Sunday, January 31, 2010

Decadal Survey Update

Steve Squyres has just published the January update for the Decadal Survey.  I'd characterize the current efforts as laying the foundation for the eventual plan.  Like laying the foundation for a building, this isn't the glamorous work, but without it, the edifice won't stand.  Three sets of activity are underway:

The steering committee has been focusing on two key threats to the ability to carry out a robust program: the rapidly escalating cost of launch vehicles and the plutonium-238 shortage.  Later this winter it will look at the technology development program.

The panels (each focuses on a group of destinations, for example Mars or the outer planet satellites) are nearing completion of their assessments of the key science goals for the next decade.  Eventually, once these lists are merged, these goals will be used to prioritize a set of missions.  Their reports, if memory serves me right, are due out this spring.

In parallel with the goals assessments, 21 mission concepts are being defined and/or having cost estimates prepared.  This effort will lead to determining which concepts are technically ready and can fit within the budget.  Since the last update, one new concept has been added, a Venus Tessera Lander.  While lowland Venus lander studies already were underway, this study focuses on how to land in the rugged highlands of Venus.

---------------------------

Monday will see the release of the President's budget proposal for fiscal year 2011, including for NASA's planetary program.  I'll publish an analysis Monday evening or Tuesday morning.  Then later next week I'll publish an entry on missions to study the trace gases in the Martian atmosphere.

Tuesday, January 26, 2010

What a Budget Freeze Might Mean

Apparently, large parts of the American federal budget will be subjected to a budget freeze for three years in the President's upcoming 2011 budget proposal.  Word on the street is that NASA as a whole will get a slight increase, but my betting is that any increase will go to manned spaceflight and Earth science missions.

In a week we'll know what the proposed budget will be for NASA's planetary program.  In the meantime, I did a little work with Excel to see what a budget freeze in the planetary program would mean.  Typically, inflation runs at around 3% in a year. Consumer inflation in 2009 was 2.7%; I don't know what the inflation rate was for aerospace spending and will use 3% as a guideline.  If the planetary program were subjected to a three year budget freeze and then budgets rose to cover inflation, the loss of spending power would be a fall between the burdened costs of a Discovery and a New Frontiers mission (~$950M FY09 dollars).  If the budget freeze were extended over an entire decade, the loss of spending power would be equivalent to a Discovery and a New Frontiers mission (~$1.8B).

Saturday, January 23, 2010

My Stab at a Decadal Priority List

We're in a bit of a hiatus in terms of Decadal Survey news.  The next round of meetings for the discipline panels (e.g., Inner Planets) aren't scheduled to occur until April and May.  The Steering Committee will meeting in late February, but it appears to be focusing primarily on enabling technologies.

I've been following the Survey's progress probably as closely as anyone outside of the process has.  During the last few months, I've been wondering what criteria I would use to set priorities.  And that led me to thinking what priorities would I choose.

I want to emphasize that what follows isn't an attempt to persuade anyone about what the priorities should be.  Your opinions are as valid as mine, and except for perhaps a lucky one or two readers who may be involved in the process, your and my opinions are likely to have the same impact.  However, I often learn more from a carefully crafted argument than I do from just reading the facts (which is why I read the opinions page of the newspaper more regularly than the front page).  So here goes (and I hope that you find this carefully crafted).

A successful program has to meet a number of goals:
  1. It must be fiscally possible.  That is, it has to fit within the $12-12.5B budget expected for the next decade.
  2. It must be compelling to the public and to the politicians who will have to prioritize dollars spent here over other worthy projects over the course of a decade.
  3. It must significantly advance our scientific understanding of the solar system.
  4. It should provide a balance between types of solar system bodies.  The list of discipline panels suggests the breadth possible: Inner planets, Mars, giant planets, outer solar system satellites, and primitive bodes

There's another criteria that may or may not be adopted by the Survey, but I think should be.  It is quite possible that over the course of the decade that the budget for planetary exploration may be cut.  (Recent reports that NASA will not receive a $1B budget boost for the next fiscal year leads credence to this fear.  Planetary missions will be in competition with the politically popular manned and Earth observation programs.)  I believe that the prioritized list of missions should remain useful if budget cuts occur.

