| DATE POSTED |
ARTICLES |
| 25 JUNE 09
|
The Complicated Geologic History of Asteroid 4 Vesta
by G. Jeffrey Taylor
Meteorites from asteroid 4 Vesta show that it contains patches of granite-like rock. |
PSRD-Vesta.granite-like.pdf |
| 19 FEB 09
|
More Evidence for Multiple Meteorite Magmas
by G. Jeffrey Taylor
Cosmochemists show that a pair of meteorites formed in an asteroid that erupted a newly-recognized type of asteroidal magma. |
PSRD-asteroidalMagmas.pdf |
| 8 JULY 08
|
Heating, Cooling, and Cratering: One Asteroid's Complicated Story
by G. Jeffrey Taylor
Cooling rate data indicate that the H-chondrite parent asteroid was deeply cratered as it cooled slowly. |
PSRD-H-chondrite-parent.pdf |
| 27 NOV 07
|
Getting to Know Vesta
by Linda M. V. Martel
Scientists are primed with geochemical data from HED meteorites for Dawn's encounter with asteroid 4 Vesta. |
PSRD-HEDs-Vesta.pdf |
| 17 SEPT 07
|
Melted Crumbs from Asteroid Vesta
by Linda M. V. Martel
Researchers studying some of the rarest of the smallest meteorites call them melted crumbs from asteroid Vesta. |
PSRD-cosmicSpherules.pdf |
| 18 APRIL 07
|
When Worlds Really Did Collide
by Edward Scott, Jijin Yang, and Joseph Goldstein
Cosmochemical studies and dynamical models of protoplanetary collisions suggest a new origin for iron meteorites. |
PSRD-irons.pdf |
| 27 NOV 06
|
Hit-and-Run as Planets Formed
by G. Jeffrey Taylor
Collisions between large protoplanets as the planets formed may have ripped some of them to shreds, producing molten asteroid-sized bodies, driving off water and other volatiles, and scrambling partially molten protoplanets. |
PSRD-hit-and-run.pdf |
| 21 JULY 06
|
Iron Meteorites as the Not-So-Distant Cousins of Earth
by William F. Bottke and Linda M. V. Martel
Numerical simulations suggest that some iron meteorites are fragments of the long lost precursor material that formed the Earth and other terrestrial planets. |
PSRD-asteroidGatecrashers.pdf |
| 2 APRIL 04
|
Asteroid Heating: A Shocking View
by G. Jeffrey Taylor
Mineral intergrowths in chondritic meteorites may indicate that some asteroids were heated by impact. |
PSRD-asteroidHeating.pdf
|
| 9 MAR 04 |
Tiny Traces of a Big Asteroid Breakup
by Linda M. V. Martel
Fossil meteorites and chromite grains record a hundred-fold increase in the number of meteorites that fell 480 million years ago compared to the meteorite influx today. |
PSRD-fossilMeteorites.pdf
|
| 28 APRIL 03 |
Asteroidal Lava Flows
by G. Jeffrey Taylor
Meteorite studies indicate that we have pieces of lava flows from at least five asteroids.
|
PSRD-asteroidalLava.pdf
|
| 23 JAN 03 |
QUE 93148: A Part of the Mantle of Asteroid 4 Vesta?
by Christine Floss
A tiny meteorite tells a story of melting in the deep mantle of a big asteroid.
|
PSRD-QUE93148.pdf
|
| 28 JUNE 02 |
Using Chondrites to Understand
the Inside of Asteroid 433 Eros
by Linda M. V. Martel
Data from ordinary chondrite meteorites and from the NEAR mission suggest that asteroid 433 Eros is heavily fractured.
|
PSRD-ErosPorosity.pdf
|
| 26 FEB 02 |
The Composition of Asteroid 433 Eros
by G. Jeffrey Taylor
X-rays and reflected light suggest that asteroid 433 Eros is similar in composition to the most common type of meteorite--maybe. |
PSRD-eros.pdf
|
| 3 DEC 01 |
Oxygen Isotopes Give Clues to the Formation of Planets, Moons, and Asteroids
by Edward R. D. Scott
As they formed from gas and dust near the Sun, grains in some meteorites acquired oxygen that originated in numerous other stars that shone long before our solar system was born. |
PSRD-Oisotopes.pdf
|
| 21 NOV 00 |
Mining the Moon, Mars, and Asteroids
by G. Jeffrey Taylor
Applied cosmochemistry plays a key role in plans to use the resources of the Moon, Mars, and asteroids. |
PSRD-mining.pdf
|
| 17 DEC 99 |
Difficult Experiments on Weird Rocks
by G. Jeffrey Taylor
Melting experiments on oxygen-depleted meteorites give clues about magma compositions and core formation in asteroids. |
PSRD-indarch.pdf
|
| 24 AUG 99 |
Honeycombed Asteroids
by G. Jeffrey Taylor
Asteroids have lower densities than expected, probably because they have been disrupted and then reassembled into porous rubble piles. |
PSRD-asteroidDensity.pdf
|
| 8 FEB 99 |
From a Cloud of Gas and Dust to an Asteroid with Percolating Hot Water
by G. Jeffrey Taylor
Isotopes of manganese and chromium indicate that chemical reactions involving hot water altered minerals on water-bearing asteroids during the same time interval that other asteroids were melted, between 7 and 16 million years after the first solids formed in the Solar System. |
PSRD-fayalite.pdf
|
| 12 NOV 98 |
Dry Droplets of Fiery Rain
by G. Jeffrey Taylor
Experiments test an idea for the origin of droplets of rocky material melted before the planets formed. |
PSRD-chondrules.pdf
|