ESO ALMA: Chile Earthquake Leaves Astronomy Observatories Unscathed

The epicenter for the 8.2 earthquake that rocked Chile on Tuesday was approximately 310 miles (500 km) from the Very Large Telescope and ALMA.

Credit: ESO

The massive earthquake that struck Chile on Tuesday (April 1) left three main European-built observatories in the region relatively untouched despite causing damage and a tsunami along the country's western coast.

The powerful 8.2-magnitude earthquake struck about 60 miles (95 kilometers) northwest of the coastal city Iquique, causing several landslides and triggering a tsunami that rose some 7 feet (2.1 meters).

The earthquake struck at 8:46 p.m. local time (7:46 EDT).

A powerful 7.6-magnitude aftershock rattled the area late Wednesday night (April 2).

The European Southern Observatory (ESO) operates three major observatories in Chile, each with multiple telescopes: the Paranal Observatory, which is home to Europe's Very Large Telescope; the La Silla Observatory, which hosts various telescopes, such as the 2.2-m Max-Planck telescope, 1.2-m Swiss Leonhard Euler Telescope and the 1.5-m Danish Telescope; and ALMA and APEX, or the Atacama Large Millimeter/submillimeter Array and the Atacama Pathfinder Experiment. (Also in the Chajnantor region is Caltech's Chajnantor Observatory.)

The epicenter was located approximately 310 miles (500 km) from both the ALMA/APEX and Paranal sites.

"The quake was felt at the ALMA camp as a prolonged swaying, which lasted for about 2 minutes," the ALMA Observatory said in a statement.

However, none of the ESO facilities reported any damage.

ESA /ESO APEX Image: Setting the Dark on Fire

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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 [2] lurking at its heart.

In the centre of the nebula is a dark patch, which can be seen even more clearly in this 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.