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You searched for subject:(Carbonaceous Meteorites). Showing records 1 – 6 of 6 total matches.

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Columbia University

1. Crapster-Pregont, Ellen J. Constraining the Chemical Environment and Processes in the Protoplanetary Disk: Perspective from Populations of Calcium- and Aluminum-rich Inclusions in Ornans-group and Metal-rich Chondrules in Renazzo-group Carbonaceous Chondrites.

Degree: 2017, Columbia University

Carbonaceous chondrites have an approximately solar bulk composition, with some exceptions (e.g. H), and exhibit a range of parent body alteration. Investigations of both pristine… (more)

Subjects/Keywords: Geochemistry; Solar system; Carbonaceous chondrites (Meteorites)

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APA (6th Edition):

Crapster-Pregont, E. J. (2017). Constraining the Chemical Environment and Processes in the Protoplanetary Disk: Perspective from Populations of Calcium- and Aluminum-rich Inclusions in Ornans-group and Metal-rich Chondrules in Renazzo-group Carbonaceous Chondrites. (Doctoral Dissertation). Columbia University. Retrieved from https://doi.org/10.7916/D8SN0N85

Chicago Manual of Style (16th Edition):

Crapster-Pregont, Ellen J. “Constraining the Chemical Environment and Processes in the Protoplanetary Disk: Perspective from Populations of Calcium- and Aluminum-rich Inclusions in Ornans-group and Metal-rich Chondrules in Renazzo-group Carbonaceous Chondrites.” 2017. Doctoral Dissertation, Columbia University. Accessed March 24, 2019. https://doi.org/10.7916/D8SN0N85.

MLA Handbook (7th Edition):

Crapster-Pregont, Ellen J. “Constraining the Chemical Environment and Processes in the Protoplanetary Disk: Perspective from Populations of Calcium- and Aluminum-rich Inclusions in Ornans-group and Metal-rich Chondrules in Renazzo-group Carbonaceous Chondrites.” 2017. Web. 24 Mar 2019.

Vancouver:

Crapster-Pregont EJ. Constraining the Chemical Environment and Processes in the Protoplanetary Disk: Perspective from Populations of Calcium- and Aluminum-rich Inclusions in Ornans-group and Metal-rich Chondrules in Renazzo-group Carbonaceous Chondrites. [Internet] [Doctoral dissertation]. Columbia University; 2017. [cited 2019 Mar 24]. Available from: https://doi.org/10.7916/D8SN0N85.

Council of Science Editors:

Crapster-Pregont EJ. Constraining the Chemical Environment and Processes in the Protoplanetary Disk: Perspective from Populations of Calcium- and Aluminum-rich Inclusions in Ornans-group and Metal-rich Chondrules in Renazzo-group Carbonaceous Chondrites. [Doctoral Dissertation]. Columbia University; 2017. Available from: https://doi.org/10.7916/D8SN0N85


University of Hawaii – Manoa

2. Jilly, Christine. Timescales and Conditions for the Aqueous Alteration of Chondrites.

Degree: 2017, University of Hawaii – Manoa

Ph.D. University of Hawaii at Manoa 2015.

It has become well-recognized that water played a critical role in the early geological evolution of materials through… (more)

Subjects/Keywords: Meteorites; Carbonaceous Chondrites; Astrobiology; Solar System Formation; Secondary Ion Mass Spectrometry

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APA (6th Edition):

Jilly, C. (2017). Timescales and Conditions for the Aqueous Alteration of Chondrites. (Thesis). University of Hawaii – Manoa. Retrieved from http://hdl.handle.net/10125/51098

Note: this citation may be lacking information needed for this citation format:
Not specified: Masters Thesis or Doctoral Dissertation

Chicago Manual of Style (16th Edition):

Jilly, Christine. “Timescales and Conditions for the Aqueous Alteration of Chondrites.” 2017. Thesis, University of Hawaii – Manoa. Accessed March 24, 2019. http://hdl.handle.net/10125/51098.

Note: this citation may be lacking information needed for this citation format:
Not specified: Masters Thesis or Doctoral Dissertation

MLA Handbook (7th Edition):

Jilly, Christine. “Timescales and Conditions for the Aqueous Alteration of Chondrites.” 2017. Web. 24 Mar 2019.

Vancouver:

Jilly C. Timescales and Conditions for the Aqueous Alteration of Chondrites. [Internet] [Thesis]. University of Hawaii – Manoa; 2017. [cited 2019 Mar 24]. Available from: http://hdl.handle.net/10125/51098.

Note: this citation may be lacking information needed for this citation format:
Not specified: Masters Thesis or Doctoral Dissertation

Council of Science Editors:

Jilly C. Timescales and Conditions for the Aqueous Alteration of Chondrites. [Thesis]. University of Hawaii – Manoa; 2017. Available from: http://hdl.handle.net/10125/51098

Note: this citation may be lacking information needed for this citation format:
Not specified: Masters Thesis or Doctoral Dissertation


University of Arizona

3. Palmer, Eric Edward. Volatiles on Solar System Objects: Carbon Dioxide on Iapetus and Aqueous Alteration in CM Chondrites .

