Ralph Lorenz

Last updated

Ralph D. Lorenz is a planetary scientist and engineer at the Johns Hopkins Applied Physics Lab. [1] whose research focuses on understanding surfaces, atmospheres, and their interactions on planetary bodies, especially Titan, Venus, Mars, and Earth. [2] He currently serves as Mission Architect of Dragonfly , NASA's fourth selected New Frontiers mission, [3] [4] and as participating scientist on Akatsuki [5] and InSight . [6] He is a Co-Investigator on the SuperCam instrument on the Perseverance rover, responsible for interpreting data from its microphone. He leads the Venus Atmospheric Structure Investigation on the DAVINCI Discovery mission to Venus. He is the recipient of the 2020 International Planetary Probe Workshop (IPPW) Al Seiff memorial award, and the 2022 American Geophysical Union's Fred Whipple Award for contributions to planetary science. [7]

Contents

Education

Lorenz earned a B.Eng. in Aerospace Systems Engineering from the University of Southampton (UK) Department of Aeronautics and Astronautics in 1990. For his thesis "Exploring the Surface of Titan", Lorenz was awarded a PhD in Space Sciences from the University of Kent at Canterbury in 1994. Lorenz spent 1994-2006 at the University of Arizona as a postdoctoral fellow and research scientist. In 2006, he joined the Johns Hopkins Applied Physics Lab. [8] [9]

Research

Lorenz has published over 200 papers on spacecraft exploration of several bodies of the solar system, using scientific instruments and housekeeping data from engineering systems (such as observing the Mars environment and a transit of Deimos [10] via the solar array currents on the InSight lander [11] or measuring the dust and gas in the plumes of Enceladus using Cassini's attitude control system [12] ). He has conducted field research on dust devils, [13] sand dunes and volcanos, exploiting techniques such as kite-borne, [14] timelapse and near-infrared photography. He has also published on the dynamics of Frisbees, [15] the thermodynamics of the drinking bird toy, [16] and the moving rocks ("Sailing Stones") of Racetrack Playa in Death Valley. [17] He documented the migration of sand dunes at the Mos Espa film set in Tunisia, seen on the Star Wars movies. [18] His contributions in scientific history include noting the calculations of Edmond Halley on the size of wings needed for human flight , [19] and the definition [20] of the circumstellar habitable zone by Edward Maunder.

Lorenz has participated in several NASA and ESA missions. He was a Young Graduate Trainee for ESA's Huygens from 1990-1991 and continued on as a member of the Huygens Science Team, designing and building its penetrometer instrument. [8] [9] As a member of the Cassini RADAR team, [21] Lorenz led the planning of Titan radar observations during Cassini's 13 year mission in the Saturn system. Lorenz was selected as a participating scientist on the Japanese mission Akatsuki in 2010 [5] and NASA's InSight mission at Mars in 2017 [6]

He has also been involved in numerous mission concepts, including the Titan Mare Explorer (TiME), [22] the "Billion Dollar Box" Saturnian system study, [23] Titan Airship Explorer, [24] AVIATR, [25] a Mars meteorology and seismology concept, [26] and a Titan submarine [27]

Books

TitleAuthorsPublisherDateISBN
Planetary Exploration with Ingenuity and Dragonfly : Rotary-Wing Flight on Mars and TitanRalph LorenzAmerican Institute of Aeronautics and Astronautics2022978-1624106366
Saturn's Moon Titan Owners' Workshop ManualRalph LorenzHaynes2020978-1785216435
Exploring Planetary ClimateR.D. LorenzCambridge University Press2019978-1108471541
Dust DevilsD. Reiss, R. D. Lorenz, M. Balme, L. Neakrase, A. Pio Rossi, A. Spiga, and J. Zarnecki (Editors)Springer978-9402411331
Planetary Climate before the Space AgeR.D. LorenzAmazon Digital Services LLC2017
NASA/ESA/ASI Cassini-Huygens: 1997 onwards (Cassini orbiter, Huygens probe and future exploration concepts) (Owners' Workshop Manual)R.D. LorenzHaynes Publishing UK2017978-1785211119
Dune Worlds: How Windblown Sand Shapes Planetary LandscapesR.D. Lorenz and J. R. ZimbelmanSpringer2014978-3540897248
Non-equilibrium Thermodynamics and the Production of Entropy: Life, Earth, and Beyond (Understanding Complex Systems)Axel Kleidon, Ralph D. Lorenz (Editors)Springer2005978-3-540-22495-2 and 3-540-22495-5
Spinning Flight: Dynamics of Frisbees, Boomerangs, Samaras, and Skipping StonesR.D. LorenzSpringer2006978-0387307794
Titan Unveiled: Saturn's Mysterious Moon ExploredR.D. Lorenz and J. MittonPrinceton University Press2010978-0691146331
Planetary Landers and Entry ProbesA. Ball, J. Garry, R.D. Lorenz, V. KerzhanovichCambridge University Press2007978-0521820028
Space Systems Failures: Disasters and Rescues of Satellites, Rocket and Space Probes (Springer Praxis Books)D.M. Harland, R.D. LorenzPraxis2005978-0387215198
Lifting Titan's Veil: Exploring the Giant Moon of SaturnR.D. Lorenz and J. MittonCambridge University Press2002978-0521793483

