Search Results - "Bland, Michael T."

Refine Results
  1. 1

    Composition and structure of the shallow subsurface of Ceres revealed by crater morphology by Bland, Michael T., Raymond, Carol A., Schenk, Paul M., Fu, Roger R., Kneissl, Thomas, Pasckert, Jan Hendrik, Hiesinger, Harry, Preusker, Frank, Park, Ryan S., Marchi, Simone, King, Scott D., Castillo-Rogez, Julie C., Russell, Christopher T.

    Published in Nature geoscience (01-07-2016)
    “…Before NASA’s Dawn mission, the dwarf planet Ceres was widely believed to contain a substantial ice-rich layer below its rocky surface. The existence of such a…”
    Get full text
    Journal Article
  2. 2

    Predicted crater morphologies on Ceres: Probing internal structure and evolution by Bland, Michael T.

    Published in Icarus (New York, N.Y. 1962) (01-09-2013)
    “…•We simulate viscous relaxation of impact craters in a putative ice layer on Ceres.•We predict extensive crater relaxation.•Complete crater erasure is…”
    Get full text
    Journal Article
  3. 3

    The vanishing cryovolcanoes of Ceres by Sori, Michael M., Byrne, Shane, Bland, Michael T., Bramson, Ali M., Ermakov, Anton I., Hamilton, Christopher W., Otto, Katharina A., Ruesch, Ottaviano, Russell, Christopher T.

    Published in Geophysical research letters (16-02-2017)
    “…Ahuna Mons is a 4 km tall mountain on Ceres interpreted as a geologically young cryovolcanic dome. Other possible cryovolcanic features are more ambiguous,…”
    Get full text
    Journal Article
  4. 4

    Enceladus' extreme heat flux as revealed by its relaxed craters by Bland, Michael T., Singer, Kelsi N., McKinnon, William B., Schenk, Paul M.

    Published in Geophysical research letters (16-09-2012)
    “…Enceladus' cratered terrains contain large numbers of unusually shallow craters consistent with deformation by viscous relaxation of water ice under conditions…”
    Get full text
    Journal Article
  5. 5

    Current Status of the Community Sensor Model Standard for the Generation of Planetary Digital Terrain Models by Hare, Trent M., Kirk, Randolph L., Bland, Michael T., Galuszka, Donna M., Laura, Jason R., Mayer, David P., Redding, Bonnie L., Wheeler, Benjamin H.

    Published in Remote sensing (Basel, Switzerland) (01-02-2024)
    “…The creation of accurate elevation models (topography) from stereo images are critical for a large variety of geospatial activities, including the production…”
    Get full text
    Journal Article
  6. 6

    How Well Do We Know Europa’s Topography? An Evaluation of the Variability in Digital Terrain Models of Europa by Bland, Michael T., Kirk, Randolph L., Galuszka, Donna M., Mayer, David P., Beyer, Ross A., Fergason, Robin L.

    Published in Remote sensing (Basel, Switzerland) (01-12-2021)
    “…Jupiter’s moon Europa harbors one of the most likely environments for extant extraterrestrial life. Determining whether Europa is truly habitable requires…”
    Get full text
    Journal Article
  7. 7

    Ceres internal structure from geophysical constraints by King, Scott D., Castillo‐Rogez, Julie C., Toplis, M. J., Bland, Michael T., Raymond, Carol A., Russell, Christopher T.

    Published in Meteoritics & planetary science (01-09-2018)
    “…Thermal evolution modeling has yielded a variety of interior structures for Ceres, ranging from a modestly differentiated interior to more advanced evolution…”
    Get full text
    Journal Article
  8. 8

    Improving the Usability of Galileo and Voyager Images of Jupiter's Moon Europa by Bland, Michael T., Weller, Lynn A., Archinal, Brent A., Smith, Ethan, Wheeler, Benjamin H.

    Published in Earth and space science (Hoboken, N.J.) (01-12-2021)
    “…NASA's Voyager 1, Voyager 2, and Galileo spacecraft acquired hundreds of images of Jupiter's moon Europa. These images provide the only moderate‐ to…”
    Get full text
    Journal Article
  9. 9

    Cryovolcanic rates on Ceres revealed by topography by Sori, Michael M., Sizemore, Hanna G., Byrne, Shane, Bramson, Ali M., Bland, Michael T., Stein, Nathaniel T., Russell, Christopher T.

