Tuesday, 27 September 2016

Still NASA won’t admit their Galileo team got Europa wrong, Richard Greenberg was right

  Press Release  NASA's Hubble spots possible water plumes erupting on Jupiter's moon Europa

It’s taken NASA years to admit that 100-km plumes seen in 2012 by a SWRI team (Hubble images, Lorenz Roth et al.) are probably water vapour emitted from an ocean below the outer ice crust. 

A new image below indicates H2O plumes in the 7 o'clock position.

Richard Greenberg long ago argued that NASA’s Galileo spacecraft images taken, 1995-2003, implied an ice shell thin enough (few km) to enable the ocean to penetrate the major cracks maintained by tidal flexing. But this contradicted the project’s assumption of a thick crust entombing a deep internal ocean, and Greenberg was ostracised by NASA’s team leaders.  The new announcement fails to acknowledge Greenberg as being correct, showing NASA maintains their feud with him for severe criticism of the ‘thick ice’ cabal in Unmasking Europa: The Search for Life on Jupiter's Ocean Moon.


The Astrobiology Mag review of Greenberg's book in 2008 by Michael Shirber presented the basic case admirably.


On the basis that water in the ocean would be pumped up and down in the inter-plate cracks though tidal stresses on the ice-plates, Greenberg predicted that some would burst out to the surface.  He proceeded to further predict that the cracks would provide a suitable environment for oceanic microbial and plant-life.  

A professor in the Lunar and Planetary Laboratory at the University of Arizona, Greenberg was one of the first to formulate how tidal forces could shape the geology on Jovian moons. He had the opportunity to test his ideas as a member of the imaging team on NASA’s Galileo spacecraft, which orbited Jupiter from 1995 to 2003, but the team leaders refused his inputs and ostracised him.

Thursday, 9 July 2015

Do micro-organisms explain features on comets?

So was the RAS’s provocative headline on the Press Release for our presentation on 6th July Icy structures and terrain in comet 67P.
    The thrust of the talk was that the comet appears more habitable for microorganisms than the Arctic and Antarctic regions, with its organic-rich surface warming in sunlight, shielding an icy environment below a protective crust which traps gases.  A second point linked the surface crust with particles from comets collected in the stratosphere.  These comprise consolidated aggregates as well as ‘fluffy’ smoke-like particles, both high in carbon.  The former could be identified with fragments of the surface crust - some of these studied in Cardiff University labs show embedded Si-rich fibres, unlike crystalline astrophysical silicates.  The fibres were suggested to be spines from terrestrial  ice diatoms (Miyake, EPSC 2013).

What of the refutation no-alien-life-on-philae-comet ? Stuart Clark ignored the substance, approving instead of Uwe Meierhenrich (co-investigator on Philae’s COSAC chemical analyser) telling him a comet’s black surface crust was a prediction made in 1986 by J. Mayo Greenberg (Nature 321, 385), who had modelled what would happen to naturally occurring organic molecules on the comet when they were struck by cosmic rays and light. “These explanations seem to be valid, also with regard to new data of the cometary Rosetta mission,” wrote Meierhenrich, though the chemistry is indecisive.

Hoyle & Wickramasinghe did publish the prediction of a black surface (Earth Moon Planets 36, 289) before Greenberg in 1986.  Significantly, the Vega/Giotto missions to comet Halley proved Greenberg’s "bird’s nest" structure of rod-particles and UV-processed condensates on mineral cores to be wrong. The PIA and PUMA dust analysers found carbonaceous (CHON) particles, mineral particles and mixed ones.  The carbonaceous CHON component is highly complex, more than the UV-induced compounds of Greenberg’s experiments.  
   Cometary science needs to include past discoveries over comet Halley as well as newer ones on interplanetary dust particles.

Relevant papers in the RAS session Comets: Rosetta results and related science
Cometary dust properties measured by Rosetta GIADA:   Simon F. Green (OU) + GIADA Science Team.  GIADA has detected two distinct particle populations emitted from the nucleus: compact, 0.03-1 mm grains analogous to the processed mineral grains detected by Stardust, and ultra-low density fluffy aggregates of sub-micron grains with diameters 0.2-2.5 mm.

