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EI2GYB > ASTRO 11.09.21 11:35l 287 Lines 16949 Bytes #999 (0) @ WW
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Subj: Untangling the Tarantula Nebula
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Untangling the Tarantula Nebula, the sky's largest stellar nursery
This vast cosmic cloud gives us a spectacular close-up view of stars bursting
into life.
In 1799, French soldiers unearthed a large black rock near the Egyptian town of
Rosetta (now Rashid) in the Nile delta. Inscribed on its flat face were three
versions of a single decree from 196 b.c. affirming the royalty of 13-year-old
Ptolemy V: one in ancient Greek, one in the everyday language of the Egyptian
people, and one in hieroglyphs. The Rosetta Stone provided the key for
understanding ancient Egyptian hieroglyphics, and ultimately the great
civilization that created them.
Some 50 years before Napoleon's troops found the Rosetta Stone buried in the
ground, another French explorer made an equally stunning discovery not beneath
their feet, but above their heads. In 1751, astronomer Nicolas-Louis de
Lacaille was surveying the deep southern sky from the Cape of Good Hope through
his 1/2-inch refractor when he stumbled upon a small nebula. The object resided
near the northeastern edge of the Large Magellanic Cloud (LMC), the immense
nebulous region that astronomers now recognize as a satellite galaxy to the
Milky Way.
Lacaille cataloged it as a "Nebula of the first kind," meaning he could not see
any star in the nebula through his telescope. In his 1801 star atlas
Uranographia, German astronomer Johann Bode referred to it as 30 Doradus,
reflecting its position in the constellation Dorado the Dolphinfish. It wasn't
until the 20th century that deep photographic exposures taken through
large-aperture scopes revealed the object's spidery tendrils of glowing gas
that inspired its common name: the Tarantula Nebula.
Big, bright, and beautiful
The Tarantula is a giant stellar nursery in the midst of transforming a massive
reservoir of mostly hydrogen gas into hundreds of thousands of stars. The
biggest of these newborn suns are among the most massive known, and they burn
hot and bright, ionizing the surrounding gas and causing it to glow with a
characteristic reddish color.
Although you can use words like big and bright to describe the Tarantula, they
really don't do it justice. The entire nebula spans roughly 1,000 light-years.
For comparison, the Milky Way's Orion Nebula (M42), the finest example of a
star-forming region visible from mid-northern latitudes, is a mere 25
light-years in diameter. And the Tarantula shines brightly enough to see with
the naked eye from the Southern Hemisphere, despite lying some 160,000
light-years from Earth. By contrast, naked-eye M42 is but a stone's throw away
at 1,500 light-years.
To put it another way, if you were to place the Tarantula at the same distance
as the Orion Nebula, it would cover as much sky as 75 Full Moons placed side by
side - enough to stretch 40 percent of the way from the horizon to the zenith.
And it would be bright enough to cast noticeable shadows.
Even where it is, the Tarantula is still close to us in cosmic terms. And that
makes it an enticing target for astronomers. "The Tarantula Nebula is the
region of most intense star formation in the Local Group - a region within
about 10 million light-years of the Sun that includes more than 80 galaxies,"
says astronomer Elena Sabbi of the Space Telescope Science Institute in
Baltimore. "[It's] the only example of a starburst - an extremely intense and
rapid episode of star formation - that we can study in detail."
In fact, astronomers wouldn't necessarily want the Tarantula to be any closer.
Because it lies away from the dust-laden disk of the Milky Way, scientists have
an unobscured view, allowing them to clearly see the objects within it. It's
more difficult to study nearby star-forming hot spots - like the Orion Nebula
and the Carina Nebula (NGC 3372) - because astronomers must view them through
the dusty haze of our galaxy's disk.
"The Tarantula is close enough for us to study individual stars across the
electromagnetic spectrum, from X-rays to infrared, as well as to consider it as
a single nebula," says Paul Crowther of the University of Sheffield in the U.K.
You have to look much farther to see similarly impressive star-forming regions,
he adds, so astronomers can't resolve their individual stars and can study only
their overall properties.
Untangling the Tarantula's web
The Tarantula has enthralled astronomers ever since Lacaille first laid eyes on
it 270 years ago. But the tools needed to decipher the nebula's inner workings
have a much shorter pedigree.
The Hubble Space Telescope has played a leading role in deciphering the
Tarantula. Sabbi leads the Hubble Tarantula Treasury Project (HTTP), a
multiwavelength survey that provides the most accurate census of the nebula's
stars. "HTTP is a high-resolution survey that consists of several filters from
the near ultraviolet, [which is] sensitive to the light coming from the hottest
and most massive stars, to the near infrared, [which] can penetrate thick walls
of dust and reveal where low-mass young stars are still growing," she says.
