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The Orbiting Carbon Observatory (OCO) mission
- D. Crisp, R. Atlas, S. Schroll
- Environmental Science
- 1 December 2004
Chondrites as samples of differentiated planetesimals
- L. Elkins‐Tanton, B. Weiss, M. Zuber
- Geology, Physics
- 1 March 2009
Ferromagnetic resonance and low-temperature magnetic tests for biogenic magnetite
- B. Weiss, S. Kim, A. Komeili
- Geology
- 30 July 2004
The Constitution and Structure of the Lunar Interior
- M. Wieczorek, B. Jolliff, B. Bussey
- Geology
- 2006
The current state of understanding of the lunar interior is the sum of nearly four decades of work and a range of exploration programs spanning that same time period. Missions of the 1960s including…
The lunar dynamo
It has now been established that a dynamo magnetic field likely existed on the Moon from at least 4.5 billion to 3.56 billion years ago, with an intensity similar to that at the surface of Earth today.
Records of an ancient Martian magnetic field in ALH84001
- B. Weiss, H. Vali, F. Baudenbacher, J. Kirschvink, S. Stewart, D. Shuster
- Geology, Physics
- 1 March 2001
The bombardment history of the Moon as recorded by 40Ar‐39Ar chronology
- V. Fernandes, J. Fritz, B. Weiss, I. Garrick‐Bethell, D. Shuster
- Geology
- 1 February 2013
New petrography and 40Ar‐39Ar ages have been obtained for 1–3 mm sized rock fragments from Apollo 16 Station 13 soil 63503 (North Ray crater ejecta) and chips from three rocks collected by Apollo 16…
Geology of Lonar Crater, India
- A. Maloof, S. Stewart, P. M. Poussart
- Geology
- 2010
Lonar Crater, India, is one of the youngest and best preserved impact structures on Earth. The 1.88-km-diameter simple crater formed entirely within the Deccan traps, making it a useful analogue for…
A low temperature transfer of ALH84001 from Mars to Earth.
- B. Weiss, J. Kirschvink, J. Wikswo
- Geology, PhysicsScience
- 27 October 2000
Images of the magnetic field of martian meteorite ALH84001 reveal a spatially heterogeneous pattern of magnetization associated with fractures and rock fragments, indicating that the interior of the rock has not been above this temperature since before its ejection from the surface of Mars.
Early Lunar Magnetism
- I. Garrick‐Bethell, B. Weiss, D. Shuster, J. Buz
- Physics, GeologyScience
- 1 March 2007
It is uncertain whether the Moon ever formed a metallic core or generated a core dynamo. The lunar crust and returned samples are magnetized, but the source of this magnetization could be meteoroid…
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