Category:Asteroids

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The ability to work with tidally locked body will be developed in the future, but is not yet available.
 
The ability to work with tidally locked body will be developed in the future, but is not yet available.
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* Define the body type
 
* Define the body type
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  dv>krc(lat=12.,body="Pluto")
 
  dv>krc(lat=12.,body="Pluto")
 
  dv>
 
  dv>
 
Over 3,200 comets are supported
 
  
  
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  dv>
 
  dv>
  
A list of comets currently supported is provided here
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A list of comets currently supported is provided [[:http://krc.mars.asu.edu/images/8/85/Comet_Names.txt | here]]
  
Over 390,000 comets are supported
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Over 3,200  comets are supported
  
 
Make sure to turn off the atmosphere by setting PTOTAL=0.
 
Make sure to turn off the atmosphere by setting PTOTAL=0.
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<u>''Asteroids''</u> : bodytype="minor"
 
<u>''Asteroids''</u> : bodytype="minor"
  
A list of asteroids currently supported is provided here
 
 
Over 3200 comets are supported
 
 
Make sure to turn off the atmosphere by setting PTOTAL=0.
 
 
 
 
  dv> out=krc(lat=0.,body="Bennu",bodytype="minor",PTOTAL=0.)
 
  dv> out=krc(lat=0.,body="Bennu",bodytype="minor",PTOTAL=0.)
 
  dv>  
 
  dv>  
  
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A list of asteroids currently supported is provided [[:http://krc.mars.asu.edu/images/5/50/Asteroid_Names.txt | here]]
  
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Over 390,000 asteroids are supported
  
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Make sure to turn off the atmosphere by setting PTOTAL=0.
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TAURAT: Ratio of thermal to visible opacity of dust
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* Define subsurface density/conductivity/specific heat profiles
 
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DUSTA: Single scattering albedo of dust
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ARC2: Henyey-Greenstein asymmetry factor
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KRC assumes broadband atmospheric opacities, but the default values are given a specific wavelengths.
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'''1.''' ''VIS/9μm dust opacity ratio is ~2:1'' (M. Smith personal communication);
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'''2.''' ''9μm to broadband TIR ratio is 2.5:1'' (ratio of maximum and average values of the dust opacity spectrum from Bandfield and Smith, [2003], Figure 3);
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[[Image:Atm_parameters_Change.png|600px|Figure 3 from Bandfield and Smith (2003)]]
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Latest revision as of 16:46, 8 November 2016

[edit] Running KRC for Non-Tidally Locked Airless Bodies

KRC can predict surface and subsurface temperatures for asteroids, comets, or any non-tidally locked body.

The ability to work with tidally locked body will be developed in the future, but is not yet available.


  • Define the body type

Planets and Pluto : No need to define bodytype

Mercury(!!!), Venus, Earth, Mars, Jupiter(!!!), Saturn(!!!), Uranus(!!!), Neptune(!!!), and Pluto can be modeled. (!!!): tidally locked or no rocky surface

Make sure to adjust the atmospheric parameters !

dv>krc(lat=12.,body="Pluto")
dv>


Comets : bodytype="comet"

dv>krc(lat=12.,bodytype="comet",body="1P-Halley",PTOTAL=0.)
dv>

A list of comets currently supported is provided here

Over 3,200 comets are supported

Make sure to turn off the atmosphere by setting PTOTAL=0.


Asteroids : bodytype="minor"

dv> out=krc(lat=0.,body="Bennu",bodytype="minor",PTOTAL=0.)
dv> 

A list of asteroids currently supported is provided here

Over 390,000 asteroids are supported

Make sure to turn off the atmosphere by setting PTOTAL=0.


  • Define subsurface density/conductivity/specific heat profiles

DOCUMENT THIS SECTION

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