Filmography

Lorenz has appeared in numerous science documentaries and series, including NOVA, NASA's Unexplained Files, Horizon, and Wonders of the Solar System. [28]

Related Research Articles

<span class="mw-page-title-main">Jet Propulsion Laboratory</span> Research and development center and NASA field center in California, United States

Jet Propulsion Laboratory (JPL) is a federally funded research and development center in Pasadena, California, United States. Founded in 1936 by Caltech researchers, the laboratory is now owned and sponsored by the National Aeronautics and Space Administration (NASA) and administered and managed by the California Institute of Technology.

<span class="mw-page-title-main">Titan (moon)</span> Largest moon of Saturn and second-largest moon in Solar System

Titan is the largest moon of Saturn and the second-largest in the Solar System, larger than any of the dwarf planets of the Solar System. It is the only moon known to have a dense atmosphere, and is the only known object in space other than Earth on which clear evidence of stable bodies of surface liquid has been found.

<i>Cassini–Huygens</i> Space research mission sent to the Saturnian system

Cassini–Huygens, commonly called Cassini, was a space-research mission by NASA, the European Space Agency (ESA), and the Italian Space Agency (ASI) to send a space probe to study the planet Saturn and its system, including its rings and natural satellites. The Flagship-class robotic spacecraft comprised both NASA's Cassini space probe and ESA's Huygens lander, which landed on Saturn's largest moon, Titan. Cassini was the fourth space probe to visit Saturn and the first to enter its orbit, where it stayed from 2004 to 2017. The two craft took their names from the astronomers Giovanni Cassini and Christiaan Huygens.

<i>Huygens</i> (spacecraft) European reconnaissance lander sent to Saturns moon Titan

Huygens was an atmospheric entry robotic space probe that landed successfully on Saturn's moon Titan in 2005. Built and operated by the European Space Agency (ESA), launched by NASA, it was part of the Cassini–Huygens mission and became the first spacecraft to land on Titan and the farthest landing from Earth a spacecraft has ever made. The probe was named after the 17th-century Dutch astronomer Christiaan Huygens, who discovered Titan in 1655.

<span class="mw-page-title-main">Enceladus</span> Natural satellite orbiting Saturn

Enceladus is the sixth-largest moon of Saturn. It is about 500 kilometers in diameter, about a tenth of that of Saturn's largest moon, Titan. It is mostly covered by fresh, clean ice, making it one of the most reflective bodies of the Solar System. Consequently, its surface temperature at noon reaches only −198 °C, far colder than a light-absorbing body would be. Despite its small size, Enceladus has a wide variety of surface features, ranging from old, heavily cratered regions to young, tectonically deformed terrain.

<span class="mw-page-title-main">Aerocapture</span> Orbital transfer maneuver

Aerocapture is an orbital transfer maneuver in which a spacecraft uses aerodynamic drag force from a single pass through a planetary atmosphere to decelerate and achieve orbit insertion.

<span class="mw-page-title-main">Marsquake</span> Seismic event occurring on Mars

A marsquake is a quake which, much like an earthquake, would be a shaking of the surface or interior of the planet Mars as a result of the sudden release of energy in the planet's interior, such as the result of plate tectonics, which most quakes on Earth originate from, or possibly from hotspots such as Olympus Mons or the Tharsis Montes. The detection and analysis of marsquakes could be informative to probing the interior structure of Mars, as well as identifying whether any of Mars's many volcanoes continue to be volcanically active.

<span class="mw-page-title-main">Life on Titan</span> Scientific assessments on the microbial habitability of Titan

Whether there is life on Titan, the largest moon of Saturn, is currently an open question and a topic of scientific assessment and research. Titan is far colder than Earth, but of all the places in the Solar System, Titan is the only place besides Earth known to have liquids in the form of rivers, lakes, and seas on its surface. Its thick atmosphere is chemically active and rich in carbon compounds. On the surface there are small and large bodies of both liquid methane and ethane, and it is likely that there is a layer of liquid water under its ice shell. Some scientists speculate that these liquid mixes may provide prebiotic chemistry for living cells different from those on Earth.

