adsabs/AstroCLIMB huggingface dataset:
Paper: Organic Hazes as a Source of Life’s Building Blocks to Warm Little Ponds on the Hadean Earth
Authors: Ben K. D. Pearce, Sarah M. Hörst, Joshua A. Sebree, Chao He
Figure caption: GC/MS/MS mass spectra for gate 10 GC peaks integrated over retention time ∼11.66–11.77 minutes, for each of our four haze particle samples.
Paper: Organic Hazes as a Source of Life’s Building Blocks to Warm Little Ponds on the Hadean Earth
Authors: Ben K. D. Pearce, Sarah M. Hörst, Joshua A. Sebree, Chao He
Figure caption: GC/MS/MS chromatogram standards for seven nucleobases at nine different sample concentrations/injection volumes (i.e., injection masses). The standards were created in our lab from individual nucleobases purchased from Sigma Aldrich.
Paper: Organic Hazes as a Source of Life’s Building Blocks to Warm Little Ponds on the Hadean Earth
Authors: Ben K. D. Pearce, Sarah M. Hörst, Joshua A. Sebree, Chao He
Figure caption: GC/MS/MS chromatogram standards for 22 physiological amino acids and other biomolecules at nine different sample concentrations/injection volumes (i.e., injection masses). The complete standard was purchased from Sigma Aldrich.
Paper: Organic Hazes as a Source of Life’s Building Blocks to Warm Little Ponds on the Hadean Earth
Authors: Ben K. D. Pearce, Sarah M. Hörst, Joshua A. Sebree, Chao He
Figure caption: Calibration curves calculated for 22 amino acids and other organics. Equations of the lines of best fit and χ 2 values are added to the legend. Uncertainties are the shaded regions calculated as the variance from a model linearly connecting each data point. Peak areas for the 5% CH4 haze particles are added to the plots to demonstrate our quantification calculations.
Paper: Organic Hazes as a Source of Life’s Building Blocks to Warm Little Ponds on the Hadean Earth
Authors: Ben K. D. Pearce, Sarah M. Hörst, Joshua A. Sebree, Chao He
Figure caption: A screenshot of the interactive Python code that we developed to find peaks, calculate peak areas, and estimate peak area uncertainty. Noise regions within each gate are manually selected and used to calculate S/N. This peak represents the cytosine detection in our high-methane experimental haze sample.
Paper: Organic Hazes as a Source of Life’s Building Blocks to Warm Little Ponds on the Hadean Earth
Authors: Ben K. D. Pearce, Sarah M. Hörst, Joshua A. Sebree, Chao He
Figure caption: GC/MS/MS chromatogram standard for hypoxanthine, followed by 17 GC/MS/MS runs of a procedural blank containing an MTBSTFA derivatizer. Only four of the wash runs are displayed for clarity.
Paper: Organic Hazes as a Source of Life’s Building Blocks to Warm Little Ponds on the Hadean Earth
Authors: Ben K. D. Pearce, Sarah M. Hörst, Joshua A. Sebree, Chao He
Figure caption: Calibration curves calculated for 22 amino acids and other organics. Equations of the lines of best fit and χ 2 values are added to the legend. Uncertainties are the shaded regions calculated as the variance from a model linearly connecting each data point. Peak areas for the 0.5% CH4 haze particles are added to the plots to demonstrate our quantification calculations.
Paper: An Updated Shape Model of Dimorphos from DART Data
Authors: R. Terik Daly, Carolyn M. Ernst, Olivier S. Barnouin, Robert W. Gaskell, Hari Nair, Harrison Agrusa, Nancy L. Chabot, Andrew F. Cheng, Elisabetta Dotto, Elena Mazzotta Epifani, Raymond C. Espiritu, Tony L. Farnham, Eric E. Palmer, Petr Pravec, Andrew S. Rivkin, Dany C. Waller, Angelo Zinzi
Figure caption: Examples of shape modeling tests with large errors in the B-axis (i.e., the axis into and out of the page). The left column shows a simulated image used to build the model, the middle column shows the starting ellipsoid, and the right column shows the SPC model made from the simulated images. Each row shows a different shape modeling test. See Daly et al. (2022) for details on the shape modeling tests done for DART. Blue arrows show the location of the terminator in the simulated images. The arrows are in the same positions relative to the image in all three columns. Offsets between the points of the arrows and the terminator in the SPC model indicate errors in the model.
