Below is a list of the most recent file uploads.
See the
gallery of new files for a more visual overview.
19:44, 29 December 2006Amaratalkcontribs uploaded
File:Grapsdustytrail.jpg(Astrophysicists and planetary scientists are especially intrigued by the chondritic IDPs because they provide a link to the astrophysical conditions out of which our solar system formed. We can follow the trail to the right in the diagram above to the ID)
03:50, 22 September 2005Amaratalkcontribs uploaded
File:Porous chondriteIDP.jpg(== Summary == This is a scanning electron micrscope image of a interplanetary dust particle that has roughly
chondritic elemental composition and is highly rough (chondritic porous: "CP"). CP types are usually aggregates of large numbers of)
10:18, 21 September 2005Amaratalkcontribs uploaded
File:IDPmajorelements.jpg(== Summary == The largest data set for major elements (Schramm et al., 1989) comes from the analyses of 200 stratospheric interplanetary dust particles. Brownlee (1997) gives electron microprobe data for 500 cosmic spherules in the 1 micrometer to 1 mili)
10:11, 21 September 2005Amaratalkcontribs uploaded
File:IDPmajorelements.jpg(The largest data set for major elements (Schramm et al., 1989) comes from the analyses of 200 stratospheric interplanetary dust particles. Brownlee (1997) gives electron microprobe data for 500 cosmic spherules in the 1 micrometer to 1 milimeter size ran)
09:21, 21 September 2005Amaratalkcontribs uploaded
File:Smooth chondriteIDP.jpg(== Summary == This is a scanning electron micrscope image of an interplanetary dust particle that has roughly
chondritic elemental composition and is highly smooth (chondritic smooth: "CS"). CS types are usually aggregates of large numbers o)
09:19, 21 September 2005Amaratalkcontribs uploaded
File:Porous chondriteIDP.jpg(== Summary == This is a scanning electron micrscope image of a interplanetary dust particle that has roughly
chondritic elemental composition and is highly rough (chondritic porous: "CP"). CP types are usually aggregates of large numbers of)
19:50, 20 September 2005Amaratalkcontribs uploaded
File:Smooth chondriteIDP.jpg(This is a scanning electron micrscope image of an interplanetary dust particle that has roughly
chondritic elemental composition and is highly smooth (chondritic smooth: "CS"). CS types are usually aggregates of large numbers of sub-micromet)
19:24, 20 September 2005Amaratalkcontribs uploaded
File:Smoothchond.jpg(This is a scanning electron micrscope image of a interplanetary dust particle that has roughly
chondritic elemental composition and is highly smooth (chondritic smooth: "CS"). CS types are usually aggregates of large numbers of sub-micromete)
19:17, 20 September 2005Amaratalkcontribs uploaded
File:Porous chondriteIDP.jpg(This is a scanning electron micrscope image of a interplanetary dust particle that has roughly
chondritic elemental composition and is highly rough (chondritic porous: "CP"). CP types are usually aggregates of large numbers of sub-micrometer)
18:58, 20 September 2005Amaratalkcontribs uploaded
File:Porous chondriteIDP.jpg( [Porous_chondriteIDP.jpg]|porous chondrite]] This is a scanning electron micrscope image of a interplanetary dust particle that has roughly
chondritic elemental composition and is highly rough (chondritic porous: "CP"). CP types are usually)
Below is a list of the most recent file uploads.
See the
gallery of new files for a more visual overview.
19:44, 29 December 2006Amaratalkcontribs uploaded
File:Grapsdustytrail.jpg(Astrophysicists and planetary scientists are especially intrigued by the chondritic IDPs because they provide a link to the astrophysical conditions out of which our solar system formed. We can follow the trail to the right in the diagram above to the ID)
03:50, 22 September 2005Amaratalkcontribs uploaded
File:Porous chondriteIDP.jpg(== Summary == This is a scanning electron micrscope image of a interplanetary dust particle that has roughly
chondritic elemental composition and is highly rough (chondritic porous: "CP"). CP types are usually aggregates of large numbers of)
10:18, 21 September 2005Amaratalkcontribs uploaded
File:IDPmajorelements.jpg(== Summary == The largest data set for major elements (Schramm et al., 1989) comes from the analyses of 200 stratospheric interplanetary dust particles. Brownlee (1997) gives electron microprobe data for 500 cosmic spherules in the 1 micrometer to 1 mili)
10:11, 21 September 2005Amaratalkcontribs uploaded
File:IDPmajorelements.jpg(The largest data set for major elements (Schramm et al., 1989) comes from the analyses of 200 stratospheric interplanetary dust particles. Brownlee (1997) gives electron microprobe data for 500 cosmic spherules in the 1 micrometer to 1 milimeter size ran)
09:21, 21 September 2005Amaratalkcontribs uploaded
File:Smooth chondriteIDP.jpg(== Summary == This is a scanning electron micrscope image of an interplanetary dust particle that has roughly
chondritic elemental composition and is highly smooth (chondritic smooth: "CS"). CS types are usually aggregates of large numbers o)
09:19, 21 September 2005Amaratalkcontribs uploaded
File:Porous chondriteIDP.jpg(== Summary == This is a scanning electron micrscope image of a interplanetary dust particle that has roughly
chondritic elemental composition and is highly rough (chondritic porous: "CP"). CP types are usually aggregates of large numbers of)
19:50, 20 September 2005Amaratalkcontribs uploaded
File:Smooth chondriteIDP.jpg(This is a scanning electron micrscope image of an interplanetary dust particle that has roughly
chondritic elemental composition and is highly smooth (chondritic smooth: "CS"). CS types are usually aggregates of large numbers of sub-micromet)
19:24, 20 September 2005Amaratalkcontribs uploaded
File:Smoothchond.jpg(This is a scanning electron micrscope image of a interplanetary dust particle that has roughly
chondritic elemental composition and is highly smooth (chondritic smooth: "CS"). CS types are usually aggregates of large numbers of sub-micromete)
19:17, 20 September 2005Amaratalkcontribs uploaded
File:Porous chondriteIDP.jpg(This is a scanning electron micrscope image of a interplanetary dust particle that has roughly
chondritic elemental composition and is highly rough (chondritic porous: "CP"). CP types are usually aggregates of large numbers of sub-micrometer)
18:58, 20 September 2005Amaratalkcontribs uploaded
File:Porous chondriteIDP.jpg( [Porous_chondriteIDP.jpg]|porous chondrite]] This is a scanning electron micrscope image of a interplanetary dust particle that has roughly
chondritic elemental composition and is highly rough (chondritic porous: "CP"). CP types are usually)