I think that the most critical decision the Survey will face will be setting the balance between the large Flagship missions and smaller New Frontiers and Discovery class missions.  Two Flagship missions are likely candidates, Mars Sample Return (MSR) and the Jupiter Europa Orbiter (JEO).  These missions are large enough that they together would chew up three quarters of the budget.  However, it could be argued that these two large missions would provide the greatest scientific return of any missions on the candidate list.  There would also sufficient budget to fly the Mars Trace Gas Oribiter, support the ExoMars rover (as part of MSR's MAX-C rover), and fly three smaller missions which could visit the inner planets and primitive bodies (MSR and JEO would take care of Mars, the giant planets, and outer solar system satellites).



Example of a priority list and budget for a program that emphasizes Flagship missions.  Figures are in $Bs, and use either published estimates or my own best guesses.  New Frontiers and Discovery figures include the PI budget (~$650M and ~$450M) plus launches and other overhead.

I have two concerns about this priority list.  First, MSR and JEO could easily experience large cost overruns that prevent missions to other destinations.  Second, large missions make tempting targets for politicians looking to cut budgets.  Both of these missions would have to find political support across at least two Presidents and about a half dozen Congresses.  (In America, we elect the entire House of Representatives and a third of the Senators every two years, which counts as a new Congress (even though the reelection rate is so high that 'new' may be a misnomer).)  The counter argument is that scientific support for these big missions would be great enough to shield them from cancellation.  There's some truth to this (look at the survival of the James Webb telescope and the Mars Science Laboratory despite massive overruns).  On the other hand, a number of large science programs have been cut in the past; remember the Comet Rendezvous and Asteroid Flyby (CRAF) sister ship of Cassini cut in the early 1990s.

I instead prefer a priority list that focuses on smaller missions to many solar system targets.  Then if budgets permit, I would fly the full JEO mission and the first component of MSR, the MAX-C rover, as the lowest priorities.  This way, if budgets are cut, there is still a robust program of missions to a number of destinations.



How I would prioritized my list of missions based on mission concepts that have been studied to date.

While this list may seem like a scattered set of missions, there are some themes.  Mars remains the top priority with over a third of the budget.  Icy moons would be a priority with missions to the Jovian moons, Titan, Enceladus, and Triton.  The single Venus mission looks lonesome, but I see it as the NASA contribution to an international flotilla to that world.  However, the primitive bodies scientists would rightfully feel left out with just a single Discovery mission.  (I left both the Venus and primitive bodies missions as placeholders.  Depending on which missions are selected in the current New Frontiers and Discovery competitions, the priorities for these missions may change.)  It was really hard leaving off some missions I really like and that would produce great science like the Io Volcanic Observer (IVO).  (However, I could imagine a scenario where a line of New Frontiers class spacecraft were built using nearly identical spacecraft for the JMO, TEO, and Argo missions and then the savings might fund IVO.)

You'll note that I don't specify specific targets for several Discovery and New Frontiers class missions.  I have concerns about the totally open competitions to date, which make it impossible to know which missions will fly.  A consequence of this is that NASA has a harder time prioritizing its technology development funds.  If, however, NASA knows that it will be flying a lander to Venus, it can prioritize the appropriate development work.  Prioritizing specific targets also makes it easier to put together international collaborations.  If NASA will be flying a Titan/Enceladus observer, then perhaps another space agency would fund a Saturn atmospheric probe or a Titan lander to ride along.

As I said in the beginning, there's nothing special about my list.  However, I hope that it will get you to thinking about what priorities you would set.

