that some are actually mirror images of themselves. From this, they argue that the universe could be much smaller than we think.
(http://physicsworld.com/cws/article/print/23009)

That’s not the only strange new line of evidence.

Tracking the movement of distant galaxies, astronomers found huge clusters moving at about two million miles per hour in the direction of the Constellation Centaurus.
(http://www.sciencedaily.com/releases/2010/03/100310162829.htm)

With the results published in a top scientific journal, the astronomers describe an immense gravitational presence that may loom beyond our visible horizon, perhaps another universe that inflated near our own.
(Here’s possible evidence of the universe before the big bang: http://physicsworld.com/cws/article/news/44388)

Ideas like these may well have led to imprisonment or death in centuries past. Now, they are part of a field of study that is bursting with data and ideas.

Cosmology, the study of the universe as a whole, has long been infused with metaphysics and philosophy. Today, it’s steadily merging into the physical sciences.
(It’s important to note that scientists and the public don’t always see eye to eye: http://pewforum.org/Science-and-Bioethics/Public-Opinion-on-Religion-and-Science-in-the-United-States.aspx)

So is the universe infinite?

Scientists will continue to look for evidence of what lies beyond our horizons and test theories on the nature of time and space. But like the room at the end of an endless corridor, the final final answer will always elude us.


Friday, November 5, 2010

Is the Universe Infinite?

Because our audience has such passion for the subjects we tackle, we thought we'd let them in on our process.  Here is the rough draft of the transcript for our next episode of Cosmic Journeys: "Is the Universe Infinite?" It's about the historic struggle with the concept of infinity from the Greeks to the present. 

We'd love to hear suggestions or corrections. Please cite your sources! Our sources are in the endnotes 
below.




Draft Script: "Is the Universe Infinite?"

How far do the stars stretch? And what’s beyond them?

In modern times, we built giant telescopes that have allowed us to cast our gaze deep into the universe. Astronomers have been able to pinpoint the time of its birth.   They’ve reconstructed the course of cosmic history…. And found clues to its ongoing evolution.

Now, they are beginning to conclude that what we can see… the stars and galaxies on out to the limits of our vision… may represent only a tiny fraction of all there is.

A concept discovered in ancient times… infinity… has reemerged from a long debate about the limits of knowledge...

To challenge long-held views of the cosmos… and of our own place within it.

To begin to get a handle on infinity, we’re going to need some perspective on the numbers and scales that define our universe.

One place to start is a narrow side street in Charles Dickens’ London.  A Curiosity Shop, fictional to be sure.  Here you can find an unparalleled collection of stuff.

Old shrunken heads, Russian manuscripts, Persian rug designs, crumbling newspapers, and odd bits and pieces too numerous to count.  Some can be counted, to a degree.

From Zimbabwe comes this 100 trillion note. In late 2008, with that nation battered by hyperinflation, it was worth about a dollar fifty US.[1]

Go up two orders of magnitude to something a little more useful. The fastest supercomputer in history, due out in 2011, will hum along at 20,000 trillion calculations per second… a twenty followed by 15 zeroes.[2]

You have to run it about a day and a half for your calculations to equal the number of grains of sand on all the world’s beaches. That’s around a sextillion… a ten followed by 22 zeroes.[3]  That’s approximately the number of stars in the visible universe… depending on what assumptions you make.

Atoms in the visible universe? That’s upwards of 10 followed by 78 zeroes, or 10 to the 78th power. [4] [5]

Cubic centimeters? A ten with 84 zeroes, a number that goes by the name of septvigintillion. [6]  Subdivide the visible universe into the smallest units known… called Planck volumes. That’s just over a sexagintillion, a 10 with 185 zeroes.

Even that’s downright tiny compared to the largest number considered to be mathematically useful, according to the Guinness Book of Records.  A calculation of angles in a cube, Graham’s number is so large it doesn’t yield to conventional notation.

Take that number, and square it. Then square the answer.

Now you have a number that’s incomprehensibly large. It’s still nowhere near the ultimate ceiling: infinity.