<span class="mw-page-title-main">Atmosphere of Titan</span> Thick atmospheric layers of Saturns moon Titan

The atmosphere of Titan is the dense layer of gases surrounding Titan, the largest moon of Saturn. It is the only thick atmosphere of a natural satellite in the Solar System. Titan's lower atmosphere is primarily composed of nitrogen (94.2%), methane (5.65%), and hydrogen (0.099%). There are trace amounts of other hydrocarbons, such as ethane, diacetylene, methylacetylene, acetylene, propane, PAHs and of other gases, such as cyanoacetylene, hydrogen cyanide, carbon dioxide, carbon monoxide, cyanogen, acetonitrile, argon and helium. The isotopic study of nitrogen isotopes ratio also suggests acetonitrile may be present in quantities exceeding hydrogen cyanide and cyanoacetylene. The surface pressure is about 50% higher than on Earth at 1.5 bars which is near the triple point of methane and allows there to be gaseous methane in the atmosphere and liquid methane on the surface. The orange color as seen from space is produced by other more complex chemicals in small quantities, possibly tholins, tar-like organic precipitates.

<span class="mw-page-title-main">Lakes of Titan</span> Hydrocarbon lakes on Titan, a moon of Saturn

Lakes of liquid ethane and methane exist on the surface of Titan, Saturn's largest moon. This was confirmed by the Cassini–Huygens space probe, as had been suspected since the 1980s. The large bodies of liquid are known as maria (seas) and the small ones as lacūs (lakes).

<span class="mw-page-title-main">Kraken Mare</span> Largest hydrocarbon lake on Titan

Kraken Mare is the largest known body of liquid on the surface of Saturn's moon Titan. It was discovered by the space probe Cassini in 2006, and was named in 2008 after the Kraken, a legendary sea monster. It covers an area slightly bigger than the Caspian Sea on Earth, making it the largest known lake in the Solar System.

<span class="mw-page-title-main">Ligeia Mare</span> Sea on Titan

Ligeia Mare is a lake in the north polar region of Titan, the planet Saturn's largest moon. It is the second largest body of liquid on the surface of Titan, after Kraken Mare. Larger than Lake Superior on Earth, it is mostly composed of liquid methane, with unknown but lesser components of dissolved nitrogen and ethane, as well as other organic compounds. It is located at 78° N, 249° W, and has been fully imaged by the Cassini spacecraft. Measuring roughly 420 km (260 mi) by 350 km (217 mi) across, it has a surface area of about 126,000 km2, and a shoreline over 2,000 km (1,240 mi) in length. The lake may be hydrologically connected to the larger Kraken Mare. Its namesake is Ligeia, one of the sirens in Greek mythology.

<span class="mw-page-title-main">Randii Wessen</span> American economist

Randii Ray Wessen is an American astronautics systems engineer specifically involved in planetary exploration, experimental economist, and writer. Dr. Wessen has been an employee of the California Institute of Technology's Jet Propulsion Laboratory since 1984. He is currently the A-Team Lead Study Architect for JPL's Innovation Foundry. On the side, Wessen works with Dr. David Porter of Chapman University in the field of Experimental Economics, where they are designing a system to help allocate resources for building instruments on robotic deep space planetary spacecraft. This proposed system will build on the success of the Cassini Resource Exchange and be applied to NASA's Outer Planet Flagship Missions.

<span class="mw-page-title-main">Titan Mare Explorer</span> Proposed spacecraft lander design

Titan Mare Explorer (TiME) is a proposed design for a lander for Saturn's moon Titan. TiME is a relatively low-cost, outer-planet mission designed to measure the organic constituents on Titan and would have performed the first nautical exploration of an extraterrestrial sea, analyze its nature and, possibly, observe its shoreline. As a Discovery-class mission it was designed to be cost-capped at US$425 million, not counting launch vehicle funding. It was proposed to NASA in 2009 by Proxemy Research as a scout-like pioneering mission, originally as part of NASA's Discovery Program. The TiME mission design reached the finalist stage during that Discovery mission selection, but was not selected, and despite attempts in the U.S. Senate failed to get earmark funding in 2013. A related Titan Submarine has also been proposed.