Degree: 2009, University of Arizona

 Volatiles are critical in understanding the history of the solar system. We conducted two case studies intended to further this understanding. First, we analyzed the… (more)

Subjects/Keywords: Carbon Dioxide; Carbonaceous Chondrites; Iapetus; Ice; Meteorites; Photochemistry

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APA (6th Edition):

Palmer, E. E. (2009). Volatiles on Solar System Objects: Carbon Dioxide on Iapetus and Aqueous Alteration in CM Chondrites . (Doctoral Dissertation). University of Arizona. Retrieved from http://hdl.handle.net/10150/194263

Chicago Manual of Style (16th Edition):

Palmer, Eric Edward. “Volatiles on Solar System Objects: Carbon Dioxide on Iapetus and Aqueous Alteration in CM Chondrites .” 2009. Doctoral Dissertation, University of Arizona. Accessed March 24, 2019. http://hdl.handle.net/10150/194263.

MLA Handbook (7th Edition):

Palmer, Eric Edward. “Volatiles on Solar System Objects: Carbon Dioxide on Iapetus and Aqueous Alteration in CM Chondrites .” 2009. Web. 24 Mar 2019.

Vancouver:

Palmer EE. Volatiles on Solar System Objects: Carbon Dioxide on Iapetus and Aqueous Alteration in CM Chondrites . [Internet] [Doctoral dissertation]. University of Arizona; 2009. [cited 2019 Mar 24]. Available from: http://hdl.handle.net/10150/194263.

Council of Science Editors:

Palmer EE. Volatiles on Solar System Objects: Carbon Dioxide on Iapetus and Aqueous Alteration in CM Chondrites . [Doctoral Dissertation]. University of Arizona; 2009. Available from: http://hdl.handle.net/10150/194263

4. Biron, Katarzyna. The Molecular structure of the Insoluble Organic Matter (MOI) deposited from organic plasma : Comparison with IOM isolated from carbonaceous meteorites : Structure moléculaire de la matière organique insoluble (MOI) déposé à partir d'un plasma organique : Comparaison avec le MOI isolé de météorites carbonées.

Degree: Docteur es, Histoire de la Terre, 2016, Paris, Muséum national d'histoire naturelle

Les météorites carbonées sont les objets les plus primitifs du système solaire. Ils contiennent jusqu'à 4 % de carbone, principalement présent sous forme de matière… (more)

Subjects/Keywords: Météorites; Matière organique insoluble; Heteroatomes; Carbonaceous Meteorites; Insoluble organic matter; Heteroatoms; 523.5

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APA (6th Edition):

Biron, K. (2016). The Molecular structure of the Insoluble Organic Matter (MOI) deposited from organic plasma : Comparison with IOM isolated from carbonaceous meteorites : Structure moléculaire de la matière organique insoluble (MOI) déposé à partir d'un plasma organique : Comparaison avec le MOI isolé de météorites carbonées. (Doctoral Dissertation). Paris, Muséum national d'histoire naturelle. Retrieved from http://www.theses.fr/2016MNHN0004

Chicago Manual of Style (16th Edition):

Biron, Katarzyna. “The Molecular structure of the Insoluble Organic Matter (MOI) deposited from organic plasma : Comparison with IOM isolated from carbonaceous meteorites : Structure moléculaire de la matière organique insoluble (MOI) déposé à partir d'un plasma organique : Comparaison avec le MOI isolé de météorites carbonées.” 2016. Doctoral Dissertation, Paris, Muséum national d'histoire naturelle. Accessed March 24, 2019. http://www.theses.fr/2016MNHN0004.

MLA Handbook (7th Edition):

Biron, Katarzyna. “The Molecular structure of the Insoluble Organic Matter (MOI) deposited from organic plasma : Comparison with IOM isolated from carbonaceous meteorites : Structure moléculaire de la matière organique insoluble (MOI) déposé à partir d'un plasma organique : Comparaison avec le MOI isolé de météorites carbonées.” 2016. Web. 24 Mar 2019.

Vancouver:

Biron K. The Molecular structure of the Insoluble Organic Matter (MOI) deposited from organic plasma : Comparison with IOM isolated from carbonaceous meteorites : Structure moléculaire de la matière organique insoluble (MOI) déposé à partir d'un plasma organique : Comparaison avec le MOI isolé de météorites carbonées. [Internet] [Doctoral dissertation]. Paris, Muséum national d'histoire naturelle; 2016. [cited 2019 Mar 24]. Available from: http://www.theses.fr/2016MNHN0004.