Paper: An Updated Shape Model of Dimorphos from DART Data
Authors: R. Terik Daly, Carolyn M. Ernst, Olivier S. Barnouin, Robert W. Gaskell, Hari Nair, Harrison Agrusa, Nancy L. Chabot, Andrew F. Cheng, Elisabetta Dotto, Elena Mazzotta Epifani, Raymond C. Espiritu, Tony L. Farnham, Eric E. Palmer, Petr Pravec, Andrew S. Rivkin, Dany C. Waller, Angelo Zinzi
Figure caption: Keypoint assessments. Colored lines in (a) and (b) connect features matched by the algorithm in the image and on the shape model. Panel (c) shows a metric based on differences between corresponding keypoints across many DRACO images. Panel (d) shows a model-to-image scale factor derived by comparing the distances measured between all keypoints in the reference DRACO image to the distances measured between all keypoints in the rendered shape model. The arrow in (b) indicates the direction of Dimorphos north (+Z).
Paper: Depth-to-diameter Ratios of Fresh Craters on the Moon and Implications for Surface Age Estimates
Authors: Rachael H. Hoover, Stuart J. Robbins, Brian M. Hynek, Paul O. Hayne
Figure caption: The d/D of craters measured in this study (red squares for mare craters and red circle for the highlands crater) compared to ranges estimated or measured by previous workers (black circles and pink diamonds). Pink diamonds indicate measurements made from shadows of new crater detections in previous work. Error bars shown are calculated using the standard deviation and the number of points used in the elevation measurements, which is discussed in Section 3.4. Averages from our data (red lines) and past work (black lines) are overlaid. The average d/D for craters <100 m is similar between this study and previous studies, but the average differs for craters >100 m.
Paper: Depth-to-diameter Ratios of Fresh Craters on the Moon and Implications for Surface Age Estimates
Authors: Rachael H. Hoover, Stuart J. Robbins, Brian M. Hynek, Paul O. Hayne
Figure caption: The 10 craters used in our study. The left image in each panel is one of the NAC orthoimages used in the creation of the DTM, and the right image is the DTM overlying the NAC image. Beneath the pair is a single topographic profile. Panels (a)–(d) are new crater impacts observed by LROC, and panels (e)–(j) are cold spot craters observed by DIVINER.
Paper: Achievement of the Planetary Defense Investigations of the Double Asteroid Redirection Test (DART) Mission
Authors: Nancy L. Chabot, Andrew S. Rivkin, Andrew F. Cheng, Olivier S. Barnouin, Eugene G. Fahnestock, Derek C. Richardson, Angela M. Stickle, Cristina A. Thomas, Carolyn M. Ernst, R. Terik Daly, Elisabetta Dotto, Angelo Zinzi, Steven R. Chesley, Nicholas A. Moskovitz, Brent W. Barbee, Paul Abell, Harrison F. Agrusa, Michele T. Bannister, Joel Beccarelli, Dmitriy L. Bekker, Megan Bruck Syal, Bonnie J. Buratti, Michael W. Busch, Adriano Campo Bagatin, Joseph P. Chatelain, Sidney Chocron, Gareth S. Collins, Luca Conversi, Thomas M. Davison, Mallory E. DeCoster, J. D. Prasanna Deshapriya, Siegfried Eggl, Raymond C. Espiritu, Tony L. Farnham, Marin Ferrais, Fabio Ferrari, Dora Föhring, Oscar Fuentes-Muñoz, Igor Gai, Carmine Giordano, David A. Glenar, Edward Gomez, Dawn M. Graninger, Simon F. Green, Sarah Greenstreet, Pedro H. Hasselmann, Isabel Herreros, Masatoshi Hirabayashi, Marek Husárik, Simone Ieva, Stavro L. Ivanovski, Samuel L. Jackson, Emmanuel Jehin, Martin Jutzi, Ozgur Karatekin, Matthew M. Knight, Ludmilla Kolokolova, Kathryn M. Kumamoto, Michael Küppers, Fiorangela La Forgia, Monica Lazzarin, Jian-Yang Li, Tim A. Lister, Ramin Lolachi, Michael P. Lucas, Alice Lucchetti, Robert Luther, Rahil Makadia, Elena Mazzotta Epifani, Jay McMahon, Gianmario Merisio, Colby C. Merrill, Alex J. Meyer, Patrick Michel, Marco Micheli, Alessandra Migliorini, Kate Minker, Dario Modenini, Fernando Moreno, Naomi Murdoch, Brian Murphy, Shantanu P. Naidu, Hari Nair, Ryota