Andrew Yee
October 1st 04, 01:50 AM
University of California-Davis
Media contact(s):
Qing-Zhu Yin, Geology, (530) 752-0934,
Andy Fell, UC Davis News Service, (530) 752-4533,
September 21, 2004
What Genesis Solar Particles Can Tell Us
The recent crash of NASA's Genesis space probe may have looked like bad news for
scientists, but its cargo of particles captured from the sun should still yield
useful information, according to Qing-Zhu Yin, a planetary scientist at UC Davis.
Yin, who is not directly affiliated with the Genesis mission, studies the
composition of meteorites to learn about the formation of the solar system. Like
the Genesis capsule, meteorites have a hard landing on the Earth, but can still
yield useful information, he said.
By looking at the ratio of oxygen-16, -17 and -18 isotopes in the solar
particles, scientists should be able to test theories about how the sun and
planets formed. Oxygen-16 is by far the most common. The Earth, moon, Mars and
some meteorites all have slightly different ratios of the three isotopes.
The oxygen makeup of the sun, which contains about 99.9 percent of all the mass
in the solar system, is much harder to measure. The Genesis spacecraft was built
to answer that question by collecting particles blown out from the sun.
In a "Perspectives" article in the Sept. 17 issue of the journal Science, Yin
describes new theories about local variations in oxygen isotopes in the vast
dust and gas cloud around the young sun. Free oxygen was released when
ultraviolet light hit carbon monoxide gas. Because oxygen-16 was so abundant, it
was released mostly near the surface of the cloud, but breakdown of carbon
monoxide containing less abundant oxygen-17 or -18 continued deeper into the cloud.
Free oxygen and hydrogen formed water that froze onto dust grains and eventually
formed into planets, preserving the oxygen-17 and -18 signature, Yin said. The
models predict that the Sun itself should have a much lower ratio of oxygen-17
and -18 to oxygen-16 than the rocky planets, a prediction that can be tested by
Genesis and future missions.
Media contact(s):
Qing-Zhu Yin, Geology, (530) 752-0934,
Andy Fell, UC Davis News Service, (530) 752-4533,
September 21, 2004
What Genesis Solar Particles Can Tell Us
The recent crash of NASA's Genesis space probe may have looked like bad news for
scientists, but its cargo of particles captured from the sun should still yield
useful information, according to Qing-Zhu Yin, a planetary scientist at UC Davis.
Yin, who is not directly affiliated with the Genesis mission, studies the
composition of meteorites to learn about the formation of the solar system. Like
the Genesis capsule, meteorites have a hard landing on the Earth, but can still
yield useful information, he said.
By looking at the ratio of oxygen-16, -17 and -18 isotopes in the solar
particles, scientists should be able to test theories about how the sun and
planets formed. Oxygen-16 is by far the most common. The Earth, moon, Mars and
some meteorites all have slightly different ratios of the three isotopes.
The oxygen makeup of the sun, which contains about 99.9 percent of all the mass
in the solar system, is much harder to measure. The Genesis spacecraft was built
to answer that question by collecting particles blown out from the sun.
In a "Perspectives" article in the Sept. 17 issue of the journal Science, Yin
describes new theories about local variations in oxygen isotopes in the vast
dust and gas cloud around the young sun. Free oxygen was released when
ultraviolet light hit carbon monoxide gas. Because oxygen-16 was so abundant, it
was released mostly near the surface of the cloud, but breakdown of carbon
monoxide containing less abundant oxygen-17 or -18 continued deeper into the cloud.
Free oxygen and hydrogen formed water that froze onto dust grains and eventually
formed into planets, preserving the oxygen-17 and -18 signature, Yin said. The
models predict that the Sun itself should have a much lower ratio of oxygen-17
and -18 to oxygen-16 than the rocky planets, a prediction that can be tested by
Genesis and future missions.