Tag Archive for 'Magma'

This artist's impression shows the exoplanet Corot-7b, which is so close to its Sun-like host star that it must experience extreme conditions. Image credit: ESO / L. Calcada.

Weather Forecast for Lava Planet K2-141b: Rock Rains and Supersonic Winds

Nov 10, 2020 by News Staff

Using computer simulations, an international team of astronomers has studied the weather conditions on K2-141b, an Earth-size exoplanet with supersonic...

When the Moon formed into a sphere approximately 1,700 km in radius 4.425 billion years ago, its interior heated up considerably due to the energy released when it accreted. The rock melted and an ocean of magma, possibly more than 1,000 km deep, formed. Later, light rocks crystallized, which rose to the surface and formed a first crust on the Moon. This crust insulated the Moon from space, and the magma ocean beneath it cooled down slowly. Around 200 million years would pass before the Moon completely solidified. Image credit: NASA’s Goddard Space Flight Center.

Moon May Be 85 Million Years Younger than Thought

Jul 15, 2020 by News Staff

Earth’s only natural satellite formed 4.425 billion years ago — around 85 million years later than previous estimates, according to a new modeling...

$Illustration showing the present-day hydrogen reservoirs in and on Mars. The mass fractions (pie chart) of Martian water are based on the mass of water in the bulk crust (C), the mantle (M) and the combined inventory (A) of the atmosphere and polar ice deposits (PID). The mantle mass fraction is the combination of depleted shergottites (DS) and enriched shergottites (ES). Image credit: Barnes et al, doi: 10.1038/s41561-020-0552-y.$

Early Mars Had Multiple Water Sources, New Study Shows

Mar 31, 2020 by News Staff

An analysis of two Martian meteorites — Northwest Africa (NWA) 7034 and Allan Hills (ALH) 84001 — shows that Mars likely received water from...

The internal sctructure of Earth. Image credit: NASA / JPL / Université Paris Diderot / Institut de Physique du Globe de Paris.

‘Basal Magma Ocean’ Generated Early Earth’s Magnetic Field, New Research Suggests

Mar 18, 2020 by News Staff

In a new study published in the journal Earth and Planetary Science Letters, a team of researchers from the Scripps Institution of Oceanography at the...

As NASA’s Dawn spacecraft takes off for its next destination, this mosaic synthesizes some of the best views the spacecraft had of the giant asteroid Vesta. Dawn studied Vesta from July 2011 to September 2012. The towering mountain at the south pole -- more than twice the height of Mount Everest -- is visible at the bottom of the image. The set of three craters known as the ‘snowman’ can be seen at the top left. Image credit: NASA / JPL-Caltech / UCLA / MPS / DLR / IDA.

Asteroid Vesta Has Turbulent Past

Mar 5, 2020 by News Staff

A new study by Curtin University researchers has shed light on the early days of Vesta, the second largest asteroid of the main belt and the fourth such...

New Study Looks at Why Neptune-Sized and Larger Exoplanets are Rare

Jan 3, 2020 by News Staff

Sub-Neptunes — extrasolar planets with radii between 2.7 and 3 times that of Earth — are much more numerous than Neptune-sized and larger planets....

The newfound petit-spot volcano near Minamitorishima Island, Japan. Image credit: Tohoku University.

New ‘Petit-Spot’ Volcano Discovered beneath Pacific Ocean

Dec 30, 2019 by Enrico de Lazaro

A team of Japanese scientists has discovered a 3-million-year-old petit-spot submarine volcano in one of the oldest parts of the Pacific Plate. The newfound...

The South Pole-Aitken Basin on the lunar far side is one of the largest and oldest impact features in the Solar System. It’s easily seen in the elevation data. The low center is dark blue and purple. Mountains on its edge, remnants of outer rings, are red and yellow. Image credit: NASA / GSFC / University of Arizona.

Mysterious Mass of Material Discovered Beneath Moon’s South Pole-Aitken Basin

Jun 11, 2019 by News Staff

The South Pole-Aitken basin — the largest crater in the Solar System — is a gigantic impact structure on the far side of the Moon. Data from...

Backscattered electron images of experimental charges. Locations of images (A) to (D) from sediment-peridotite reaction experiments are schematically shown in capsule on the left. (A, C, and D) - reaction experiments at 5 GPa/1000 degrees Celsius with superimposed energy-dispersive x-ray maps of chlorine [green in (C) and (D)]. The sediment half of two-layer experiments recrystallized to garnet and clinopyroxene (Cpx), whereas orthopyroxene (Opx), magnesite (Mgs), and Na-K chlorides formed at the leading edge of the reaction zone against the peridotite. (B) - peridotite layer in the reaction experiment at 3 GPa/900 degrees Celsius contained phlogopite (Phl) behind the magnesite plus orthopyroxene zone, and Na-K chlorides were absent. (E and F) - sediment melting experiment (no peridotite included) at 4 GPa/1000 degrees Celsius showing silicate melt (E) in equilibrium with garnet (Gt), coesite (Coe), and Mg calcite (Mg-Cc) shown in (F). Scale bars - 100 μm (A and B) and 20 μm (C to F). Image credit: Förster et al, doi: 10.1126/sciadv.aau2620.