<span class="mw-page-title-main">Flyby (spaceflight)</span> Flight event at some distance from the object

A flyby is a spaceflight operation in which a spacecraft passes in proximity to another body, usually a target of its space exploration mission and/or a source of a gravity assist to impel it towards another target. Spacecraft which are specifically designed for this purpose are known as flyby spacecraft, although the term has also been used in regard to asteroid flybys of Earth for example. Important parameters are the time and distance of closest approach.

<i>Dragonfly</i> (Titan space probe) Robotic space exploration mission to Titan

Dragonfly is a planned spacecraft and NASA mission to send a robotic rotorcraft to the surface of Titan, the largest moon of Saturn. It is planned to be launched in July 2028 and arrive in 2034. It would be the first aircraft on Titan and is intended to make the first powered and fully controlled atmospheric flight on any moon, with the intention of studying prebiotic chemistry and extraterrestrial habitability. It would then use its vertical takeoffs and landings (VTOL) capability to move between exploration sites.

<span class="mw-page-title-main">Moon Diver (spacecraft)</span>

Moon Diver is a proposed lunar mission concept by NASA's Jet Propulsion Laboratory that would employ a robotic lander and a – distant coaxial – two-wheeled rover called Axel to investigate the exposed geological layers on the walls of a deep lunar pit.

<span class="mw-page-title-main">Sushil Atreya</span> Indian–American engineer and planetary scientist

Sushil K. Atreya is a planetary scientist, educator, and researcher. Atreya is a professor of Climate and Space Sciences and Engineering at the University of Michigan, Ann Arbor.