Nakano, Cyrielle Opitom, Jens Ormö, J. Michael Owen, Maurizio Pajola, Eric E. Palmer, Pasquale Palumbo, Paolo Panicucci, Laura M. Parro, Jason M. Pearl, Antti Penttilä, Davide Perna, Elisabeta Petrescu, Petr Pravec, Sabina D. Raducan, K. T. Ramesh, Ryan Ridden-Harper, Juan L. Rizos, Alessandro Rossi, Nathan X. Roth, Agata Rożek, Benjamin Rozitis, Eileen V. Ryan, William H. Ryan, Paul Sánchez, Toni Santana-Ros, Daniel J. Scheeres, Peter Scheirich, Cem Berk Senel, Colin Snodgrass, Stefania Soldini, Damya Souami, Thomas S. Statler, Rachel Street, Timothy J. Stubbs, Jessica M. Sunshine, Nicole J. Tan, Gonzalo Tancredi, Calley L. Tinsman, Paolo Tortora, Filippo Tusberti, James D. Walker, C. Dany Waller, Kai Wünnemann, Marco Zannoni, Yun Zhang
Figure caption: LICIACube image acquired 143 s following DART's kinetic impact, showing a complex system of ejecta rays. Each rectangle represents a different level of contrast in order to better see the fine structure in the ejecta. The innermost rectangle is roughly 1.3 km wide. (LICIACube LUKE image triplet acquired at 23:16:47 UTC; credit: ASI/NASA/APL.)
Paper: Achievement of the Planetary Defense Investigations of the Double Asteroid Redirection Test (DART) Mission
Authors: Nancy L. Chabot, Andrew S. Rivkin, Andrew F. Cheng, Olivier S. Barnouin, Eugene G. Fahnestock, Derek C. Richardson, Angela M. Stickle, Cristina A. Thomas, Carolyn M. Ernst, R. Terik Daly, Elisabetta Dotto, Angelo Zinzi, Steven R. Chesley, Nicholas A. Moskovitz, Brent W. Barbee, Paul Abell, Harrison F. Agrusa, Michele T. Bannister, Joel Beccarelli, Dmitriy L. Bekker, Megan Bruck Syal, Bonnie J. Buratti, Michael W. Busch, Adriano Campo Bagatin, Joseph P. Chatelain, Sidney Chocron, Gareth S. Collins, Luca Conversi, Thomas M. Davison, Mallory E. DeCoster, J. D. Prasanna Deshapriya, Siegfried Eggl, Raymond C. Espiritu, Tony L. Farnham, Marin Ferrais, Fabio Ferrari, Dora Föhring, Oscar Fuentes-Muñoz, Igor Gai, Carmine Giordano, David A. Glenar, Edward Gomez, Dawn M. Graninger, Simon F. Green, Sarah Greenstreet, Pedro H. Hasselmann, Isabel Herreros, Masatoshi Hirabayashi, Marek Husárik, Simone Ieva, Stavro L. Ivanovski, Samuel L. Jackson, Emmanuel Jehin, Martin Jutzi, Ozgur Karatekin, Matthew M. Knight, Ludmilla Kolokolova, Kathryn M. Kumamoto, Michael Küppers, Fiorangela La Forgia, Monica Lazzarin, Jian-Yang Li, Tim A. Lister, Ramin Lolachi, Michael P. Lucas, Alice Lucchetti, Robert Luther, Rahil Makadia, Elena Mazzotta Epifani, Jay McMahon, Gianmario Merisio, Colby C. Merrill, Alex J. Meyer, Patrick Michel, Marco Micheli, Alessandra Migliorini, Kate Minker, Dario Modenini, Fernando Moreno, Naomi Murdoch, Brian Murphy, Shantanu P. Naidu, Hari Nair, Ryota Nakano, Cyrielle Opitom, Jens Ormö, J. Michael Owen, Maurizio Pajola, Eric E. Palmer, Pasquale Palumbo, Paolo Panicucci, Laura M. Parro, Jason M. Pearl, Antti Penttilä, Davide Perna, Elisabeta Petrescu, Petr Pravec, Sabina D. Raducan, K. T. Ramesh, Ryan Ridden-Harper, Juan L. Rizos, Alessandro Rossi, Nathan X. Roth, Agata Rożek, Benjamin Rozitis, Eileen V. Ryan, William H. Ryan, Paul Sánchez, Toni Santana-Ros, Daniel J. Scheeres, Peter Scheirich, Cem Berk Senel, Colin Snodgrass, Stefania Soldini, Damya Souami, Thomas S. Statler, Rachel Street, Timothy J. Stubbs, Jessica M. Sunshine, Nicole J. Tan, Gonzalo Tancredi, Calley L. Tinsman, Paolo Tortora, Filippo Tusberti, James D. Walker, C. Dany Waller, Kai Wünnemann, Marco Zannoni, Yun Zhang
Figure caption: A mosaic of DRACO images showing Dimorphos (left, extent in Z-direction, 115 m) and Didymos (right, extent in Z-direction, 607 m) oriented with their north poles toward the top of the image and with each asteroid and their distance to each other to scale. Dimorphos is a scaled down version of Figure 7. The image of Didymos is a composition of 58 DRACO images assembled by layering the higher-resolution images on top of the lower-resolution ones.