So far, the census includes 820,000 stars, ranging from monstrosities that tip
the scales at more than 200 solar masses down to stars with just half the mass
of the Sun. "Thanks to Hubble, we can study how high- and low-mass stars
coexist, and if the powerful radiation coming from the massive stars modifies
the normal evolution of their smaller companions," Sabbi says.
Another key player in the study of the Tarantula is the VLT-FLAMES Tarantula
Survey. The survey, led by Chris Evans at the UK Astronomy Technology Centre in
Edinburgh, Scotland, concentrates on the nebula's massive stars.
Evans and three of his colleagues hatched the idea for the survey in late 2007.
They were in Utrecht in the Netherlands, attending a meeting of researchers
studying massive stars in the Milky Way and the Large and Small Magellanic
Clouds using the Fibre Large Array Multi Element Spectrograph, or FLAMES. The
instrument can target more than 100 objects at a time, splitting the light from
each one into its own spectrum to reveal its physical properties.
Evans and his colleagues had been studying massive O-type stars, but they had
precious few examples in their dataset. As they huddled at a local pub, a plan
to enlist FLAMES began to take form.
"We came up with a working idea of: 'Let's try to do everything in the
Tarantula,' " recalls Evans. "That would give us a sample size large enough to
solve many of our problems." They mapped out a rough idea for the survey in the
following weeks and then assembled a proposal for time to use FLAMES on one of
the 8.2-meter telescopes of the European Southern Observatory's Very Large
Telescope (VLT) array in Chile.
"FLAMES provides us with optical spectra of up to 130 objects simultaneously
across a 25' field of the sky," says Evans. That's enough to cover a large
fraction of the Tarantula. "This means that instead of obtaining spectra of
stars one by one in such a rich part of the sky, we can make much more
efficient use of precious VLT time." The observations yield the temperature,
surface gravity, composition, rotation, and line-of-sight velocity of each star.
nto the spider's lair
The Tarantula may seem like a monolithic entity, but the surveys have helped to
show it has many interrelated parts, with several distinct star clusters and
multiple regions of nebulosity. At the nebula's heart lies the impressive star
cluster Radcliffe 136 (R136). Until the 1980s, astronomers suspected that this
intensely bright central region held a single supermassive star that weighed
perhaps 1,000 Suns. That would be quite remarkable, not least because the laws
of physics dictate that no such star could exist.
But as astronomers developed high-resolution imaging techniques and Hubble
soared above Earth's distorting atmosphere, R136's true nature came into focus.
It turns out to be a compact star cluster comprising dozens of O-type
main-sequence stars - the hottest, brightest, and most massive stars that are
still converting hydrogen into helium in their cores - and equally hot and
massive Wolf-Rayet stars, which are characterized by ferocious stellar winds.
No other spot in the known universe contains as many of these stellar
behemoths. "The Tarantula in general, and its dense star cluster R136 in
particular, contain the most massive stars we have currently identified, with
several dozen exceeding over 100 times the mass of our Sun," says Crowther.
"The most extreme likely started their lives with 200 to 300 solar masses, but
they have already slimmed down by 10 to 20 percent in the last million years or
so because they shed weight at an amazing rate." The 10 brightest of these
stars provide nearly 30 percent of the energy ionizing all of the Tarantula's
gas.
The more massive a star, the shorter its lifespan. O-type stars live no more
than a couple of million years before they exhaust their nuclear fuel and
ultimately detonate as supernovae or implode directly into black holes. The
abundance of these heavyweights in R136 suggests it is no more than 1 million
to 2 million years old. Sabbi's team has also discovered a smaller, more
diffuse clump of stars 15 to 20 light-years northeast of R136. This group has
no O-type stars but does hold slightly smaller and cooler B-type stars,
implying it is perhaps a million years older than its neighbor.
The density of stars in this region leads some scientists to speculate whether
it might one day form a globular cluster. Although all of the globulars in the
Milky Way are ancient, dating back to near the birth of our galaxy, the LMC
holds many youthful lookalikes. The volume within about 65 light-years of R136
contains nearly 90,000 solar masses of material, close to the average size of
Milky Way globulars.
Seeing first light
Surrounding R136 lies NGC 2070, the brightest region of nebulosity in the
Tarantula. This is where the bulk of the remaining hydrogen gas resides, and
where stars currently are forming at a furious rate.
The Tarantula's environment isn't quite so hectic beyond NGC 2070's borders.
The nebula apparently came to life 20 to 30 million years ago, when stars
started to turn on some 145 light-years northwest of R136's current location.
This initial surge gave birth to the star cluster Hodge 301. Tens of millions
of years is plenty of time for the most massive stars to explode, and
astronomers estimate between 40 and 60 supernovae have gone off here during the
cluster's lifetime.