References

  1. "JHUAPL - , Ralph, Lorenz - Science Research Portal". secwww.jhuapl.edu. Retrieved October 27, 2019.
  2. Zacny, K.; Lorenz, R.; Rehnmark, F.; Costa, T.; Sparta, J.; Sanigepalli, V.; Mank, Z.; Yen, B.; Yu, D.; Bailey, J.; Bergman, D. (2019). "Application of Pneumatics in Delivering Samples to Instruments on Planetary Missions". 2019 IEEE Aerospace Conference. pp. 1–13. doi:10.1109/AERO.2019.8741887. ISBN   978-1-5386-6854-2. S2CID   195222645.
  3. Voosen, Paul (July 5, 2019). "NASA to fly drone on Titan". Science. 365 (6448): 15.1–15. Bibcode:2019Sci...365...15V. doi:10.1126/science.365.6448.15-a. ISSN   0036-8075. PMID   31273103. S2CID   195807081.
  4. JHU APL. "Dragonfly Team". Dragonfly. Retrieved October 23, 2019.
  5. 1 2 "NASA - Scientists Chosen to Help on Venus Climate Orbiter". www.nasa.gov. Retrieved October 23, 2019.
  6. 1 2 "InSight Participating Scientist Program (INSTPSP) Abstracts of selected proposals" (PDF). NSPIRES.
  7. "Lectures". agu.org. Archived from the original on December 28, 2022. Retrieved December 28, 2022.
  8. 1 2 "Ralph D Lorenz - Curriculum Vitae". arizona.edu. Retrieved August 30, 2023.
  9. 1 2 Spring 2020, Dale Keiger / Published (March 19, 2020). "Destination Titan". The Hub. Retrieved March 25, 2020.{{cite web}}: CS1 maint: numeric names: authors list (link)
  10. Lorenz, Ralph D.; Lemmon, Mark T.; Mueller, Nils (2020). "A Transit Lightcurve of Deimos, Observed with the InSight Solar Arrays". Research Notes of the American Astronomical Society. 4 (4): 57. Bibcode:2020RNAAS...4...57L. doi: 10.3847/2515-5172/ab8d21 . S2CID   219008928.
  11. Lorenz, Ralph D.; Lemmon, Mark T.; Maki, Justin; Banfield, Donald; Spiga, Aymeric; Charalambous, Constantinos; Barrett, Elizabeth; Herman, Jennifer A.; White, Brett T.; Pasco, Samuel; Banerdt, W. Bruce (2020). "Scientific Observations with the InSight Solar Arrays: Dust, Clouds and Eclipses on Mars". Earth and Space Science. 7 (5): e2019EA000992. Bibcode:2020E&SS....700992L. doi: 10.1029/2019EA000992 . PMC   7375148 . PMID   32715027.
  12. Lorenz, R. D.; Burk, T. A. (2018). "Enceladus Plume Density from Cassini Spacecraft Attitude Control Data". Icarus. 300: 200–202. Bibcode:2018Icar..300..200L. doi:10.1016/j.icarus.2017.09.003. PMC   6278931 . PMID   30524143.
  13. "A Roundup of Dust Devil Research". The Planetary Society. Retrieved August 30, 2023.
  14. Lorenz, Ralph D.; Scheidt, Stephen P. (2014). "Compact and inexpensive kite apparatus for geomorphological field aerial photography, with some remarks on operations". Georesj. 3–4: 1–8. Bibcode:2014GeoRJ...3....1L. doi: 10.1016/j.grj.2014.06.001 .
  15. Lorenz, Ralph D. (2005). "Flight and attitude dynamics measurements of an instrumented Frisbee". Measurement Science and Technology. 16 (3): 738–748. Bibcode:2005MeScT..16..738L. doi:10.1088/0957-0233/16/3/017. S2CID   16105503.
  16. Lorenz, Ralph (2006). "Finite-time thermodynamics of an instrumented drinking bird toy". American Journal of Physics. 74 (8): 677–682. Bibcode:2006AmJPh..74..677L. doi:10.1119/1.2190688.
  17. Lorenz, R. D.; Norris, J. M.; Jackson, B. K.; Norris, R. D.; Chadbourne, J. W.; Ray, J. (August 28, 2014). "Trail formation by ice-shoved "sailing stones" observed at Racetrack Playa, Death Valley National Park". Earth Surface Dynamics Discussions. 2 (2): 1005–1022. Bibcode:2014ESuDD...2.1005L. doi: 10.5194/esurfd-2-1005-2014 .
  18. "Dunes on Tatooine". The Planetary Society. Retrieved August 30, 2023.
  19. "Edmond Halley's Aeronautical Calculations on the Feasibility of Manned Flight in 1691". Journal of Aeronautical History. 2012 (2). 2012.
  20. Lorenz, Ralph D. (2020). "Maunder's Work on Planetary Habitability in 1913: Early Use of the term "Habitable Zone" and a "Drake Equation" Calculation". Research Notes of the American Astronomical Society. 4 (79): 79. Bibcode:2020RNAAS...4...79L. doi: 10.3847/2515-5172/ab9831 . S2CID   219930646.
  21. "The Team | Cassini Mission". NASA Solar System Exploration. Retrieved October 23, 2019.
  22. Stofan, E.; Lorenz, R.; Lunine, Jonathan I.; Bierhaus, E. B.; Clark, B.; Mahaffy, P. R.; Ravine, M. (2013). "TiME - the Titan Mare Explorer". 2013 IEEE Aerospace Conference. p. 211. Bibcode:2013aero.confE.211S. doi:10.1109/AERO.2013.6497165. ISBN   978-1-4673-1813-6. S2CID   17290531.
  23. Spilker, T. R.; Reh, K. R.; Elliott, J. O.; Lorenz, R.; Spencer, J. (2008). "The "Billion Dollar Box" Study of Science Missions to Saturnian Satellites". 2008 IEEE Aerospace Conference. pp. 1–9. doi:10.1109/AERO.2008.4526246. ISBN   978-1-4244-1487-1. S2CID   23343537.
  24. Hall, J. L.; Kerzhanovich, V. V.; Jones, J. A.; Cutts, J. A.; Yavrouian, A. A.; Colozza, A.; Lorenz, R. D. (2002). "Titan Airship Explorer". Proceedings, IEEE Aerospace Conference. Vol. 1. pp. 1–336. doi:10.1109/AERO.2002.1036852. ISBN   0-7803-7231-X. S2CID   110089994.
  25. Barnes, Jason W.; Lemke, Lawrence; Foch, Rick; McKay, Christopher P.; Beyer, Ross A.; Radebaugh, Jani; Atkinson, David H.; Lorenz, Ralph D.; Le Mouélic, Stéphane; Rodriguez, Sebastien; Gundlach, Jay (2012). "AVIATR—Aerial Vehicle for In-situ and Airborne Titan Reconnaissance". Experimental Astronomy. 33 (1): 55–127. doi: 10.1007/s10686-011-9275-9 . ISSN   1572-9508.
  26. Lorenz, R.; Oleson, S.; Cataldo, R.; Schmitz, P.; Colozza, A.; Bairstow, B.; Lee, Y.; Amini, R. (2014). "MASER: A Mars meteorology and seismology mini-network mission concept enabled by Milliwatt-RPS". 2014 IEEE Aerospace Conference. pp. 1–11. doi:10.1109/AERO.2014.6836397. ISBN   978-1-4799-1622-1. S2CID   46223014.
  27. Oleson, Steve (July 2015). "Phase I Final Report: Titan Submarine" (PDF). Retrieved August 13, 2023.
  28. "Ralph Lorenz". IMDb .