A new image from the Atacama Pathfinder Experiment (APEX) telescope in Chile shows a beautiful view of clouds of cosmic dust
in the region of Orion, typical of dust clouds throughout the Universe
that have recently been discovered to incubate the comlpex organic
building blocks of life. While these dense interstellar clouds seem dark
and obscured in visible-light observations, APEX’s LABOCA camera can
detect the heat glow of the dust and reveal the hiding places where new
stars are being formed. But one of these dark clouds is not what it
seems.
In space, dense clouds of cosmic gas and dust are the birthplaces of new
stars. In visible light, this dust is dark and obscuring, hiding the
stars behind it. So much so that, when astronomer William Herschel
observed one such cloud in the constellation of Scorpius in 1774, he
thought it was a region empty of stars and is said to have exclaimed,
"Truly there is a hole in the sky here!"
In order to better understand star formation, astronomers need
telescopes that can observe at longer wavelengths, such as the
submillimetre range, in which the dark dust grains shine rather than
absorb light. APEX, on the Chajnantor Plateau in the Chilean Andes, is
the largest single-dish submillimetre-wavelength telescope operating in
the southern hemisphere, and is ideal for astronomers studying the birth
of stars in this way.
Located in the constellation of Orion (The Hunter), 1500 light-years away from Earth, the Orion Molecular Cloud Complex is the closest region of massive star formation to Earth, and contains a treasury of bright nebulae,
dark clouds and young stars. The new image shows just part of this vast
complex in visible light, with the APEX observations overlaid in
brilliant orange tones that seem to set the dark clouds on fire. Often,
the glowing knots from APEX correspond to darker patches in visible
light — the tell-tale sign of a dense cloud of dust that absorbs visible
light, but glows at submillimetre wavelengths, and possibly a site of
star formation.
The bright patch below of the centre of the image is the nebula NGC 1999.
This region — when seen in visible light — is what astronomers call a
reflection nebula, where the pale blue glow of background starlight is
reflected from clouds of dust. The nebula is mainly illuminated by the
energetic radiation from the young star V380 Orionis lurking
at its heart. In the centre of the nebula is a dark patch, which can be
seen even more clearly in a well-known image from the NASA/ESA Hubble
Space Telescope.
Normally, a dark patch such as this would indicate a dense cloud of
cosmic dust, obscuring the stars and nebula behind it. However, in this
image we can see that the patch remains strikingly dark, even when the
APEX observations are included. Thanks to these APEX observations,
combined with infrared observations from other telescopes, astronomers
believe that the patch is in fact a hole or cavity in the nebula,
excavated by material flowing out of the star V380 Orionis. For once, it
truly is a hole in the sky!
The region in this image is located about two degrees south of the large and well-known Orion Nebula (Messier 42), which can be seen at the top edge of the wider view in visible light from the Digitized Sky Survey.
Recent discoveries in vast interstellar dust clouds
permeating the universe and in nebula have revealed hints of organic
matter that could be created naturally by stars, according to
researchers in a 2011 study at the University of Hong Kong. The discovery team observed stars at different evolutionary phases and found that they are able to produce complex organic compounds and eject them into space, filling the voids between stars.
The compounds are so complex that their chemical structures resemble the makeup of coal and petroleum, the study's lead author, Sun Kwok of
the University of Hong Kong, said. Kwok and his colleague Yong Zhang,
also of the University of Hong Kong, studied a set of well-known but
mysterious infrared emissions found in stars, interstellar space and
galaxies. These phenomena, which are collectively called Unidentified
Infrared Emission (UIE) features, have been known for 30 years, but the
exact source of the emissions has not been identified, and remains a
broad assumption.
Such chemical complexity was thought to arise only from living
organisms, but the results of the new study show that these organic
compounds can be created in space even when no life forms are present.
In fact, such complex organics could be produced naturally by stars, and
at an extremely rapid pace.
"What impressed me most is that complex organics are easily formed by
stars, they are everywhere in our own galaxy and in other galaxies,"
Kwok told Space.com. "Nature is much more clever than we had imagined."
"In the astronomy community, it has been commonly assumed that the
UIE features are emitted by (polycyclic aromatic hydrocarbon, or PAH)
molecules, which are simple, purely aromatic, molecules made of carbon
and hydrogen," Kwok said. Their findings have overturned this
assumption.
Kwok and Zhang analyzed data from the European Space Agency's Infrared Space Observatory and NASA's Spitzer Space Telescope to show that the Unidentified Infrared Emission features are not emitted by PAH molecules because the emissions have chemical structures that are far more complex.
Kwok and Zhang analyzed data from the European Space Agency's Infrared Space Observatory and NASA's Spitzer Space Telescope to show that the Unidentified Infrared Emission features are not emitted by PAH molecules because the emissions have chemical structures that are far more complex.
"I have been suspecting this for many years," Kwok said. "Now we think we have the evidence."
The researchers observed stars at different phases of stellar evolution — first low- to medium-mass stars, then stars in the protoplanetary nebula phase, which is a short-lived episode during a star's rapid evolution, and finally stars in the planetary nebula phase, which is characterized by an expanding shell of ionized gas that is ejected by certain types of stars late in their life.
Kwok and his colleague found that characteristics of the Unidentified
Infrared Emission features could not be detected in low- to medium-mass
stars. But, the astronomers found that the emissions began to appear in
stars in the protoplanetary nebula stage and grew stronger as the stars
matured into the planetary nebula phase.
"Since we know their dynamical and evolutionary ages of these objects
(dynamical age is how fast the nebula will disperse, and evolutionary
age is how fast the star is evolving), we can put constraints on the
chemical time scales," Kwok said. "Since the dynamical/evolution ages
are of the order of thousands of years, the appearance of the spectral
features suggests that the organic compounds are made on time scales
shorter than thousands of years."
"Their spectra changed from a pure gas spectrum to a dust spectrum on
a matter of days or weeks," Kwok added. "The sudden appearance of the
features suggests that organic dust can be made extremely quickly."
The image at the top of the page shows the long tail of interstellar
dust shines in the reflected light of stars in this view of a nebula in
the constellation Corona Australis (the southern crown). In some parts
the dust accumulates to form dense molecular clouds from which it is
thought young stars are born.
Image credit: NASA / JPL-Caltech / SSI and David Malin.
Source: The Daily Galaxy via ESO, nature.com and space.com
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