The explosions have had two distinct consequences. First, they have cleared out
much of the gas and dust in Hodge 301, affording astronomers a reasonably crisp
view of the cluster. Second, the expanding supernovae shock waves have
compressed gas on the outskirts of NGC 2070, helping to jumpstart star
formation there.
The Tarantula's third major star cluster is NGC 2060. It lies about 290
light-years southwest of R136 and its stars formed roughly 4 million to 6
million years ago, placing it intermediate in age between R136 and Hodge 301.
Although NGC 2060 looks rather dull compared to R136 and is not as well-defined
as Hodge 301, it embraces some of the Tarantula's most notable citizens.
Top of the list has to be the X-ray pulsar PSR J0537-6910. This object formed
when a massive star exploded about 5,000 years ago (as seen from Earth),
leaving behind a rapidly spinning neutron star. Not only is this pulsar the
most energetic one known, but it is also the fastest rotating young pulsar. It
spins once on its axis every 16 milliseconds, more than twice as fast as the
pulsar at the center of the Milky Way's Crab Nebula. The supernova remnant
associated with the stellar explosion, N157B, also can be seen in NGC 2060.
The cluster likewise harbors the fastest rotating normal star, VFTS 102. The
VLT-FLAMES survey found this star's equatorial regions spinning at a rate of
1.4 million mph (2.2 million km/h), or some 300 times faster than the Sun. The
rapid rotation means VFTS 102's shape more closely resembles an M&M than a
sphere.
These three regions tell only part of the Tarantula's story. Massive stars are
spread across the entire region, with some of them apparently flung from their
birthplaces. VFTS 016, for example, is a massive runaway star located well to
the northwest of NGC 2060. Discovered as a fast mover during the initial stages
of the VLT-FLAMES survey, the team only managed to measure its line-of-sight
velocity. Eight years later, the researchers used data from the European Space
Agency's Gaia spacecraft to pin down its speed: 225,000 mph (360,000 km/h)! Its
position and motion indicate it was ejected from R136 about 1.5 million years
ago and has since traversed 375 light-years. The scientists suspect the star
once belonged to a binary system that suffered a rogue encounter with a third
star, launching it on its epic journey.
Probe of the distant universe
Studying massive binary systems in the Tarantula was one of the motivating
forces behind the VLT-FLAMES survey. The results are startling: "We estimate
that at least 50 percent of our targets are in binary systems," says Evans.
"Alongside complementary studies in our own Milky Way, this result has
significantly changed our perspective on stellar evolution."
Close binaries can interact in many ways, he adds. Mass and angular momentum
can be transferred from one star to the other, and eventually the two stars can
merge. "This results in very different evolutionary paths than if [they were]
born as single stars." Some of these systems may develop into binary black
holes and ultimately merge, producing a torrent of gravitational waves like
those from similar systems that astronomers began detecting in 2015. Not
surprisingly, the current record holder for a massive binary system, Melnick
34, resides in the Tarantula. Each of its two components weighs in at about 120
solar masses.
The biggest opportunity to arise from the HTTP has been to study the lifecycle
of a starburst from up close. "The Tarantula Nebula has been forming stars for
the past 30 million years," says Sabbi. "The epicenter of star formation during
this time has moved considerably, and we can see how powerful stellar winds and
violent supernova explosions have shut down star formation in one region of the
Tarantula, just to start it again a few hundred light-years away."
What has happened just recently in the Tarantula may be a window into the
universe's early history. Casting their gaze outward, astronomers detect what
seem to be similar starbursts in galaxies so distant that universal expansion
has shifted their light far toward the red end of the spectrum. "The
Tarantula's properties appear to be comparable to knots of intense star
formation in young galaxies at high redshift, so it gives us a local clue to
galaxy assembly in the early universe," says Crowther.
Using the Tarantula as a model for these systems offers one more advantage over
any potential Milky Way counterparts: The Tarantula and the surrounding LMC
have far fewer heavy elements than star-forming regions in our own galaxy. The
amount of metals - astro-speak for elements heavier than helium that stars have
cooked up over the eons - in the LMC is only half that of the Milky Way, making
it much more similar to the more pristine material present in the distant,
early cosmos. With the Tarantula, it's almost as if astronomers have stumbled
on their own Rosetta Stone, and have started using it as a key to understanding
the mysteries of star and galaxy formation.
Scientists have been fortunate to have front-row seats to the Tarantula's
display. "We're lucky to be witnessing these fireworks when the Large
Magellanic Cloud is on its closest approach to the Milky Way in the last
billion years or so," says Crowther. Alas, the performance may not run that
much longer. "Much of the gas from the original molecular cloud has now turned
into stars, so we expect the rate of star formation to decline in the next few
million years."
When the show eventually ends, every astronomer in the house will say it had a
great run.
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