Oh, and as the Survey studies additional mission concepts, it is likely that my list of priorities will change.  There's a number of exciting concepts under study.

Thursday, January 21, 2010

Russian and European Venus Ambitions

The VEXAG meeting last October (presentations were posted just a couple of weeks ago) had presentations on Russia's Venera-D mission and ESA's possible European Venus Explorer (EVE).   Both are in the definition stage, with the Russian mission apparently funded and a European contribution under consideration.

The Venera-D mission at its most expansive would consist of a capable science orbiter, a lander, and several balloons, and one or more drop sondes that would profile the atmosphere (and take descent images?).  This would be a very sophisticated mission.  A group of U.S. scientists considered a mission of similar scope, the Venus Climate Flagship (or Flagship Lite), and estimated its cost to be $1.7B.  Russia ended its presentation with a slide that read, "We Invite Everybody for Cooperation," suggesting that it would like to share the expenses.



 From the Venera-D presentation.  This scenario appears to be the most ambitious of several configurations of the mission under consideration.

ESA is considering contributing to the mission by providing a balloon platform that would study the upper atmosphere for seven days.  Apparently Japan is considering a second balloon platform that would explore the mid atmosphere.  (It's hard to tell how serious ESA's consideration is.  The presentation to be originally from mid 2008.  EVE was not selected as a candidate for the next round of mission selection.  However, I've read that interest in contributing to Venera-D is growing in Europe.)



From the European Venus Explorer Exploration

Editorial Thoughts: The Venera-D mission is ambitious and would significantly advance our knowledge of Venus.  It's not clear how important international participation would be to see it fully implemented.  If Europe decides not to participate, the mission likely would be less ambitious.  It's not clear how Russia might reduce the scope of the mission.  It might drop the balloon element, or alternatively it might implement its own balloon platform and reduce the capabilities of the orbiter, for example.

NASA's role in the proposed Russia-ESA-JAXA mission apparently would be minor.  However, NASA could potentially make significant complimentary studies.  If the SAGE New Frontiers lander were to be selected, then the NASA and Russian landers could be sent to complimentary sites.  (It appears from the Venera-D presentation that the landers would have similar capabilities.)  Both missions would launch in 2016.

In addition, the Venera-D orbiter apparently would not carry a mapping radar instrument (although a sub-surface sounding radar might be carried).  A NASA mission such as the proposed RAVEN Discovery mission could fill this hole and re-image Venus' surface.

 Venus is currently being explored by Europe's Venus Express mission, and Japan will soon launch an orbiter to study the climate.  Combine these missions with Venera-D and possibly a NASA mission or two, and our knowledge of Venus could see the kind of explosion that has come from the series of Mars missions over the last decade and a half.

Resources:

Venera-D: http://www.lpi.usra.edu/vexag/oct2009/presentations/zasovaVeneraD.pdf

European Venus Explorer: http://www.lpi.usra.edu/vexag/oct2009/presentations/chassefiereEuropeanVenusExplorer.pdf

Monday, January 18, 2010

SAGE New Frontiers Proposal (Enhanced)

Bruce Moomaw found the time to pull some more information out the the SAGE presentation (see link below), so I'm reposting this with his additions (in italics).


At the October VEXAG meeting (presentations were posted just a few days ago), Larry Esposito the principal investigator for the proposed SAGE lander presented some details of the mission.  In addition to the information in the slides reproduced below, there were several interesting tidbits:

  • The lander should last several hours on the surface
  • Surface composition would be measured at depths of 3-10 cm (depending on surface material) using a surface excavation sampling arm
  • Composition measurements would be made using a LIBS/Raman instrument steerable in one direction.  [This suggests that the choice of sampling area might be limited by both the reach of the sampling arm and the pointing capabilities of the LIBS/Raman instrument.]
  • Images of the surface would be made during descent in the near infrared.  Surface panoramas and microscopic images of the excavation site would be taken on the surface.
  • Descent through the atmosphere would last ~ 1 hour and the lander would survive ~3 hours on the surface

In addition to Esposito's presentation, the meeting also had a short presentation on LIBS/Raman instruments for Venus.  Check it out if you want to know more about this approach.

