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Complex	
  organic	
  ma/er	
  delivery	
  
by	
  carbonate-­‐rich	
  meteorites:	
  
kine:c	
  models	
  
Savino	
  Longo	
  
Chemistry	
  Department,	
  UniBa	
  
Nanotec-­‐CNR,	
  INAF-­‐Arcetri	
  
savino.longo@nanotec.cnr.it	
  
Shock	
  bow	
  
Compression	
  zone	
   Direc:on	
  of	
  mo:on	
  
Trail	
  
Villa	
  M.,	
  Montanari	
  E.,	
  Meteore	
  e	
  meteori),	
  Astromedia	
  2001	
  
Trajectory	
  and	
  thermal	
  model	
  	
  
simplest	
  version	
  –	
  plane	
  parallel	
  atmosphere	
  
•  v(t),	
  h(t),	
  T(t)	
  and	
  m(t)	
  
	
  
	
  
	

	

Colapinto	
  M.	
  M.Sc.	
  Thesis,	
  University	
  of	
  Bari	
  2012	
  
Trajectory	
  and	
  thermal	
  model	
  	
  
simplest	
  version	
  –	
  plane	
  parallel	
  atmosphere	
  
Grain	
  temperature	
  vs.	
  :me	
  
Test	
  case:	
  1	
  ng	
  Fe.	
  
45°	
  entry,	
  20	
  km/s	
  
t=0	
  at	
  150	
  km	
  
Colapinto	
  M.	
  M.Sc.	
  Thesis,	
  University	
  of	
  Bari	
  2012	
  
Bisceglia	
  E,	
  Micca	
  Longo	
  G,	
  Longo	
  S,	
  Thermal	
  decomposi:on	
  rate	
  of	
  MgCO3	
  as	
  an	
  inorganic	
  
astrobiological	
  matrix	
  in	
  meteors,	
  Interna)onal	
  Journal	
  of	
  Astrobiology	
  in	
  press	
  (2016)	
  
Idea:	
  chemical	
  thermal	
  protec:on	
  of	
  a	
  carbonate	
  grain	
  a`er	
  exposure	
  
(high-­‐al:tude	
  mechanical	
  fragmenta:on	
  of	
  a	
  larger	
  body)	
  
	
  
Ra:onale:	
  much	
  energy	
  is	
  absorbed	
  by	
  MCO3	
  decomposi:on	
  
	
  
	
   	
   	
  MCO3	
  	
  MO	
  +	
  CO2	
  	
   	
   	
  at	
  rela:vely	
  low	
  T	
  
	
  
The	
  2	
  kinds	
  of	
  TPS:	
  
	
  
1)  Radia:ve	
  
2)  Abla:ve	
  
	
   	
   	
   	
  	
  
Abla:ve/Radia:ve	
  cooling	
  of	
  silicates	
  	
  <<	
  1	
  for	
  T	
  <	
  1200°	
  (Opik)	
  
	
  
The	
  3	
  kinds	
  of	
  TPS	
  in	
  astrochemistry	
  according	
  to	
  our	
  proposal:	
  
	
  
1)  Radia:ve	
  
2)  Abla:ve	
  	
  
3)  Chemical	
  	
  (effec:ve	
  in	
  vacuum	
  at	
  T	
  as	
  low	
  as	
  a	
  few	
  100°s	
  )	
  
	
  We	
  checked	
  MgCO3	
  as	
  a	
  test	
  mineral	
  for	
  first	
  calcula:ons	
  
Ja	
  
MgCO3	
  	
  MgO	
  +	
  CO2	
  	
  
Calcula:ng	
  the	
  molecular	
  ouhlux	
  using	
  kine:c	
  theory	
  (Langmuir	
  Law)	
  
NIST	
  thermochemical	
  
data	
  for	
  MgCO3,	
  MgO	
  
and	
  CO2	
  
Power	
  dissipated	
  per	
  unit	
  surface	
  
by	
  thermal	
  decomposi:on	
  
	
   	
   	
   	
  	
  
Pdec (Tsurf ) = J
!H
NA
~ vthe"!G/RT !H
4RT
Power	
  dissipated	
  per	
  unit	
  surface	
  
by	
  thermal	
  radia:on	
  
	
  
	
   	
   	
   	
  	
  
Prad (Tsurf ) =!SB!Tsurf
4
DNA	
  dry	
  thermal	
  
decomposi:on	
  	
  
	
  ~	
  190°	
  	
  
	
  
Karni,	
  Moshe,	
  et	
  al.	
  
"Thermal	
  degrada:on	
  of	
  
DNA."	
  DNA	
  and	
  cell	
  
biology	
  32.6	
  (2013):	
  
298-­‐301.	
  
1mm	
  oxide	
  
STONE	
  atmospheric	
  entry	
  tests*	
  
Foucher,	
  F	
  et	
  al.	
  Tes:ng	
  the	
  survival	
  of	
  microfossils	
  in	
  ar:ficial	
  mar:an	
  sedimentary	
  meteorites	
  during	
  
entry	
  into	
  Earth's	
  atmosphere:	
  the	
  STONE	
  6	
  experiment,	
  Icarus,	
  207	
  (2009)	
  616	
  
Ki/y's	
  Gap	
  Chert	
  sediment	
  sample	
  
Conclusion:	
  magnesium-­‐rich	
  carbona:c	
  globules	
  may	
  offer	
  much	
  
be/er	
  thermal	
  protec:on	
  to	
  complex	
  organic	
  species	
  than	
  typical	
  
meteor	
  ma/er,	
  thanks	
  to	
  facile	
  decomposi:on	
  reac:ons.	
  