Paper: Achievement of the Planetary Defense Investigations of the Double Asteroid Redirection Test (DART) Mission
Authors: Nancy L. Chabot, Andrew S. Rivkin, Andrew F. Cheng, Olivier S. Barnouin, Eugene G. Fahnestock, Derek C. Richardson, Angela M. Stickle, Cristina A. Thomas, Carolyn M. Ernst, R. Terik Daly, Elisabetta Dotto, Angelo Zinzi, Steven R. Chesley, Nicholas A. Moskovitz, Brent W. Barbee, Paul Abell, Harrison F. Agrusa, Michele T. Bannister, Joel Beccarelli, Dmitriy L. Bekker, Megan Bruck Syal, Bonnie J. Buratti, Michael W. Busch, Adriano Campo Bagatin, Joseph P. Chatelain, Sidney Chocron, Gareth S. Collins, Luca Conversi, Thomas M. Davison, Mallory E. DeCoster, J. D. Prasanna Deshapriya, Siegfried Eggl, Raymond C. Espiritu, Tony L. Farnham, Marin Ferrais, Fabio Ferrari, Dora Föhring, Oscar Fuentes-Muñoz, Igor Gai, Carmine Giordano, David A. Glenar, Edward Gomez, Dawn M. Graninger, Simon F. Green, Sarah Greenstreet, Pedro H. Hasselmann, Isabel Herreros, Masatoshi Hirabayashi, Marek Husárik, Simone Ieva, Stavro L. Ivanovski, Samuel L. Jackson, Emmanuel Jehin, Martin Jutzi, Ozgur Karatekin, Matthew M. Knight, Ludmilla Kolokolova, Kathryn M. Kumamoto, Michael Küppers, Fiorangela La Forgia, Monica Lazzarin, Jian-Yang Li, Tim A. Lister, Ramin Lolachi, Michael P. Lucas, Alice Lucchetti, Robert Luther, Rahil Makadia, Elena Mazzotta Epifani, Jay McMahon, Gianmario Merisio, Colby C. Merrill, Alex J. Meyer, Patrick Michel, Marco Micheli, Alessandra Migliorini, Kate Minker, Dario Modenini, Fernando Moreno, Naomi Murdoch, Brian Murphy, Shantanu P. Naidu, Hari Nair, Ryota Nakano, Cyrielle Opitom, Jens Ormö, J. Michael Owen, Maurizio Pajola, Eric E. Palmer, Pasquale Palumbo, Paolo Panicucci, Laura M. Parro, Jason M. Pearl, Antti Penttilä, Davide Perna, Elisabeta Petrescu, Petr Pravec, Sabina D. Raducan, K. T. Ramesh, Ryan Ridden-Harper, Juan L. Rizos, Alessandro Rossi, Nathan X. Roth, Agata Rożek, Benjamin Rozitis, Eileen V. Ryan, William H. Ryan, Paul Sánchez, Toni Santana-Ros, Daniel J. Scheeres, Peter Scheirich, Cem Berk Senel, Colin Snodgrass, Stefania Soldini, Damya Souami, Thomas S. Statler, Rachel Street, Timothy J. Stubbs, Jessica M. Sunshine, Nicole J. Tan, Gonzalo Tancredi, Calley L. Tinsman, Paolo Tortora, Filippo Tusberti, James D. Walker, C. Dany Waller, Kai Wünnemann, Marco Zannoni, Yun Zhang
Figure caption: The DART spacecraft in 2021 September, during the pre-ship inspection at the Johns Hopkins Applied Physics Laboratory. In this image, the NEXT-C ion-propulsion engine is at the top of the spacecraft, one of the rolled-up ROSAs is on the right side, and LICIACube is contained on the gold-colored blanketed spacecraft side. In this position, DRACO is not visible as it is pointing at the floor. The main structure of the spacecraft is roughly a cube with dimensions of about 1.3 m, from which other structures extend to result in measurements of roughly 1.8 m in width, 1.9 m in length, and 2.6 m in height.