Comet nucleus surface properties in-situ, in the lab and on the computer: Axel Hagermann, DPS, The Open University

The picture of the physical nature of cometary nuclei has been changing dramatically since Giotto's encounter with 1P/Halley. The talk used information from laboratory experiments, computer models and in-situ measurements. The comet is rugged with firm surface and dark surface crust.  How is this compatible with low density?  Philae’s drill failed to penetrate when on low power (before shut down).  The OU group have repeated laboratory simulation of building up a dust-crust from a snow-dirt mix, as in the COSI experiments in the ’90s (Gruen et al).  Heat transport via vapour convection dominates over thermal convection when T>205K.  Fluffy snow converts to hard but porous ice under vapour transport, as modelled by Kossacki (Icarus 2015, applied to comet Tempel-1).  Thus, sintering of the snow-dirt mix increases the contact between ice grains with no change in porosity, so creating the firm and coherent surface crust. But the model contains mineral particles only, not the carbonaceous component which chemically degrades near the surface.

Wednesday, 8 July 2015

Storm over Life-on-Comets concept

TV - ITN report, Monday 6th July:  There could be life beneath the surface of the comet 67P/Churyumov-Gerasimenko according to two UK astronomers. Apparently the comet displays characteristics typical of an environment that could support alien life, including a black crust and icy lakes. Rosetta, the European Space Agency [ESA], spacecraft is also said to have picked up clusters of organic material that resemble viral particles.
## And two articles in The Guardian
  Neither Rosetta nor Philae are equipped to search for direct evidence of life after a proposal to include this in the mission was allegedly laughed out of court.

## Then the bloggers got busy:
"This morning, several news outlets gave voice to an extraordinary claim... But extraordinary claims, we all know, require extraordinary evidence. So guess what these morning’s claims were lacking!"

## Storm over the Concept, not the Content
What the paper at the RAS meeting concluded from considering various indications of ice below the dark crust is that the comet would be more hospitable to microorganisms (terrestrial, not 'alien' ones) than the Arctic and Antarctic; I added to this previously-published stratospheric microdust particles which can now be identified with fragments of such a comet’s crust. Surely rather mild claims! 
   The critics attack Press Reports of the RAS press release in their popular, exaggerated language, rather than consider the RAS Abstract and published work linked to it (previous post).  Why such a reaction from people who call themselves scientists, who should be concerned with the concept and evidence, even if poorly presented?  Why do critics use debating strategies and extravagant language, quite non-scientifically ?
  •    The hoary old saying about extraordinary claims requiring extraordinary evidence is repeated, yet the evidence comprises some ignored as not fitting mainstream theories and some from samples studied in Cardiff University labs.  The evidence is extraordinary only in the way it’s put together.  No-one was concerned about stratospheric dust containing siliceous fibres until identified as extraterrestrial with silicious spines of diatoms embedded in the matrix.  No-one was really concerned until the tentative identification of microdust particles as bits of cometary crust such as found on comet CG.
  •    No surprise that galaxy-astrophysicist Jillian Scudder failed to recognise potentially “extraordinary evidence”.
  •    The ESA project’s Matt Taylor declares “pure speculation”, yet he’s well aware of the published work and well aware that Rosetta studies have confirmed our concept of a cometary crust of carbonaceous-mineral aggregate. He saw our evidence of comet-like particles containing bio-fibres.  Is he bound by ESA’s decision against seeking evidence of extraterrestrial life (first Guardian article) ?
  •    Sarah Hörst says her research horizon is the ‘origin of life on Earth’.  Have discoveries of the hardiness of microorganisms carried on meteorites from Mars and space passed her by?  Perhaps she's unaware of panspermia studies, showing that viable spores (and DNA) can spread between planets and, on some arguments, spread to the interstellar dust that contributes to new planetary systems?
  •    Monika Grady is well aware of this as a meteoriticist, so she comments more moderately: “highly unlikely”. We await her argument  for saying our stratospheric dust particles are unlikely to come from a comet and/or unlikely to be representative of comet CG’s crust.

