Stephanie C. Werner

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Stephanie C. Werner (born 1974) [1] is a German geologist and planetologist, known for her work on Mars and the Arctic. She is a professor in the Centre for Earth Evolution and Dynamics of the University of Oslo in Norway.

Contents

Her research has included the discovery that many meteorites of Martian origin come from the Mojave impact crater on Mars, [2] and an estimate that an era of planetary migration in the solar system occurred earlier than previously thought. [3]

Education and career

Werner earned a diploma in geophysics in 1999 from the University of Kiel, and completed a doctorate (Dr. rer. nat.) in 2005 at the Free University of Berlin; her dissertation was Major Aspects of the Chronostratigraphy and Geologic Evolutionary History of Mars. [4]

After postdoctoral research at the Free University Berlin and the Geological Survey of Norway, she became a researcher at the University of Oslo in 2009. In 2014 she became an associate professor there, and in 2017 a full professor. [4]

Recognition

In 2019, Werner was elected to the Norwegian Academy of Science and Letters. [5]

Asteroid 11449 Stephwerner is named for her. [6]

Related Research Articles

<span class="mw-page-title-main">Meteorite</span> Solid debris from outer space that hits a planetary surface

A meteorite is a solid piece of debris from an object, such as a comet, asteroid, or meteoroid, that originates in outer space and survives its passage through the atmosphere to reach the surface of a planet or moon. When the original object enters the atmosphere, various factors such as friction, pressure, and chemical interactions with the atmospheric gases cause it to heat up and radiate energy. It then becomes a meteor and forms a fireball, also known as a shooting star; astronomers call the brightest examples "bolides". Once it settles on the larger body's surface, the meteor becomes a meteorite. Meteorites vary greatly in size. For geologists, a bolide is a meteorite large enough to create an impact crater.

<span class="mw-page-title-main">Meteor Crater</span> Meteorite impact crater in northern Arizona

Meteor Crater, or Barringer Crater, is a meteorite impact crater about 37 mi (60 km) east of Flagstaff and 18 mi (29 km) west of Winslow in the desert of northern Arizona, United States. The site had several earlier names, and fragments of the meteorite are officially called the Canyon Diablo Meteorite, after the adjacent Cañon Diablo. Because the United States Board on Geographic Names recognizes names of natural features derived from the nearest post office, the feature acquired the name of "Meteor Crater" from the nearby post office named Meteor.

<span class="mw-page-title-main">Impact event</span> Collision of two astronomical objects with measurable effects

An impact event is a collision between astronomical objects causing measurable effects. Impact events have physical consequences and have been found to regularly occur in planetary systems, though the most frequent involve asteroids, comets or meteoroids and have minimal effect. When large objects impact terrestrial planets such as the Earth, there can be significant physical and biospheric consequences, though atmospheres mitigate many surface impacts through atmospheric entry. Impact craters and structures are dominant landforms on many of the Solar System's solid objects and present the strongest empirical evidence for their frequency and scale.

<span class="mw-page-title-main">Martian meteorite</span> Meteorite made of rock originating from Mars

A Martian meteorite is a rock that formed on Mars, was ejected from the planet by an impact event, and traversed interplanetary space before landing on Earth as a meteorite. As of September 2020, 277 meteorites had been classified as Martian, less than half a percent of the 72,000 meteorites that have been classified. The largest complete, uncut Martian meteorite, Taoudenni 002, was recovered in Mali in early 2021. It weighs 14.5 kilograms and is on display at the Maine Mineral & Gem Museum.

<span class="mw-page-title-main">Ejecta blanket</span> Symmetrical apron of ejecta that surrounds an impact crater

An ejecta blanket is a generally symmetrical apron of ejecta that surrounds an impact crater; it is layered thickly at the crater's rim and thin to discontinuous at the blanket's outer edge. The impact cratering is one of the basic surface formation mechanisms of the solar system bodies and the formation and emplacement of ejecta blankets are the fundamental characteristics associated with impact cratering event. The ejecta materials are considered as the transported materials beyond the transient cavity formed during impact cratering regardless of the state of the target materials.

Susan Elizabeth Werner Kieffer is an American physical geologist and planetary scientist. Kieffer is known for her work on the fluid dynamics of volcanoes, geysers, and rivers, and for her model of the thermodynamic properties of complex minerals. She has also contributed to the scientific understanding of meteorite impacts.

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References

  1. Birth year from German National Library catalog entry, retrieved 2020-03-20
  2. Bennington-Castro, Joseph (6 March 2014), "Meteorites on Earth May Be From Ancient Crater on Mars, Study Says", National Geographic
  3. Strain, Daniel (12 August 2019), "A new timeline of Earth's cataclysmic past", CU Boulder Today, University of Colorado Boulder
  4. 1 2 Stephanie Werner, University of Oslo Department of Geosciences, retrieved 2020-03-20
  5. Academy Members, Norwegian Academy of Science and Letters , retrieved 2020-03-20
  6. "11449 Stephwerner (1979 QP)", JPL Small-Body Database, Jet Propulsion Laboratory, retrieved 2020-03-20