	
  
Evapora:on	
  rate	
  model:	
  Bisceglia	
  E,	
  Micca	
  Longo	
  G,	
  Longo	
  S,	
  Interna)onal	
  
Journal	
  of	
  Astrobiology	
  in	
  press	
  (2016)	
  
	
  
Test	
  of	
  the	
  concept	
  in	
  context	
  by	
  an	
  integrated	
  entry	
  model:	
  in	
  prepara)on	
  
	
  
Other	
  composi:ons	
  (including	
  Fe2+)	
  &	
  solid	
  state	
  diffusion:	
  future	
  work	
  
Collaborators	
  
	
  
Enrico	
  Bisceglia,	
  Master	
  student,	
  Paris	
  Nord	
  -­‐	
  Bari	
  
Gaia	
  Micca	
  Longo,	
  PhD	
  student,	
  Bari	
  University	
  
	
  
Thank	
  you	
  for	
  kind	
  a/en:on	
  

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Firenze

  • 1. Complex  organic  ma/er  delivery   by  carbonate-­‐rich  meteorites:   kine:c  models   Savino  Longo   Chemistry  Department,  UniBa   Nanotec-­‐CNR,  INAF-­‐Arcetri   savino.longo@nanotec.cnr.it  
  • 2. Shock  bow   Compression  zone   Direc:on  of  mo:on   Trail   Villa  M.,  Montanari  E.,  Meteore  e  meteori),  Astromedia  2001  
  • 3. Trajectory  and  thermal  model     simplest  version  –  plane  parallel  atmosphere   •  v(t),  h(t),  T(t)  and  m(t)       Colapinto  M.  M.Sc.  Thesis,  University  of  Bari  2012  
  • 4. Trajectory  and  thermal  model     simplest  version  –  plane  parallel  atmosphere   Grain  temperature  vs.  :me   Test  case:  1  ng  Fe.   45°  entry,  20  km/s   t=0  at  150  km   Colapinto  M.  M.Sc.  Thesis,  University  of  Bari  2012  
  • 5. Bisceglia  E,  Micca  Longo  G,  Longo  S,  Thermal  decomposi:on  rate  of  MgCO3  as  an  inorganic   astrobiological  matrix  in  meteors,  Interna)onal  Journal  of  Astrobiology  in  press  (2016)  
  • 6. Idea:  chemical  thermal  protec:on  of  a  carbonate  grain  a`er  exposure   (high-­‐al:tude  mechanical  fragmenta:on  of  a  larger  body)     Ra:onale:  much  energy  is  absorbed  by  MCO3  decomposi:on          MCO3    MO  +  CO2        at  rela:vely  low  T     The  2  kinds  of  TPS:     1)  Radia:ve   2)  Abla:ve             Abla:ve/Radia:ve  cooling  of  silicates    <<  1  for  T  <  1200°  (Opik)     The  3  kinds  of  TPS  in  astrochemistry  according  to  our  proposal:     1)  Radia:ve   2)  Abla:ve     3)  Chemical    (effec:ve  in  vacuum  at  T  as  low  as  a  few  100°s  )  
  • 7.   We  checked  MgCO3  as  a  test  mineral  for  first  calcula:ons  
  • 8. Ja   MgCO3    MgO  +  CO2     Calcula:ng  the  molecular  ouhlux  using  kine:c  theory  (Langmuir  Law)   NIST  thermochemical   data  for  MgCO3,  MgO   and  CO2  
  • 9. Power  dissipated  per  unit  surface   by  thermal  decomposi:on             Pdec (Tsurf ) = J !H NA ~ vthe"!G/RT !H 4RT Power  dissipated  per  unit  surface   by  thermal  radia:on               Prad (Tsurf ) =!SB!Tsurf 4 DNA  dry  thermal   decomposi:on      ~  190°       Karni,  Moshe,  et  al.   "Thermal  degrada:on  of   DNA."  DNA  and  cell   biology  32.6  (2013):   298-­‐301.  
  • 10. 1mm  oxide   STONE  atmospheric  entry  tests*   Foucher,  F  et  al.  Tes:ng  the  survival  of  microfossils  in  ar:ficial  mar:an  sedimentary  meteorites  during   entry  into  Earth's  atmosphere:  the  STONE  6  experiment,  Icarus,  207  (2009)  616   Ki/y's  Gap  Chert  sediment  sample  
  • 11. Conclusion:  magnesium-­‐rich  carbona:c  globules  may  offer  much   be/er  thermal  protec:on  to  complex  organic  species  than  typical   meteor  ma/er,  thanks  to  facile  decomposi:on  reac:ons.     Evapora:on  rate  model:  Bisceglia  E,  Micca  Longo  G,  Longo  S,  Interna)onal   Journal  of  Astrobiology  in  press  (2016)     Test  of  the  concept  in  context  by  an  integrated  entry  model:  in  prepara)on     Other  composi:ons  (including  Fe2+)  &  solid  state  diffusion:  future  work   Collaborators     Enrico  Bisceglia,  Master  student,  Paris  Nord  -­‐  Bari   Gaia  Micca  Longo,  PhD  student,  Bari  University     Thank  you  for  kind  a/en:on