Paper: Achievement of the Planetary Defense Investigations of the Double Asteroid Redirection Test (DART) Mission
Authors: Nancy L. Chabot, Andrew S. Rivkin, Andrew F. Cheng, Olivier S. Barnouin, Eugene G. Fahnestock, Derek C. Richardson, Angela M. Stickle, Cristina A. Thomas, Carolyn M. Ernst, R. Terik Daly, Elisabetta Dotto, Angelo Zinzi, Steven R. Chesley, Nicholas A. Moskovitz, Brent W. Barbee, Paul Abell, Harrison F. Agrusa, Michele T. Bannister, Joel Beccarelli, Dmitriy L. Bekker, Megan Bruck Syal, Bonnie J. Buratti, Michael W. Busch, Adriano Campo Bagatin, Joseph P. Chatelain, Sidney Chocron, Gareth S. Collins, Luca Conversi, Thomas M. Davison, Mallory E. DeCoster, J. D. Prasanna Deshapriya, Siegfried Eggl, Raymond C. Espiritu, Tony L. Farnham, Marin Ferrais, Fabio Ferrari, Dora Föhring, Oscar Fuentes-Muñoz, Igor Gai, Carmine Giordano, David A. Glenar, Edward Gomez, Dawn M. Graninger, Simon F. Green, Sarah Greenstreet, Pedro H. Hasselmann, Isabel Herreros, Masatoshi Hirabayashi, Marek Husárik, Simone Ieva, Stavro L. Ivanovski, Samuel L. Jackson, Emmanuel Jehin, Martin Jutzi, Ozgur Karatekin, Matthew M. Knight, Ludmilla Kolokolova, Kathryn M. Kumamoto, Michael Küppers, Fiorangela La Forgia, Monica Lazzarin, Jian-Yang Li, Tim A. Lister, Ramin Lolachi, Michael P. Lucas, Alice Lucchetti, Robert Luther, Rahil Makadia, Elena Mazzotta Epifani, Jay McMahon, Gianmario Merisio, Colby C. Merrill, Alex J. Meyer, Patrick Michel, Marco Micheli, Alessandra Migliorini, Kate Minker, Dario Modenini, Fernando Moreno, Naomi Murdoch, Brian Murphy, Shantanu P. Naidu, Hari Nair, Ryota Nakano, Cyrielle Opitom, Jens Ormö, J. Michael Owen, Maurizio Pajola, Eric E. Palmer, Pasquale Palumbo, Paolo Panicucci, Laura M. Parro, Jason M. Pearl, Antti Penttilä, Davide Perna, Elisabeta Petrescu, Petr Pravec, Sabina D. Raducan, K. T. Ramesh, Ryan Ridden-Harper, Juan L. Rizos, Alessandro Rossi, Nathan X. Roth, Agata Rożek, Benjamin Rozitis, Eileen V. Ryan, William H. Ryan, Paul Sánchez, Toni Santana-Ros, Daniel J. Scheeres, Peter Scheirich, Cem Berk Senel, Colin Snodgrass, Stefania Soldini, Damya Souami, Thomas S. Statler, Rachel Street, Timothy J. Stubbs, Jessica M. Sunshine, Nicole J. Tan, Gonzalo Tancredi, Calley L. Tinsman, Paolo Tortora, Filippo Tusberti, James D. Walker, C. Dany Waller, Kai Wünnemann, Marco Zannoni, Yun Zhang
Figure caption: Final 10 images returned by DRACO, spanning from 11.5 s prior to impact to a partial image acquired less than a second prior to impact. The timing and pixel scale of each image (a)–(j) are labeled for each panel. In (a), Dimorphos is roughly 177 m in length. In (i), the final complete image has a pixel scale of 5.5 cm pixel−1 and shows an area approximately 28 m in length (Ernst et al. 2024).
