Results 241 to 250 of about 3,309 (287)
Environmental Changes Recorded in Sedimentary Rocks in the Clay-Sulfate Transition Region in Gale Crater, Mars: Results From the Sample Analysis at Mars-Evolved Gas Analysis Instrument Onboard the Mars Science Laboratory Curiosity Rover. [PDF]
Clark JV +21 more
europepmc +1 more source
Conceptual thermal constraints on the growth of the first tree on a terraformed Mars. [PDF]
Wendland A +6 more
europepmc +1 more source
Sublithospheric diamond constraints on the state of deeply subducted slabs. [PDF]
Zhang Q +11 more
europepmc +1 more source
Rivers of Tears - Convergent, Multi-Scale Approaches to Monitor and Optimize the Health of Our World's Inhabitants. [PDF]
Anderson EJ +6 more
europepmc +1 more source
Life in the brine of Lunenburg, Germany: unveiling microorganisms associated with Zechstein salt deposits. [PDF]
Runzheimer K +8 more
europepmc +1 more source
Some of the next articles are maybe not open access.
Related searches:
Related searches:
Minor Planets: The Discovery of Minor Satellites
Science, 1979The recent confirmation of the discovery of a satellite of the minor planet 532 Herculina indicates that other similar anomalous sightings are probably also due to satellites, which must therefore be numerous and commonplace. There are now 23 candidate satellites for eight minor planets, and no one of these minor planets occulting a star has failed to ...
Richard P Binzel
exaly +3 more sources
Nature, 1977
A hypothesis based on the accretion model of planet formation is proposed which can explain why minor planets could not grow into full-sized planets. Temperature and impact-velocity conditions for bouncing, accumulation, and fragmentation of planetesimals are evaluated for silicate and iron planetesimals at the heliocentric distances of Mercury, Venus,
TAKAFUMI MATSUI, HITOSHI MIZUTANI
openaire +1 more source
A hypothesis based on the accretion model of planet formation is proposed which can explain why minor planets could not grow into full-sized planets. Temperature and impact-velocity conditions for bouncing, accumulation, and fragmentation of planetesimals are evaluated for silicate and iron planetesimals at the heliocentric distances of Mercury, Venus,
TAKAFUMI MATSUI, HITOSHI MIZUTANI
openaire +1 more source