Why such unscientific reactions?  Life on other planets and planetary systems is largely accepted amongst the public.  Spores travelling within meteorites to nearby comets and planets are known to potentially survive.  Only the scientific establishment declares panspermia is “extraordinary”, sticking to the old life-began-on-Earth paradigm for the various sociological reasons given by Thomas Kuhn (Structure of Scientific Revolutions).    

Tuesday, 19 May 2015

Rosetta Images of Comet 67P/Churyumov–Gerasimenko: Icy structures and terrain

Presentation to Royal Astro Soc. National Astronomy Meeting session on Comets/Rosetta Mission, 6thJuly 2015.  
Publicised by the RAS at 

Icy structures and terrain in comet 67P

Max Wallis and N. Chandra Wickramasinghe


Despite the comet’s very black crust, Rosetta’s remarkable images show several indicators of an underlying icy morphology. Comet  67P displays smooth, planar ‘seas’ (the largest 600m X 800m) and flat-bottomed craters, both features seen also on comet Tempel-1.  Comet 67P’s surface is peppered with mega-boulders (10-70km) like comet Hartley-2, while parallel furrowed terrain appears as a new ice feature.  The largest sea (‘Cheops’ Sea, 600 X 800m) curves around one lobe of the 4km diameter comet, and the crater lakes extending  to ~150m across are re-frozen bodies of water overlain with organic-rich debris (sublimation lag) of order 10 cm.  The parallel furrows relate to flexing of the asymmetric and spinning two-lobe body, which generates fractures in an underlying body of ice. The mega-boulders are hypothesised to arise from bolide impacts into ice.  In the very low gravity, boulders ejected at a fraction of 1m/s would readily reach ~100m from the impact crater and could land perched on elevated surfaces.  Where they stand proud, they indicate stronger refrozen terrain or show that the surface they land on (and crush) sublimates more quickly.  Outgassing was already evident in September at 3.3AU, with surface temperature peaks of 220-230K, which implies loosely bound H2O and/or unconsolidated organic mixtures.   Increasing rates of gassing as Rosetta follows comet 67P around its 1.3 AU perihelion will hopefully reveal the activation of possible micro-organisms as well as the nature and prevalence of near-surface ices.

Wallis MK, Wickramasinghe NC (2015) Rosetta Images of Comet 67P/Churyumov–Gerasimenko: Inferences from Its Terrain and Structure. Astrobiol Outreach 3: 127. doi:10.4172/2332-2519.1000127  Open Access
Parallel paper:
Wickramasinghe NC, Wainwright M, Smith WE, Tokoro G, Al Mufti S, et al. (2015) Rosetta Studies of Comet 67P/Churyumov–Gerasimenko: Prospects for Establishing Cometary Biology. Astrobiol Outreach 3: 126. doi:10.4172/2332-2519.1000126 Open Access

David S. McKay 1936-2013 memorial tribute

Pioneer on martian meteorite biomorphs => Life-on-Mars 
To a large number in the scientific community, David McKay is best known as being the point person in the Allan Hills 84001 (ALH84001) Life on Mars hypothesis.  David was the lead author of the 1996 Science manuscript which jarred the scientific community into reexamining our concepts about life on Mars.  The paper was a team effort lead by David, Everett Gibson and Kathie Thomas-Keprta.  The three team leaders and all of the other members of the team (Christopher Romanek, Hojatollah Vali, Simon J. Clemett, Xavier D.F. Chillier, Claud R. Maechling and Richard Zare) contributed to the hypothesis.