    Published in Nature astronomy (01-12-2018)
    “…Cryovolcanism, defined here as the extrusion of icy material from depth, may be an important planetary phenomenon in shaping the surfaces of many worlds in the…”
    Get full text
    Journal Article
  10. 10

    The orbital–thermal evolution and global expansion of Ganymede by Bland, Michael T., Showman, Adam P., Tobie, Gabriel

    Published in Icarus (New York, N.Y. 1962) (01-03-2009)
    “…The tectonically and cryovolcanically resurfaced terrains of Ganymede attest to the satellite's turbulent geologic history. Yet, the ultimate cause of its…”
    Get full text
    Journal Article
  11. 11

    Ceres’ Broad‐Scale Surface Geomorphology Largely Due To Asymmetric Internal Convection by King, Scott D., Bland, Michael T., Marchi, Simone, Raymond, Carol A., Russell, Christopher T., Scully, Jennifer E. C., Sizemore, Hanna G.

    Published in AGU advances (01-06-2022)
    “…While we now know much about the volatile‐rich world of Ceres from the Dawn mission, the deep interior remains something of an enigma, shrouded by a crust…”
    Get full text
    Journal Article
  12. 12

    The effects of strain localization on the formation of Ganymede’s grooved terrain by Bland, Michael T., McKinnon, William B., Showman, Adam P.

    Published in Icarus (New York, N.Y. 1962) (01-11-2010)
    “…We investigate the effects of strain localization on the formation of Ganymede’s grooved terrain by numerically modeling the extension of an ice lithosphere in…”
    Get full text
    Journal Article
  13. 13
  14. 14

    The interior structure of Ceres as revealed by surface topography by Fu, Roger R., Ermakov, Anton I., Marchi, Simone, Castillo-Rogez, Julie C., Raymond, Carol A., Hager, Bradford H., Zuber, Maria T., King, Scott D., Bland, Michael T., Cristina De Sanctis, Maria, Preusker, Frank, Park, Ryan S., Russell, Christopher T.

    Published in Earth and planetary science letters (15-10-2017)
    “…Ceres, the largest body in the asteroid belt (940 km diameter), provides a unique opportunity to study the interior structure of a volatile-rich dwarf planet…”
    Get full text
    Journal Article
  15. 15

    Mountain building on Io driven by deep faulting by Bland, Michael T., McKinnon, William B.

    Published in Nature geoscience (01-06-2016)
    “…The high relief on Jupiter’s moon Io has been linked to compression due to global subsidence. Simulations show that Io’s mountains may form along thrust faults…”
    Get full text
    Journal Article
  16. 16
  17. 17

    Increasing the Usability and Accessibility of Voyager 2 Images of Triton by Bland, Michael T., Martin, Emily S., Patthoff, Alex

    Published in The planetary science journal (01-05-2024)
    “…Abstract Much of what we know about Neptune’s moon Triton was inferred from the analysis of images returned by the Voyager 2 mission, the only spacecraft to…”
    Get full text
    Journal Article
  18. 18

    Relaxed impact craters on Ganymede: Regional variation and high heat flows by Singer, Kelsi N., Bland, Michael T., Schenk, Paul M., McKinnon, William B.

    Published in Icarus (New York, N.Y. 1962) (15-05-2018)
    “…•Apparent depths for 180 craters on Ganymede were measured.•Many craters exhibit substantially reduced depths compared to fresh craters.•Regions near the south…”
    Get full text
    Journal Article
  19. 19

    Constraining the heat flux between Enceladus’ tiger stripes: Numerical modeling of funiscular plains formation by Bland, Michael T., McKinnon, William B., Schenk, Paul M.

    Published in Icarus (New York, N.Y. 1962) (01-11-2015)
    “…•Enceladus’ funiscular terrain consists of short wavelength, periodic ridges.•We simulate lithospheric shortening to test whether the terrain formed by…”
    Get full text
    Journal Article
  20. 20