Bruce's additional comments follow:


I suspect that arm is going to extend straight down from the side of the craft to grind into the surface, which would explain how the Microscopic Camera could obtain "views of the excavation area" with maximum resolution.  Whether the tiltable LIBS/Raman instrument will swing its viewfield farther out from the spacecraft or just sweep it from one side to the other is unknown to me.

Page 10 of that presentation includes the listed acronyms of the onboard experiments, which I translate as follows:

FBC = FlyBy Camera (on the carrier, to image local cloud patterns and thus perhaps winds)

DPC/MC = Descent-Panoramic Camera/Microscopic Camera.  (The Descent Camera part of this package will take "NIR" -- that is, near-IR -- images of the suface during descent; if taken through several different filters, it could also provide some mineralogical data.)

ASI = Atmospheric Structure Instrument (temperature, pressure and wind sensors and accelerometers to measure entry deceleration and thus upper-air density)

DWE USO = Doppler Wind Experiment/Ultra-Stable Oscillator (the latter to allow precise tracking of the craft during its descent for the Doppler wind data)

NMS = Neutral Mass Spectrometer (atmospheric analysis)

TLS = Tunable Laser Spectrometer (to analyze important trace isotopes in the atmospheric gases -- especially, I imagine, carbon and oxygen)

NAGRS = Neutron-Activated Gamma Ray Spectrometer.  (This instrument would both measure natural gamma rays from uranium, thorium and potassium in the surface, and -- when the vacuum-tube neutron source is on -- it would measure a very wide variety of other elements, including trace elements.  It would presumably be located inside the lander's body and might analyze as much as a cubic meter of material underneath the lander.  Note also from the little bar chart of instrument operating altitudes on page 12 that it would start its natural gamma-ray measurements as high as 60 km above the surface.)

LIBS/Raman = Laser-Induced Breakdown Spectrometer and Raman spectrometer.  (This instrument, as noted by Van, would use brief bursts from one color laser to strike sparks of glowing plasma off the surface material and take visual spectra of them for detailed major and minor element analysis, and another color laser to scatter traces of "Raman scattered" light off the surface and analyze their spectrum to obtain really detailed and comprehensive data on the mineralogy of the surface.  A LIBS spectrometer is carried on the Mars Science Laboratory, and a Raman spectrometer on ExoMars -- the latter in part because Raman is also good at detecting trace organics, although not nearly as good as mass spectrometric analysis.)

Note that the "excavation sampling arm" (which has "calibration targets" on it, doubtless for the LIBS/Raman instrument) would grind 3-10 cm into the surface depending on surface hardness.  I don't know how they'll decide when to stop grinding -- probably a combination of grinding time and penetration depth -- but, given that Venus' surface is likely very intensely chemically weathered by that superhot and high-pressure CO2 atmosphere and its trace gases, trying to expose and analyze an unweathered (or at least less weathered) surface is very important.

The science payload is significantly different from the one on SAGE the first time it was proposed.  In particular, that first time it carried a combined X-ray diffractometer and X-ray fluorescence spectrometer -- in fact, exactly the same "CheMin" instrument as on the MSL -- for its element and mineralogy analysis, which required a big heavy setup of sampling drill and airlock to take a Venus sample actually inside the hull.  The new combination of NAGRS-LIBS-Raman should get much the same data with a much lighterweight and less vulnerable package of equipment.





 

Resources:

SAGE Proposal: http://www.lpi.usra.edu/vexag/oct2009/presentations/espositoSAGE.pdf

LIBS/Raman instruments for Venus: http://www.lpi.usra.edu/vexag/oct2009/presentations/cleggRamanLIBS.pdf