Council of Science Editors:

Biron K. The Molecular structure of the Insoluble Organic Matter (MOI) deposited from organic plasma : Comparison with IOM isolated from carbonaceous meteorites : Structure moléculaire de la matière organique insoluble (MOI) déposé à partir d'un plasma organique : Comparaison avec le MOI isolé de météorites carbonées. [Doctoral Dissertation]. Paris, Muséum national d'histoire naturelle; 2016. Available from: http://www.theses.fr/2016MNHN0004

5. Yesiltas, Mehmet. Synchrotron Based Infrared Microspectroscopy of Carbonaceous Chondrites.

Degree: 2015, University of Central Florida

 Relationships between organic molecules and inorganic minerals are investigated in five carbonaceous chondrites, Northwest Africa 852 (CR2), Tagish Lake (C2-ungroupped), Orgueil (CI1), Sutter's Mill (CM),… (more)

Subjects/Keywords: Infrared; raman; spectroscopy; microscopy; meteorites; carbonaceous chondrites; Physics; Dissertations, Academic  – Sciences; Sciences  – Dissertations, Academic

…72 Table 10. The CH2/CH3 ratios of SM meteorites and various astronomical objects… …86 xiii CHAPTER ONE: GENERAL INTRODUCTION 1.1 Meteorites Meteorites are… …small fraction comes from comets, Mars, and the Moon. Carbonaceous chondrites are the most… …primitive meteorites and are probably fragments of either primitive asteroids or comets [1… …Some carbonaceous chondrites are aqueously altered to a greater or lesser extent (… 

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APA (6th Edition):

Yesiltas, M. (2015). Synchrotron Based Infrared Microspectroscopy of Carbonaceous Chondrites. (Doctoral Dissertation). University of Central Florida. Retrieved from http://stars.library.ucf.edu/etd/1497

Chicago Manual of Style (16th Edition):

Yesiltas, Mehmet. “Synchrotron Based Infrared Microspectroscopy of Carbonaceous Chondrites.” 2015. Doctoral Dissertation, University of Central Florida. Accessed March 24, 2019. http://stars.library.ucf.edu/etd/1497.

MLA Handbook (7th Edition):

Yesiltas, Mehmet. “Synchrotron Based Infrared Microspectroscopy of Carbonaceous Chondrites.” 2015. Web. 24 Mar 2019.

Vancouver:

Yesiltas M. Synchrotron Based Infrared Microspectroscopy of Carbonaceous Chondrites. [Internet] [Doctoral dissertation]. University of Central Florida; 2015. [cited 2019 Mar 24]. Available from: http://stars.library.ucf.edu/etd/1497.

Council of Science Editors:

Yesiltas M. Synchrotron Based Infrared Microspectroscopy of Carbonaceous Chondrites. [Doctoral Dissertation]. University of Central Florida; 2015. Available from: http://stars.library.ucf.edu/etd/1497

6. Zeszut, Zoe. Measurement of Adhesion Forces in CM2 Meteorite Materials.

Degree: MSs, Geological Sciences, 2017, Case Western Reserve University

 With many current and upcoming space missions exploring C-type asteroids, there is a need for understanding the physical properties of asteroid surface material. Adhesion forces… (more)

Subjects/Keywords: Geology; Geological; Mineralogy; geology; geological sciences; planetary sciences; asteroid; asteroids; meteorite; meteorites; cm2; carbonaceous asteroid; c type asteroid; adhesion; cohesion; force; NASA; YORP; measurements; analog; analogue; regolith; mineral; serpentine; mineralogy

…first measurements of adhesion in asteroid-derived materials (CM2 meteorites). Five… …carbonaceous. Other major types include S, stony, and M, metallic (Weisberg et al., 2006)… …shown that compositions of meteorites and asteroids are strongly related; therefore meteorites… …are indicated to be the parent bodies of CM meteorites. Like C asteroids, CM meteorites are… …dark in color and are rich in phyllosilicates. Mineralogical linkages between CM carbonaceous… 

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APA (6th Edition):

Zeszut, Z. (2017). Measurement of Adhesion Forces in CM2 Meteorite Materials. (Masters Thesis). Case Western Reserve University. Retrieved from http://rave.ohiolink.edu/etdc/view?acc_num=case1499341914992823

Chicago Manual of Style (16th Edition):

Zeszut, Zoe. “Measurement of Adhesion Forces in CM2 Meteorite Materials.” 2017. Masters Thesis, Case Western Reserve University. Accessed March 24, 2019. http://rave.ohiolink.edu/etdc/view?acc_num=case1499341914992823.

MLA Handbook (7th Edition):

Zeszut, Zoe. “Measurement of Adhesion Forces in CM2 Meteorite Materials.” 2017. Web. 24 Mar 2019.

Vancouver:

Zeszut Z. Measurement of Adhesion Forces in CM2 Meteorite Materials. [Internet] [Masters thesis]. Case Western Reserve University; 2017. [cited 2019 Mar 24]. Available from: http://rave.ohiolink.edu/etdc/view?acc_num=case1499341914992823.

Council of Science Editors:

Zeszut Z. Measurement of Adhesion Forces in CM2 Meteorite Materials. [Masters Thesis]. Case Western Reserve University; 2017. Available from: http://rave.ohiolink.edu/etdc/view?acc_num=case1499341914992823

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