Paper: Achievement of the Planetary Defense Investigations of the Double Asteroid Redirection Test (DART) Mission
Authors: Nancy L. Chabot, Andrew S. Rivkin, Andrew F. Cheng, Olivier S. Barnouin, Eugene G. Fahnestock, Derek C. Richardson, Angela M. Stickle, Cristina A. Thomas, Carolyn M. Ernst, R. Terik Daly, Elisabetta Dotto, Angelo Zinzi, Steven R. Chesley, Nicholas A. Moskovitz, Brent W. Barbee, Paul Abell, Harrison F. Agrusa, Michele T. Bannister, Joel Beccarelli, Dmitriy L. Bekker, Megan Bruck Syal, Bonnie J. Buratti, Michael W. Busch, Adriano Campo Bagatin, Joseph P. Chatelain, Sidney Chocron, Gareth S. Collins, Luca Conversi, Thomas M. Davison, Mallory E. DeCoster, J. D. Prasanna Deshapriya, Siegfried Eggl, Raymond C. Espiritu, Tony L. Farnham, Marin Ferrais, Fabio Ferrari, Dora Föhring, Oscar Fuentes-Muñoz, Igor Gai, Carmine Giordano, David A. Glenar, Edward Gomez, Dawn M. Graninger, Simon F. Green, Sarah Greenstreet, Pedro H. Hasselmann, Isabel Herreros, Masatoshi Hirabayashi, Marek Husárik, Simone Ieva, Stavro L. Ivanovski, Samuel L. Jackson, Emmanuel Jehin, Martin Jutzi, Ozgur Karatekin, Matthew M. Knight, Ludmilla Kolokolova, Kathryn M. Kumamoto, Michael Küppers, Fiorangela La Forgia, Monica Lazzarin, Jian-Yang Li, Tim A. Lister, Ramin Lolachi, Michael P. Lucas, Alice Lucchetti, Robert Luther, Rahil Makadia, Elena Mazzotta Epifani, Jay McMahon, Gianmario Merisio, Colby C. Merrill, Alex J. Meyer, Patrick Michel, Marco Micheli, Alessandra Migliorini, Kate Minker, Dario Modenini, Fernando Moreno, Naomi Murdoch, Brian Murphy, Shantanu P. Naidu, Hari Nair, Ryota Nakano, Cyrielle Opitom, Jens Ormö, J. Michael Owen, Maurizio Pajola, Eric E. Palmer, Pasquale Palumbo, Paolo Panicucci, Laura M. Parro, Jason M. Pearl, Antti Penttilä, Davide Perna, Elisabeta Petrescu, Petr Pravec, Sabina D. Raducan, K. T. Ramesh, Ryan Ridden-Harper, Juan L. Rizos, Alessandro Rossi, Nathan X. Roth, Agata Rożek, Benjamin Rozitis, Eileen V. Ryan, William H. Ryan, Paul Sánchez, Toni Santana-Ros, Daniel J. Scheeres, Peter Scheirich, Cem Berk Senel, Colin Snodgrass, Stefania Soldini, Damya Souami, Thomas S. Statler, Rachel Street, Timothy J. Stubbs, Jessica M. Sunshine, Nicole J. Tan, Gonzalo Tancredi, Calley L. Tinsman, Paolo Tortora, Filippo Tusberti, James D. Walker, C. Dany Waller, Kai Wünnemann, Marco Zannoni, Yun Zhang
Figure caption: Mosaic of Dimorphos, with named features. This high-resolution view of Dimorphos was created by combining the final 10 full-frame images obtained by DRACO and layering the higher-resolution images on top of the lower-resolution ones. Dimorphos is oriented so that its north pole is toward the top of the image. The extent of Dimorphos in the Z-direction is 115 m.
