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Image Gallery : Astrochemistry

The study of molecules and chemical reactions in space. This primarily involves chemical interactions of gas and dust surrounding young stars and in interstellar space.

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These images from the Atacama Large Millimeter/submillimeter Array (ALMA) show where various gas molecules were found in the disc around the IRS 48 star, also known as Oph-IRS 48. The disc contains a cashew-nut-shaped region in its southern part, which traps millimetre-sized dust grains that can come together and grow into kilometre-sized objects like comets, asteroids and potentially even planets. Recent observations spotted several complex organic molecules in this region, including formaldehyde (H2CO; orange), methanol (CH3OH; green) and dimethyl ether (CH3OCH3; blue), the last being the largest molecule found in a planet-forming disc to date. The emission signaling the presence of these molecules is clearly stronger in the disc’s dust trap, while carbon monoxide gas (CO; purple) is present in the entire gas disc. The location of the central star is marked with a star in all four images. The dust trap is about the same size as the area taken up by the methanol emission, shown on the bottom left.
Molecules in the disc around the star IRS 48more_horiz
These science images show the molecular lines and dust continuum seen in ALMA observations of the pair of early massive galaxies known as SPT0311-58. On left: A composite image combining the dust continuum with molecular lines for H20 and CO. On right: The dust continuum seen in red (top), molecular line for H20 shown in blue (2nd from top), molecular line transitions for carbon monoxide, CO(6-5) shown in purple (middle), CO(7-6) shown in magenta (second from bottom), and CO(10-9) shown in pinks and deep blue (bottom).
Dust Continuum and Molecular Transition Lines for SPT0311-58more_horiz
This animated gif moves through the dust continuum and molecular lines for water and carbon monoxide seen in ALMA observations of the pair of early massive galaxies known as SPT0311-58. This gif begins with a composite combining the dust continuum with molecular lines for H20 and CO. It is followed by the dust continuum seen in red, molecular lines for H20 seen in blue, molecular lines for carbon monoxide, CO(10-9) shown in pinks and deep blue, CO(7-6) shown in magenta, and CO(6-5) shown in purple.
Animated Composite View of SPT0311-58more_horiz
This artist’s conception shows the dust continuum and molecular lines of carbon monoxide and water seen in the pair of galaxies known as SPT0311-58. ALMA data reveals abundant CO and H20 in the larger of the two galaxies, indicating that the molecular Universe was going strong shortly after the elements were initially forged.
Artist’s conception of SPT0311-58more_horiz
This image may look spooky to you, but astronomers see a galaxy. It was captured by the Very Large Array (VLA) as part of the Local Group L-Band Survey (LGLBS) and is an atomic gas emission image of the nearby galaxy IC 1613.
A Spooky View of Galactic Gasmore_horiz
a bright blue young star with a cloud of cold gas surrounding it
Hydrogen Cyanide in HD 163296more_horiz
ALMA has detected sodium chloride emanating from the dusty disk surrounding ORION SOURCE I
Salt Discovered Around Massive Young Star postermore_horiz
Composite image of Abell 2597
A Molecular Fountain In Abell 2597more_horiz
SPT2319-55
ALMA Observes Most Distant Galactic Outflowmore_horiz
Chart comparing ALMA and Herschel spectral line detections
Spectral Lines in the Cat’s Paw Nebulamore_horiz
Composite image of NGC 6334I
Heavy Water in NGC 6334Imore_horiz
Illustration highlighting ALMA's high-frequency observing capabilities
ALMA’s Highest-Frequency Capabilitiesmore_horiz
Composite image of CK Vul
Pair of Colliding Stars Spill Radioactive Molecules into Spacemore_horiz
Artist impression of the collision of two stars
Artist Impression of CK Vulmore_horiz
Composite image of CK Vul
First Detection of Aluminium Nuclear Isotope in Spacemore_horiz
Galaxy cluster MACS J1149.5+2223, inset image: galaxy MACS1149-JD1
ALMA Finds Most-Distant Oxygen in the Universemore_horiz
Image illustrating the detection of molecules found by ALMA in the Large Magellanic Cloud
Stellar Embryos in Nearby Dwarf Galaxy Contain Surprisingly Complex Organic Moleculesmore_horiz
Still from video explaining the discovery of benzonitrile in interstellar space
GBT Detection Unlocks Exploration of ‘Aromatic’ Interstellar Chemistrymore_horiz
Showing images 1 - 18 of 41

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