It was 1980 at the Siding Spring Observatory — just outside Coonabarabran, New South Wales, Australia — when Keith Taylor and Mike Scarrott first discovered the nebula. Due to telescopic limitations at the time, the astronomers saw merely a slight asymmetry in its lobes suggesting a curved shape like was likened to (fittingly) a boomerang. From this, the object got its name…the Boomerang Nebula.
It turns out, they discovered the coldest place in the known universe.
The temperature is so frigid that not even the woolliest of cardigans will save you. Here, particles approach the quantum minimum of speed as there is no major interior heat for the particles to absorb. The frigid temps reach one degree Kelvin.
Just to get an idea of how chilly that is, at absolute zero (-460 degrees Fahrenheit or -273 degrees Celsius), all atomic motion comes to a standstill since the cooling process has extracted all the particles’ energy. Not even a presidential tweet can move.
The Boomerang Nebula lies 5,000 light-years away from Earth in the constellation Centaurus. At just one degree Kelvin (–457.87 degrees Fahrenheit / –272.15 degrees Celsius), it is colder than the background temperature of space itself, which is generally believed to hover around 2.7 Kelvin (-454.81 degrees Fahrenheit / -270.7 degrees Celsius).
Since Taylor and Scarrot made their discovery, further observations have shown it to be a preplanetary nebula — a sun-like star in its golden years of life when the center nears its timely end and expands the nebula with rapidly outpouring gas.
This outflow from Boomerang is expanding at around 310,000 mph (500,000 kph), and cooling itself in the process. This is similar in principle to the way refrigerators use expanding gas to produce cold temperatures. The researchers were able to take the temperature of the gas in the nebula by seeing how it absorbed the cosmic microwave background radiation, which has a very uniform temperature of 2.8 degrees Kelvin (-455 degrees Fahrenheit / -270.56 Celsius).
Astronomers using the Atacama Large Millimeter/submillimeter Array (ALMA) telescope in Chile took a new look at this object in 2013 to learn more about its frigid properties and to determine its true shape, an eerily ghost-like appearance.
“This ultra-cold object is extremely intriguing and we’re learning much more about its true nature with ALMA,” said Raghvendra Sahai, a researcher and principal scientist at NASA’s Jet Propulsion Laboratory in Pasadena, Calif., and lead author of a paper published in the Astrophysical Journal. “What seemed like a double lobe, or boomerang shape, from Earth-based optical telescopes, is actually a much broader structure that is expanding rapidly into space.”
When the Aussies originally observed it with ground-based telescopes, the nebula appeared lopsided, but later observations in 2005 with NASA’s Hubble Space Telescope revealed a bow-tie-like structure — so shaped as the gas is ejected at high speed. The new ALMA data, however, reveal that the Hubble image tells only part of the story, and the twin lobes seen in that image may actually be a trick of light as seen at visible wavelengths.
Researchers should have been able to see this bow tie shape at cooler wavelengths as well, but observations with other submillimeter telescopes revealed a somewhat different shape. ALMA, which has the highest resolution yet at the submillimeter wavelength, managed to solve the mystery.
Carbon monoxide molecules in the nebula’s cloud — very bright in this wavelength of light — were in the hourglass shape in the inner parts of the nebula. Further on out, the molecules were in a rounder shape. Meanwhile, dust grains around the star — also visible in millimeter wavelengths — were masking some of the star’s light in visible wavelengths, making it appear as an hourglass.
“When astronomers looked at this object in 2003 with Hubble, they saw a very classic ‘hourglass’ shape,” commented Sahai. “Many planetary nebulae have this same double-lobe appearance, which is the result of streams of high-speed gas being jettisoned from the star. The jets then excavate holes in a surrounding cloud of gas that was ejected by the star even earlier in its lifetime as a red giant.”
Researchers using ALMA also found a dense lane of millimeter-sized dust grains that surrounded the star, explaining why this outer cloud has an hourglass shape in visible light. The dust grains created a mask that shades a portion of the central star and allows its light to leak out only in narrow but opposite directions into the cloud, giving it an hourglass appearance.
Astronomers say that the Boomerang Nebula is on its way to becoming a planetary nebula — a central star which becomes a white dwarf, causing the nebula to glow.
So far, the Boomerang is the only preplanetary nebula that we know off whose temperature has dropped below that of the Big Bang’s afterglow.
The term “planetary nebula” is arguably a misnomer because they are unrelated to planets or exoplanets. The true origin of the term was likely derived from the planet-like round shape of these nebulae as observed by astronomers through early telescopes, and although the terminology is inaccurate, it is still used by scientists.
The vocabulary’s most likely first introduction was during the 1780s with the English astronomer William Herschel who described these nebulae as resembling planets. However, as early as January 1779, the French astronomer Antoine Darquier de Pellepoix described in his observations the Ring Nebula as “very dim but perfectly outlined; it is as large as Jupiter and resembles a fading planet”.
The preplanetary nebula phase is a short period in the cycle of stellar evolution, and has nothing to do with planets. Over a few thousand years, the hot remains of the aging star in the center of the nebula heat it up, excite the gas, and make it glow as a subsequent planetary nebula. The short lifespan of preplanetary nebulae means there are relatively few of them in existence at any one time. Moreover, they are very dim, requiring powerful telescopes to be seen. This combination of rarity and faintness means they were only discovered comparatively recently. The Egg Nebula, the first to be discovered, was first spotted less than 40 years ago.
The coldest thing in the universe
It is worth noting that the Boomerang Nebula is the coldest natural place in the universe. The award for coldest actual place is in a Cambridge, Massachusetts lab at the Massachusetts Institute of Technology (MIT).
There Wolfgang Ketterle and a team of researchers managed to cool a sodium gas to only half-a-billionth of a degree above absolute zero in 1995. It is the first time that a gas was cooled below 1 nanokelvin (one-billionth of a degree).
“To go below one nanokelvin is a little like running a mile under four minutes for the first time,” said the Nobel laureate Ketterle, co-leader of the team. Ketterle is MIT’s John D. MacArthur Professor of Physics.
In their achievement, the MIT team — which had paired up with a group of researchers from the University of Colorado at Boulder — discovered a new form of matter, the Bose-Einstein condensate, where the particles march in lockstep instead of flitting around independently.
Since the team’s breakthrough, many groups across the globe now routinely reach nanokelvin temperatures; the lowest temperature reported prior was nanokelvin. The record set by the MIT group is 500 picokelvin, or six times lower.
In the future, NASA is planning to operate an apparatus onboard the International Space Station, called the Cold Atom Laboratory. The device combination of lasers and magnets will be used to chill and slow a cloud of atoms to just one-tenth of a billion of a degree above absolute zero.
At such low temperatures, atoms cannot be kept in physical containers, because they would stick to the walls. Furthermore, no known container can be cooled to such temperatures. Therefore, the atoms are surrounded by magnets, which keep the gaseous cloud confined. “In an ordinary container, particles bounce off the walls. In our container, atoms are repelled by magnetic fields,” explained physics graduate student Aaron Leanhardt.
To reach their temps, the MIT researchers came up with a novel way of confining atoms, which they called a “gravito-magnetic trap.” As the name indicates, the magnetic fields act together with gravitational forces to keep the atoms trapped.
So there you go, two of the coldest places in the universe. Cool, huh?