Paper: Achievement of the Planetary Defense Investigations of the Double Asteroid Redirection Test (DART) Mission
Authors: Nancy L. Chabot, Andrew S. Rivkin, Andrew F. Cheng, Olivier S. Barnouin, Eugene G. Fahnestock, Derek C. Richardson, Angela M. Stickle, Cristina A. Thomas, Carolyn M. Ernst, R. Terik Daly, Elisabetta Dotto, Angelo Zinzi, Steven R. Chesley, Nicholas A. Moskovitz, Brent W. Barbee, Paul Abell, Harrison F. Agrusa, Michele T. Bannister, Joel Beccarelli, Dmitriy L. Bekker, Megan Bruck Syal, Bonnie J. Buratti, Michael W. Busch, Adriano Campo Bagatin, Joseph P. Chatelain, Sidney Chocron, Gareth S. Collins, Luca Conversi, Thomas M. Davison, Mallory E. DeCoster, J. D. Prasanna Deshapriya, Siegfried Eggl, Raymond C. Espiritu, Tony L. Farnham, Marin Ferrais, Fabio Ferrari, Dora Föhring, Oscar Fuentes-Muñoz, Igor Gai, Carmine Giordano, David A. Glenar, Edward Gomez, Dawn M. Graninger, Simon F. Green, Sarah Greenstreet, Pedro H. Hasselmann, Isabel Herreros, Masatoshi Hirabayashi, Marek Husárik, Simone Ieva, Stavro L. Ivanovski, Samuel L. Jackson, Emmanuel Jehin, Martin Jutzi, Ozgur Karatekin, Matthew M. Knight, Ludmilla Kolokolova, Kathryn M. Kumamoto, Michael Küppers, Fiorangela La Forgia, Monica Lazzarin, Jian-Yang Li, Tim A. Lister, Ramin Lolachi, Michael P. Lucas, Alice Lucchetti, Robert Luther, Rahil Makadia, Elena Mazzotta Epifani, Jay McMahon, Gianmario Merisio, Colby C. Merrill, Alex J. Meyer, Patrick Michel, Marco Micheli, Alessandra Migliorini, Kate Minker, Dario Modenini, Fernando Moreno, Naomi Murdoch, Brian Murphy, Shantanu P. Naidu, Hari Nair, Ryota Nakano, Cyrielle Opitom, Jens Ormö, J. Michael Owen, Maurizio Pajola, Eric E. Palmer, Pasquale Palumbo, Paolo Panicucci, Laura M. Parro, Jason M. Pearl, Antti Penttilä, Davide Perna, Elisabeta Petrescu, Petr Pravec, Sabina D. Raducan, K. T. Ramesh, Ryan Ridden-Harper, Juan L. Rizos, Alessandro Rossi, Nathan X. Roth, Agata Rożek, Benjamin Rozitis, Eileen V. Ryan, William H. Ryan, Paul Sánchez, Toni Santana-Ros, Daniel J. Scheeres, Peter Scheirich, Cem Berk Senel, Colin Snodgrass, Stefania Soldini, Damya Souami, Thomas S. Statler, Rachel Street, Timothy J. Stubbs, Jessica M. Sunshine, Nicole J. Tan, Gonzalo Tancredi, Calley L. Tinsman, Paolo Tortora, Filippo Tusberti, James D. Walker, C. Dany Waller, Kai Wünnemann, Marco Zannoni, Yun Zhang
Figure caption: LICIACube in 2021 August, prior to its integration on the DART spacecraft. LICIACube is a 6U CubeSat contributed by the Italian Space Agency, with dimensions of 10 × 20 × 30 cm.
Paper: Morphological and Spectral Characterization of Lunar Regolith Breakdown due to Water Ice
Authors: A. Shackelford, K. L. Donaldson Hanna, M. Horton, D. Noce
Figure caption: LHS-1 (left) and LMS-1 (right) samples after 1, 3, and 6 months of freezing compared to unaltered (dry) simulant. MIR spectra are normalized to their respective Christiansen feature (CF), designated by a black, dotted line, and are offset on the y-axis for clarity. The transparency features (longward of the CF) are indicated by a black, dashed line. The first reststrahlen band for each simulant is indicated by a solid blue line.
Paper: Morphological and Spectral Characterization of Lunar Regolith Breakdown due to Water Ice
Authors: A. Shackelford, K. L. Donaldson Hanna, M. Horton, D. Noce
Figure caption: Number of <2 μm fines per particle imaged. The error bars on the counts are given according to the methodology outlined in Section 2.2.1.
Paper: Morphological and Spectral Characterization of Lunar Regolith Breakdown due to Water Ice
Authors: A. Shackelford, K. L. Donaldson Hanna, M. Horton, D. Noce
Figure caption: Primary clump-covering area given in percent (%). Markers with a purple outline indicate that the imaged particle did not fully fill the image boundaries.