Today, the idea of infinity is part of a growing link between the physical sciences and cosmology… the study of the universe as a whole that has long been infused with metaphysics and philosophy.

Monday, November 1, 2010

CASSINI Finds One of Saturn's Rings Behaving Like Galaxy

This Press Release coming out of Cassini may interest many of you who enjoyed the recent film "The Curiosity Shop of Saturn's Moons."  Knowledge of Saturn's rings has once again been extended by images taken from NASA's Cassini spacecraft.


Scientists believe they finally understand the perplexing behavior of one of the most dynamic regions in Saturn's rings thanks to images captured by NASA's Cassini spacecraft. And the answer, published
online today in the Astronomical Journal, is:  The rings are behaving like a spiral galaxy.

This new insight, garnered from images of Saturn's most massive ring, the B ring, may, in turn, solve another long-standing puzzle: What causes the bewildering variety of structures seen throughout the very  densest regions of Saturn's rings?

Images of the B ring's outer edge have also revealed at least two perturbed regions, including a long arc of narrow shadow-casting peaks extending as high as 3.5 kilometers (two miles) above the ring plane. The article suggests that these regions are likely populated by small moons that may have migrated across the outer part of the B ring sometime in the past to become trapped near the edge in a zone affected by the gravity of the moon Mimas.  This process is commonly believed to have configured the present-day solar system.

Friday, October 29, 2010

Transcript of The Incredible Journey of Apollo 12

You might not hear about it as much as Apollo 11, but Apollo 12 was one of the most important Apollo flights. This video is the ultimate buddy movie. Forty years ago, on November 19, 1969, astronauts Pete Conrad and Alan Bean landed on the moon. This video shows them making a pinpoint landing on a treacherous lunar surface, finding rocks, and generally having a blast. The program features an interview with Pete Conrad, filmed a year before he died in a tragic motorcycle accident in 1999. Credit Space.com with editorial assistance. All of the sources we used are end-noted.

From The Incredible Journey of Apollo 12 

Earth…. November 14, 1969.1

Three astronauts…2 with spacesuits, food, water, and a battery of scientific and communications equipment… were bound for the moon.

Thousands gathered at the Kennedy Space Center in Florida, including President and Mrs. Richard Nixon, to witness the historic launch.3

The Saturn V rocket that would carry them into space was theoretically designed to launch in any weather… and on this day it was raining.4 

Astronaut and Mission Commander Pete Conrad would say later: “The flight was extremely normal, for the first 36 seconds.”

The five engines of the Saturn 5’s huge first stage burned through 5 million pounds of liquid oxygen in just two and a half minutes, boosting the spacecraft 42 miles up… and 58 miles out over the Atlantic Ocean.5

Racing through the stormy environment, the rocket generated a lightning bolt that traveled down its highly conductive exhaust trail.6

Another bolt hit 16 seconds later. All the spacecraft’s circuit breakers shut off. The tracking system was lost.7

Friday, October 22, 2010

Transcript of How Large is the Universe?



The mind-blowing answer comes from a theory describing the birth of the universe in the first instant of time.  In this video, "How Large is the Universe?", explore the vast expanses of the Universe as far as can be observed and beyond. It delves into big ideas like the Big Bang and Inflation.  How could Dark energy play a role in the expansion of the Universe?   Below is the transcript with all of the sources so you can investigate even further.



From How Large Is the Universe?


The universe has long captivated us with its immense scales of distance and time.

How far does it stretch? Where does it end… and what lies beyond its star fields… and streams of galaxies extending as far as telescopes can see?

These questions are beginning to yield to a series of extraordinary new lines of investigation… and technologies that are letting us to peer into the most distant realms of the cosmos…

But also at the behavior of matter and energy on the smallest of scales.

Remarkably, our growing understanding of this kingdom of the ultra-tiny, inside the nuclei of atoms, permits us to glimpse the largest vistas of space and time.1 

In ancient times, most observers saw the stars as a sphere surrounding the earth, often the home of deities.2

The Greeks were the first to see celestial events as phenomena, subject to human investigation… rather than the fickle whims of the Gods.