Study: Salts Trapped inside Fibrous Diamonds Came from Ancient Seabeds

May 31, 2019 by News Staff

So-called fibrous diamonds, which are cloudy and less appealing to jewelers — and less often, gem-quality diamonds — trap and preserve fluids...

The south pole of Mars. Image credit: NASA.

Underground Volcanism on Mars May Have Been Active Extremely Recently

Feb 14, 2019 by News Staff

Recent radar observations from ESA’s Mars Express spacecraft were interpreted as evidence for melting beneath the south polar ice cap of Mars. Now, a...

$Jackson et al propose that magma storage occurs by reactive melt flow in long-lived mush reservoirs, rather than by the commonly invoked process of fractional crystallization in magma chambers. Image credit: Julius Silver.$

Volcanoes are Fed by ‘Mush’ Reservoirs, Says New Study

Dec 5, 2018 by News Staff

Volcanoes are not fed by liquid magma formed in large, underground caves called ‘magma’ chambers; instead, they are fed by so-called ‘mush’ reservoirs...

Mount Etna, with Catania in the foreground. Image credit: Ben Aveling / CC BY-SA 4.0.

Small Volcanic Crystals Could Help Predict Eruptions

Jan 23, 2018 by News Staff

Tiny crystals of clinopyroxenes that form deep in volcanoes may be the key for advance warnings before volcanic eruptions, according to a team of vulcanologists...

This global view of Io was obtained by NASA’s Galileo spacecraft on 19 September 1997 at a range of more than 500,000 km (310,000 miles). In this image, deposits of sulfur dioxide frost appear in white and grey hues while yellowish and brownish hues are probably due to other sulfurous materials. Bright red materials and ‘black’ spots with low brightness mark areas of recent volcanic activity and are usually associated with high temperatures and surface changes. Image credit: NASA / JPL / University of Arizona.

Astronomers Create Detailed Map of Loki Patera, Most Active Volcanic Site on Jupiter’s Moon Io

May 11, 2017 by News Staff

Taking advantage of a rare orbital alignment between Jupiter’s moons Io and Europa, a research team led by scientists at the University of California...

Artist’s conception of early Earth. Image credit: NASA’s Goddard Space Flight Center / Francis Reddy.

Early Earth was Barren, Smooth and Almost Entirely under Water, Research Suggests

May 8, 2017 by News Staff

About 4 billion years ago (Hadean eon), our planet was entirely different than it is now. It was barren, smooth and almost entirely under water with a...

This image from NASA’s Galileo spacecraft shows Io. There are rugged mountains several miles high, layered materials forming plateaus, and many irregular depressions called volcanic calderas. Several of the dark, flow-like features correspond to hot spots, and may be active lava flows. There are no landforms resembling impact craters, as the volcanism covers the surface with new deposits much more rapidly than the flux of comets and asteroids can create large impact craters. The picture is centered on the side of Io that always faces away from Jupiter; north is to the top. Image credit: NASA / JPL / University of Arizona.

Jupiter’s Moon Io May Have Subsurface Magma Ocean

Sep 14, 2015 by News Staff

Io is the Solar System’s most volcanically active planetary body. However, concentrations of volcanic activity are displaced from where they are expected...

Kilauea is the most active of the five volcanoes that together form the island of Hawaii. Image credit: University of Miami Rosenstiel School of Marine & Atmospheric Science.

Scientists Discover Huge Magma Reservoir beneath Kilauea Volcano

Jan 30, 2014 by Natali Anderson

An anomalous magma chamber has been observed at 8–11 km depth beneath the upper east rift zone of one of the world’s most active volcanoes –...

Early Earth. Image credit: Peter Sawyer / Smithsonian Institution.

Basalt Helps Scientists Understand How Earth’s Crust Formed

Nov 7, 2013 by News Staff

European scientists examined liquid basalt at record high pressures and temperatures to better understand how our planet evolved billions of years ago. Early...

Mercury May Have Harbored Magma Ocean in Distant Past

Feb 22, 2013 by Natali Anderson

Planetary scientists at Massachusetts Institute of Technology have proposed that Mercury may have harbored a large ocean of magma shortly after its formation...