The chain of evidence presented in the McKay et al. (1996) manuscript was believed to be compatible with the existence of past life on Mars: (i) an igneous Mars rock from  (age around 4 to 4.5 Ga) which had been penetrated by a low-temperature fluid along fractures and pore spaces, which then became the sites for secondary mineral formations and possible biogenic activity; (ii) a formation age for the carbonate globules (~3.9 Ga) younger than the age of the igneous rock; (iii) SEM and TEM images of carbonate globules and features resembling terrestrial microorganisms, terrestrial biogenic carbonate structures, or microfossils; (iv) magnetite and iron sulfide particles that could have resulted from oxidation and reduction reactions known to be important in terrestrial microbial systems; and (v) the presence of organic molecules associated with the carbonate globules. None of these observations is in itself conclusive for the existence of past life.  Although there are alternative explanations for each of these phenomena taken individually, when they are considered collectively, particularly in view of their spatial association, it provided evidence for primitive life on early Mars (McKay et al., 1996).  This paper has become one of the most heavily cited papers in planetary science.  With continued research, the team remains convinced their evidence is solid and the best interpretation to explain these data is that biogenic processes operated on early Mars.

 McKay et al. (1996) Search for past life on Mars: Possible relic biogenic activity in Martian meteorite ALH84001, Science 273, 924-930.
 McKay D.S., Thomas-Keprta K.L., Clemett S.J., Gibson E.K. Jr., Spencer L. and Wentworth S.J. (2009),  Life on Mars: New evidence from Martian meteorites.  Proc. of SPI,, Instruments and Methods for Astrobiology and Planetary Missions XII, Vol. 7441, 744102-1 to 733102-20 edited by R.B. Hoover, G.V. Levin, A.Y. Rozanov and K.D. Retherford.  , San Diego, CA.

from Memorial tribute prepared by:
Everett K. Gibson, Kathie Thomas-Keprta, Simon Clemett and Penny Morris-Smith
Astromaterials Research Office, NASA Johnson Space Center

Published:  June 2013 issue of Astrobiology 

Wednesday, 20 June 2012

An open-minded journalist against a panspermia-denier

The UK's Daily Telegraph on 19 June gave a full page sceptical about life originating in primordial soup “an alien concoction” which discusses panspermia with Chandra Wickramasinghe and Lewis Dartnell of UCL.

Science journalist Tom Chivers sees that the hardiness of micro-organisms – extremeophiles - to space survival and space travel gives substance to the idea of panspermia. Yet his questioning of Dr Lewis Dartnell revealed a panspermia-denier who requires a demonstration that ”terrestrial life isn’t native” before he will consider it.

Dartnell “simply can’t” see life survival on seed-bearing rocks and stones dispatched from Earth to other planetary systems, which arrive at hypervelocity and smash up on landing. But Dr. Dartnell should be aware as a UK astrobiologist that we solved this 'delivery' problem in 2004 (MNRAS 348, 52-61) by considering erosive sputtering in the dust-rich pre-planetary nebula. In this way, the Earth is likely to seed embryonic exoplanets.

The UK astrobiology specialist in hypervelocity collisions Mark Burchell in 2010 wrote Why Do Some People Reject Panspermia? as an open-minded riposte to the UK mainstream panspermia-deniers.

Friday, 11 May 2012

Carbon structures found in Tissint meteorite from Mars

Part of the newly-arrived Tissint meteorite is currently being studied by the Cardiff group led by Professor Chandra Wickramasinghe with doctoral student Jamie Wallis. The preliminary study reporting carbon structures in the meteorite is published in the current issue of the Journal of Cosmology.

Several carbon/oxygen-rich 10-20m particles have been found within the meteorite, embedded in the porous rocky matrix. The egg-shaped globule pictured shows cracking of the gold coating used for electron microscopy (SEM) due to heating by the electron beam. The working presumption is that these carbonaceous particles were accumulated among largely mineral dust by martian winds, potentially remnants of polysaccharide shells surrounding algal type cells.

The Tissint meteorite was recovered from the Moroccan desert in many pieces soon after it impacted last July.  It belongs to the type of meteorites originating from Mars classed as olivine-phyric shergottites.  The new finding supports David McKay's case for 'biomorphs' as traces of micro-life (including putative fossils) in certain other martian meteorites.