One sky-watcher, for example, suggested that meteors are made of materials found on Earth… and might have even come from the Earth.3

Those early astronomers built the foundations of modern science. But they would be shocked to see the discoveries made by their counterparts today.

The stars and planets that once harbored the gods are now seen as infinitesimal parts of a vast scaffolding of matter and energy extending far out into space.

Just how far… began to emerge in the 1920s. Working at the huge new 100-inch Hooker Telescope on California’s Mt. Wilson,4A astronomer Edwin Hubble, along with his assistant named Milt Humason, analyzed the light of fuzzy patches of sky… known then as nebulae.4B

They showed that these were actually distant galaxies far beyond our own.5

Hubble and Humason discovered that most of them are moving away from us.  The farther out they looked, the faster they were receding.6

This fact, now known as Hubble’s law, suggests that there must have been a time when the matter in all these galaxies was together in one place.7

That time… when our universe sprung forth… has come to be called the Big Bang.8

How large the cosmos has gotten since then depends on how long its been growing… and its expansion rate.

Recent precision measurements gathered by the Hubble space telescope and other instruments have brought a consensus…

That the universe dates back 13.7 billion years.9

Its radius, then, is the distance a beam of light would have traveled in that time … 13.7 billion light years. 10

That works out to about 1.3 quadrillion kilometers.11

In fact, it’s even bigger…. Much bigger. How it got so large, so fast, was until recently a deep mystery.12

Thursday, October 21, 2010

The Most Distant Galaxy Ever Measured



A European team of astronomers using ESO's Very Large Telescope (VLT) has measured the distance to the most remote galaxy so far. By carefully analyzing the very faint glow of the galaxy they have found that they are seeing it when the Universe was only about 600 million years old (a redshift of 8.6). These are the first confirmed observations of a galaxy whose light is clearing the opaque hydrogen fog that filled the cosmos at this early time. See the SpaceRip video posted here.

Studying these first galaxies is extremely difficult. By the time that their initially brilliant light gets to Earth they appear very faint and small. Furthermore, this dim light falls mostly in the infrared part of the spectrum because its wavelength has been stretched by the expansion of the Universe -- an effect known as redshift.  To make matters worse, at this early time, less than a billion years after the Big Bang, the Universe was not fully transparent and much of it was filled with a hydrogen fog that absorbed the fierce ultraviolet light from young galaxies. The period when the fog was still being cleared by this ultraviolet light is known as the era of reionization [1].  Despite these challenges, the new Wide Field Camera 3 on the NASA/ESA Hubble Space Telescope discovered several robust candidate objects in 2009 [2] that were thought to be galaxies shining in the era of reionization. Confirming the distances to such faint and remote objects is an enormous challenge and can only reliably be done using spectroscopy from very large ground-based telescopes [3], by measuring the redshift of the galaxy's light.

THE MOST MASSIVE STRUCTURES OF THE UNIVERSE



Using the South Pole Telescope, astronomers have discovered the most massive galaxy cluster yet seen at a distance of 7 billion light-years. The cluster (designated SPT-CL J0546-5345) weighs in at around 800 trillion Suns, and holds hundreds of galaxies.

"This galaxy cluster wins the heavyweight title. It's among the most massive clusters ever found at this distance," said Mark Brodwin, a Smithsonian astronomer at the Harvard-Smithsonian Center for Astrophysics. Brodwin is first author on the paper announcing the discovery, which appeared in the Astrophysical Journal.

Redshift measures how light from a distant object has been stretched by the universe's expansion. Located in the southern constellation Pictor (the Painter), the cluster has a redshift of z=1.07. This puts it at a distance of about 7 billion light-years, meaning we see it as it appeared 7 billion years ago, when the universe was half as old as now and our solar system didn't exist yet.

Even at that young age, the cluster was almost as massive as the nearby Coma cluster. Since then, it should have grown about four times larger. If we could see it as it appears today, it would be one of the most massive galaxy clusters in the universe.