| Project/Area Number |
16540444
|
|---|
| Research Category |
Grant-in-Aid for Scientific Research (C)
|
| Allocation Type | Single-year Grants |
|---|
| Section | 一般 |
|---|
| Research Field |
Geochemistry/Astrochemistry
|
|---|
| Research Institution | Graduate School of Science, The University of Tokyo |
|---|
Principal Investigator |
NAGAO Keisuke The University of Tokyo, Graduate School of Science, Professor, 大学院・理学系研究科, 教授 (40131619)
|
|---|
| Co-Investigator(Kenkyū-buntansha) |
SUMINO Hirochika The University of Tokyo, Graduate School of Science, Research Associate, 大学院・理学系研究科, 助手 (90332593)
|
|---|
| Project Period (FY) |
2004 – 2005
|
| Project Status |
Completed (Fiscal Year 2005)
|
| Budget Amount *help |
¥3,700,000 (Direct Cost: ¥3,700,000)
Fiscal Year 2005: ¥1,700,000 (Direct Cost: ¥1,700,000)
Fiscal Year 2004: ¥2,000,000 (Direct Cost: ¥2,000,000)
|
|---|
| Keywords | Noble gas isotope / Martian meteorites / Chassignite / Nakhlite / Shergottite / Ne isotopes of Martian atmosphere / Mass fractionation / Ar-Ar age / 中性子照射 / 宇宙線照射年代 / シャシニ隕石 |
|---|
| Research Abstract |
Noble gas isotopic compositions in atmosphere and interior of the Earth suggest early degassing from interior to form atmosphere. Contrary to this, noble gas distributions of Mars observed from the Viking lander and Martian meteorites are completely different from those in the Earth. To confirm this in detail, we measured many Martian meteorites using high sensitive mass spectrometers and neutron irradiated samples. Some of the results are followings :
1. Enriched Ne in Dhofar 378 shergottite shows ^<20>Ne/^<22>Ne ratio of 7.3±0.1 for Martian atmosphere. The value suggests a severe loss of Martian atmosphere.
2. NWA2737 chassignite shows much higher ^<40>Ar/^<36>Ar and ^<129>Xe/^<132>Xe than those for Chassigny. This means heterogeneous distribution of noble gas isotopes in the interior of Mars. Uniform degassing might not have occurred from the Martian interior.
3. MIL 03346 nakhlite have two phases containing heavily elementally fractionated Martian atmosphere. Weathering products formed on Mars are probable carriers for the fractionated noble gases.
4. One of the end components observed for most shergottites is thought to be a Martian interior noble gas as is observed in Chassigny. Our noble gas data for weathering products of olivine and desert sands strongly indicate that the component is not Martian origin but fractionated Earth atmosphere.
5. Ar-Ar ages for SaU 060 shergottite are 1.0-1.8 Ga at the temperatures of 700-1400℃ and 3-4 Ga at the higher temperatures. The older age might represent the age of Martian crust.
|
