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    <lastmod>2024-05-26</lastmod>
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      <image:title>Home - THE JACK HILLS</image:title>
      <image:caption>View of the granitoid rocks in the Yilgarn craton, looking southwest from the summit of Mount Hale, Jack Hills, Western Australia.</image:caption>
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      <image:loc>https://images.squarespace-cdn.com/content/v1/56d74e9c4c2f85996d16a562/1462633248662-D0AYB4X048PSAQQN2P23/JH_zirc_NRM_SM4.png</image:loc>
      <image:title>Home - JACK HILLS ZIRCON MAGNETISM</image:title>
      <image:caption>Map of the vertical component of the magnetic field of the natural remanent magnetization field 0.2 mm above Jack Hills zircons (circled) using the SQUID Microscope at MIT. The zircons have moments ranging from just 6.8e-14 to 4.4e-12 Am2.</image:caption>
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      <image:title>Home - SECONDARY MAGNETIC MINERALS IN JACK HILLS ZIRCONS</image:title>
      <image:caption>Left: magnetic field above two zircons from quantum diamond microscopy. Middle: textural and compositional map of zircons using backscattered scanning electron microscopy. Right: Map of iron abundance using wavelength-dispersive spectroscopy.</image:caption>
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      <image:title>Home - QDM MAP OF JACK HILLS ZIRCONS (CLICK IMAGE FOR DETAILS)</image:title>
      <image:caption>(Left) Map of the vertical component of the magnetic fields of Jack Hills zircons. Magnetic field map taken at a sensor-to-sample distance of ~1-10 μm. Negative (positive) values correspond to into-the-page (out-of-the-page field) directions. (Right) Zoom of maps of 12 zircons in box at left</image:caption>
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      <image:title>Home - SQUID MICROSCOPY MAP of 1$ BILL (CLICK IMAGE FOR DETAILS)</image:title>
      <image:caption>Map of the vertical component of the magnetic field of George on the United States one dollar bill using the SQUID microscope.   (Bottom Left) Photograph of mapped region.  (Bottom Center) Magnetic field map taken at a sensor-to-sample distance of ~200 μm. Negative (positive) values correspond to into-the-page (out-of-the-page field) directions.  Zooms of two boxed regions shown in Top Center and Bottom Right panels.  (Top Center) Detail of magnetic field map around George's eye.  (Bottom Right) Detail of magnetic field map around George's cheek.</image:caption>
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      <image:title>Home - MTJ MICROSCOPY MAP OF BASALT (CLICK IMAGE FOR DETAILS)</image:title>
      <image:caption>Thin section of a basaltic rock measured both with the MIT SQUID microscope and with the MTJ microscope. (Left) Crossed-polars transmitted-light microscopy image of the mapped region. Dark regions correspond to the groundmass, which is magnetic, whereas colored features are the nonmagnetic olivine phenocrysts. (Middle) Map of the vertical component of the magnetic field measured with the MIT scanning SQUID microscope at a sensor-to-sample distance of ~190 μm. (Right) Map of the vertical component of the magnetic field measured with the MTJ sensor touching the sample (sensor-to-sample distance of ~7 μm) in the same target area of the thin section.</image:caption>
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      <image:caption>Photograph of asteroid (21) Lutetia by the Optical, Spectroscopic, and Infrared Remote Imaging System (OSIRIS) camera on Rosetta.</image:caption>
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      <image:title>Home - COMET 67P/CHURYUMOV-GERASIMENKO (CLICK ON IMAGE FOR DETAILS)</image:title>
      <image:caption>Photograph of comet 67P/Churyumov-Gerasimenko by the Optical, Spectroscopic, and Infrared Remote Imaging System (OSIRIS) camera on Rosetta.</image:caption>
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      <image:title>Home - NEBULAR MAGNETIC FIELDS</image:title>
      <image:caption>Our paleomagnetic studies of chondrules from the Semarkona meteorite provided the first measurements of the intensity of nebular magnetic fields in the terrestrial-planet forming region of the early solar system.</image:caption>
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      <image:loc>https://images.squarespace-cdn.com/content/v1/56d74e9c4c2f85996d16a562/1459719026285-VB3HH8X27CQQK4ZX7BFO/dust-olivine3.png</image:loc>
      <image:title>Home - DUSTY OLIVINE CHONDRULE</image:title>
      <image:caption>The Semarkona meteorite contains chondrules with dusty olivine crystals. This transmission electron microscopy image shows how the olivine (dark grey) hosts fine pure iron metal grains (white) with excellent magnetic recording properties.  These metal grains are formed by reduction of an iron-bearing olivine precursor, which also produces excess silica (black phase at tips of metal grains)</image:caption>
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      <image:title>Home - LIFETIME OF THE SOLAR NEBULA</image:title>
      <image:caption>We found that volcanic angrites are not magnetized, indicating that the solar nebular field and gas likely had dissipated by just 3.8 million years after the formation of the oldest known solids.</image:caption>
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    <loc>http://www.benweiss.mit.edu/publications</loc>
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    <lastmod>2026-02-23</lastmod>
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    <loc>http://www.benweiss.mit.edu/about</loc>
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    <lastmod>2026-02-23</lastmod>
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    <loc>http://www.benweiss.mit.edu/opportunities</loc>
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    <lastmod>2019-02-26</lastmod>
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      <image:title>Opportunities</image:title>
      <image:caption>Former Harvard Ph.D. student Karin Louzada drilling basalts at Lonar crater, India.</image:caption>
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  <url>
    <loc>http://www.benweiss.mit.edu/psyche-magnetometer-research-scientist</loc>
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    <lastmod>2017-06-11</lastmod>
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      <image:loc>https://images.squarespace-cdn.com/content/v1/56d74e9c4c2f85996d16a562/1497210802287-JMQOSDLC0G93A7JIEFDG/PSYCHE_WIDESHOT_FINAL_ultra-low.png</image:loc>
      <image:title>Research Scientist, Psyche Magnetometer Investigation</image:title>
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    <loc>http://www.benweiss.mit.edu/50th-birthday</loc>
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    <lastmod>2023-03-07</lastmod>
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