EGU21-3308
https://doi.org/10.5194/egusphere-egu21-3308
EGU General Assembly 2021
© Author(s) 2021. This work is distributed under
the Creative Commons Attribution 4.0 License.

Interstellar Probe: A Mission to the Heliospheric Boundary and Interstellar Medium for the Next Decade

Pontus Brandt1, Ralph McNutt1, Elena Provornikova1, Carey Lisse1, Kathleen Mandt1, Kirby Runyon1, Abigail Rymer1, Parisa Mostafavi1, Robert DeMajistre1, Edmond Roelof1, Drew Turner1, Matthew Hill1, James Kinnison1, Gabe Rogers1, Clayton Smith1, Glen Fountain1, David Copeland1, Peter Kollmann1, Reza Ashtari1, Robert Stough2, and the The Interstellar Probe Study Team*
Pontus Brandt et al.
  • 1The Johns Hopkins University Applied Physics Laboratory, SRP, Laurel, Maryland, United States of America (pontus.brandt@jhuapl.edu)
  • 2Marshall Space Flight Center, Spacecraft / Payload Integration and Evolution (SPIE) Office, Huntsville, Alabama, United States of America
  • *A full list of authors appears at the end of the abstract

An Interstellar Probe mission to the Very Local Interstellar Medium (VLISM) would bring new scientific discoveries of the mechanisms upholding our vast heliosphere and directly sample the unexplored Local Interstellar Clouds that our Sun is moving through in relatively short galactic timescales. As such, it would represent Humanity's first explicit step in to the galaxy and become perhaps NASA's boldest step in space exploration. Such a mission has been discussed and studied since 1960, but the stumbling block has often been propulsion. Now this hurdle has been overcome by the availability of new and larger launch vehicles. An international team of scientists and experts are now progressing towards the final year of a NASA-funded study led by The Johns Hopkins University Applied Physics Laboratory (APL) to develop pragmatic example mission concepts for an Interstellar Probe with a nominal design lifetime of 50 years. Together with the Space Launch System (SLS) Office at the NASA Marshall Space Flight Center, the team has analyzed dozens of launch configurations and demonstrate that asymptotic speeds in excess of 7.5 Astronomical Units (AU) per year can be achieved using existing or near-term propulsion stages with a powered or passive Jupiter Gravity Assist (JGA). These speeds are more than twice that of the fastest escaping man-made spacecraft to date, which is Voyager 1 currently at 3.59 AU/year. An Interstellar Probe would therefore reach the Termination Shock (TS) in less than 12 years and cross the Heliopause into the VLISM after about 16 years from launch.

In this presentation we provide an overview and update of the study, the science mission concept, discuss the compelling discoveries that await, and the associated example science payload, measurements and operations ensuring a historic data return that would push the boundaries of space exploration by going where no one has gone before.

The Interstellar Probe Study Team:

Stuart Bale, William Kurth, Andre Galli

How to cite: Brandt, P., McNutt, R., Provornikova, E., Lisse, C., Mandt, K., Runyon, K., Rymer, A., Mostafavi, P., DeMajistre, R., Roelof, E., Turner, D., Hill, M., Kinnison, J., Rogers, G., Smith, C., Fountain, G., Copeland, D., Kollmann, P., Ashtari, R., and Stough, R. and the The Interstellar Probe Study Team: Interstellar Probe: A Mission to the Heliospheric Boundary and Interstellar Medium for the Next Decade, EGU General Assembly 2021, online, 19–30 Apr 2021, EGU21-3308, https://doi.org/10.5194/egusphere-egu21-3308, 2021.

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