Astronomers Open Window Into Europa’s Ocean

W. M. Keck Observatory press release

With data collected from the W. M. Keck Observatory, California Institute of Technology (Caltech) astronomer Mike Brown — known as the Pluto killer for discovering a Kuiper-belt object that led to the demotion of Pluto from planetary status — and Kevin Hand from the Jet Propulsion Laboratory (JPL) have found the strongest evidence yet that salty water from the vast liquid ocean beneath Europa’s frozen exterior actually makes its way to the surface.

The data suggests there is a chemical exchange between the ocean and surface, making the ocean a richer chemical environment, and implies that learning more about the ocean could be as simple as analyzing the moon’s surface. The work is described in a paper that has been accepted for publication in the Astronomical Journal.

The findings were derived from spectroscopy delivered from the Keck Observatory, which operates the largest and most scientifically productive telescopes on Earth.

“We now have the best spectrum of this thing in the world,” Brown says. “Nobody knew there was this little dip in the spectrum because no one had the resolution to zoom in on it before.”

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The Moon and Jupiter

This evening sky-watchers will note Jupiter directly beside a bright Moon. The pair will be very close separated by only 1°09′ as of sunset here in Hawai’i. Accounting for the radius of the Moon this will mean that the planet will be only 55′ off the limb of the Moon.

Observers further east and south will be able to see an occultation, with the Moon passing in front of Jupiter. Here in Hawai’i the occultation will be over before sunset. It is no use observing during the daytime either, as the planet will pass north of the Moon for our latitude.

The proximity of the two does provide a nice opportunity to see Jupiter in the daytime, as the Moon will provide a signpost to the location of the planet. The pair will rise about 14:00HST and be well up before sunset. Look just to the north of the Moon (left as they rise) for a pinpoint of light. At -2.6 magnitude the planet should be easy to spot as long as the sky is clear and not hazy.

Adaptive Optics Allows Earth-Based Monitoring of Io’s Fiery Show

W. M. Keck Observatory press release

Watching active volcanic eruptions should be done from a safe distance, and a group of California researchers has figured out how to do it from, ironically, Mauna Kea – one of Earth’s tallest volcanoes – using the W. M. Keck Observatory. Employing an ingenious combination of telescopic surveys and archival data, they have gathered nearly 40 distinct snapshots of effusive (slow) volcanic eruptions and high temperature outbursts on Jupiter’s tiny moon, Io, showing details as small as 100 km (60 miles) on the moon’s surface.

While space-based telescopes were once required for viewing surface details on Io – similar in size to our Moon, but more than 1,600 times distant – adaptive optics (AO), pioneered at Keck, allows teams like that led by Franck Marchis, a researcher at the Carl Sagan Center of the SETI Institute, to collect fascinating data on the wild show from Earth. Marchis presented results from ground-based telescopic monitoring of Io’s volcanic activity over the past decade this week, at the 2012 Division of Planetary Sciences Meeting of the American Astronomical Society.

Erupting volcanoes on Io cannot be seen well from beneath the Earth’s atmosphere using classical astronomical techniques. Io is a relatively small satellite with a 3,600 km diameter, more than 630 million kilometers away. In 1979, Voyager 1 visited the Jovian system, revealing Io’s dynamic volcanic activity from the first close-up pictures of its surface, capturing bizarre volcanic terrains, active plumes and hot spots. The Galileo spacecraft remained in orbit in the Jovian system from 1995 to 2003 and observed more than 160 active volcanoes and a broad range of eruption styles. Several outstanding questions remained in the post-Galileo era, and the origin and long-term evolution of Io’s volcanic activity is still not fully understood.

IO with Keck AO
Quiescent activity of Io observed in 2010 and 2011 showing several quasi-permanent eruptions at 3.8 microns [bottom] and the absence of bright, hotter outbursts at 2.1 microns [top]. Credit: Franck Marchis, SETI Institute

In the meantime, astronomers designed instruments to break the “seeing barrier” and improve the image quality of ground-based telescopes. The blurring (“seeing”) introduced by the constant motion of the Earth’s atmosphere can be measured and corrected in real time using adaptive optics (AO), providing an image with a resolution close to the theoretical “diffraction limit” of the telescope. The W. M. Keck Observatory has used adaptive optics since 1999.

“Since our first observation of Io in 2001 using the Keck II 10-meter telescope and its AO system from Mauna Kea in Hawaii, our group became very excited about the technology. We also began using AO at the Very Large Telescope in Chile, and at the Gemini North telescope in Hawaii. The technology has improved over the years, and the image quality and usefulness of these AO systems have made them part of the essential instrument suite for large telescopes,” said Marchis.

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The Moon and Jupiter

Tomorrow morning, August 11th, will see the Moon quite close to Jupiter. The pair will be a mere 2° apart. A bright Jupiter at -2.2 magnitude will be a nice match for a 33% illuminated Moon.

An even brightener Venus will be located about 22° east of Jupiter, closer to the horizon. You could also look for Mercury, 28° east of Venus and 16° above the horizon at sunrise.

In two more days, on the morning of August 13th, the Moon will rendezvous with Venus, for a closer conjunction, only 1° away from the planet.