Date       : June 7, 2020              
    Writer      : B.Engr.  Koji Makino            
    Review    : June 10, 2023              
                       
                Calculations for Velocities and Sound Velocities of      
            Tukuba Meteorite and  Calculations for Temperatures of     
                        the Meteorite by Aerodynamic Heating       
                       
       (When horizontal movement velocity is 1097.4m/s, 747.9m/s was added to vertical direction 
    velocity to fall to height 13000m above the ground in lapse of 90 seconds as starting to fall 
    from height of 120km.  It rushed to atmosphrere at angle of 15°of east side from the north.  
    The direction shifted to 20°east side by the power of the earth rotation.  The meteorite falling  
    down route crossed at angle of  35°to the north-south line.  "g" is gravity acceleration 
    9.8m/s2.)  The meteorite entered atmosphere, and then changed the direction by the earth 
    rotation. The meteorite started to fall from altitude of 120km after that.       
    It is a calculating formula which asks for the temperature of the flight body by which   
    aerodynamic heating is done by sound velocity.           
    Tah = Rac × r × Tab × Vs2 - 273          
    Tah : Aerodynamic Heating Temperature  Rac : Air Concentration Ratio  r : Form Coefficient
    Tab : Absolute Temperature  Vs : Velocity of Sound           
    Absolute Temperature(Tab)was 273 degree as celsius 0 degree.        
    Aerodynamic heating temperature was calculated on absolute temperature.        
    For it converted to celsius, -273 degree was added to upper formula.      
    The meteorite was warmed by the solar heat, so it was not -273℃ really.      
    Sound velocity in high altitude is slower than aboveground, since it changes in each altitudes.
    All sound velocity are calculated with 330m/s as average velocity.        
                       
     Table 1. calculated proceeding direction sound velocities and aerodynamic
           heating temperatures at elapse time every 5 seconds      
                       
  Elapse Vertical Horizontal Proceeding Proceeding Height a- Ratio of air Coeffi- Aerodyna- Visual ob-
  time direction direction direction direction bove ground concent- cient mic heating servation
    velocity velocity velocity sound start to fall ration to of form tempe-  flying
    V=g×t 1097.4   velocity from height that on r = 1 rature object
    +747.9       120km the ground     color ・
  (s) (m/s) (m/s) (m/s) (Mach) (m) (%)   (℃) state
  0 747.9 1097.4 1328.0 4.02 120000.0 0.00 1 -273.0 G., W.C.
  5 796.9 1097.4 1356.2 4.11 116138.0 0.00 1 -273.0 G., W.C.
  10 845.9 1097.4 1385.6 4.20 112031.0 0.00 1 -273.0 G., W.C.
  15 894.9 1097.4 1416.0 4.29 107679.0 0.00 1 -273.0 G., W.C.
  20 943.9 1097.4 1447.5 4.39 103082.0 0.00 1 -273.0 G., W.C.
  25 992.9 1097.4 1479.9 4.48 98240.0 0.00 1 -273.0 G., W.C.
  30 1041.9 1097.4 1513.2 4.59 93153.0 0.00 1 -273.0 G., W.C.
  35 1090.9 1097.4 1547.4 4.69 87821.0 0.00 1 -273.0 G., W.C.
  40 1139.9 1097.4 1582.3 4.79 82244.0 0.00 1 -273.0 G., W.C.
  45 1188.9 1097.4 1618.0 4.90 76422.0 0.00 1 -273.0 G., W.C.
  50 1237.9 1097.4 1654.3 5.01 70355.0 0.00 1 -273.0 G., W.C.
  55 1286.9 1097.4 1691.3 5.13 64043.0 0.01 1 -272.3 G., W.C.
  60 1335.9 1097.4 1728.8 5.24 57486.0 0.03 1 -270.8 G., W.C.
  65 1384.9 1097.4 1767.0 5.35 50684.0 0.07 1 -267.5 G., W.C.
  70 1433.9 1097.4 1805.6 5.47 43637.0 0.17 1 -259.1 G., W.C.
  75 1482.9 1097.4 1844.8 5.59 36345.0 0.46 1 -233.8 G., W.C.
  80 1531.9 1097.4 1884.4 5.71 28808.0 1.37 1 -151.0 G., W.C.
  85 1580.9 1097.4 1924.5 5.83 21026.0 4.54 1 148.5 G., W.C.
  90 1629.9 1097.4 1964.9 5.95 12999.0 16.2 1 1295.0 Bright White
    G., W.C. : Gray, White Cloud                
                       
                       
    Date       : June 7, 2020              
    Writer      : B.Engr.  Koji Makino            
    Review    : June 10, 2023              
                       
                       
        How to calculate about ratio of air concentration at the altitude to that on the ground 
    Atmospheric pressure at the altitude were corrected atmospheric pressure at the alititude     
    from data of JMA's Aerological observatory (at Tukuba) on the very day.      
    Ratio of air concentraion were calculated from atmospheric pressure at the altitude with
    that on the ground.   Atmospheric pressure were data from the ground to altitude of 33.4km by 
    the observatory. Atmospheric pressure were calculated by formula of U.S. standard atmosphere, 
    1976. over that altitude.              
                       
 
 
                   
       
       
       
       
       
       
       
       
       
       
       
       
       
       
       
       
       
       
       
                       
                       
                       
 
 
                   
                       
       
       
       
       
       
       
       
       
       
       
       
       
       
       
       
       
       
       
       
                       
                       
    Date      : June 7, 2020              
    Writer     : B.Engr.  Koji Makino              
    Review   : June 10, 2023              
                       
    The following table was drawn to confirm illuminant state every second.      
                       
     Table 2. calculated proceeding direction sound velocities and aerodynamic
           heating temperatures at elapse time from 85 second to 99 second
                       
  Elapse Vertical Horizontal Proceeding Proceeding Height a- Ratio of air Coeffi- Aerodyna- Visual ob-
  time direction direction direction direction bove ground concent- cient mic heating servation
    velocity velocity velocity sound start to fall ration to of form tempe-  flying
    V=g×t 1097.4   velocity from height that on r = 1 rature object
    +747.9       120km the ground     color ・
  (s) (m/s) (m/s) (m/s) (Mach) (m) (%)   (℃) state
  85 1580.9 1097.4 1924.5 5.83 21026.0 4.54 1 148.5 G., W.C.
  86 1590.7 1097.4 1932.5 5.86 19440.2 5.81 1 270.9 G., W.C.
  87 1600.5 1097.4 1940.6 5.88 17844.6 7.48 1 433.2 G., W.C.
  88 1610.3 1097.4 1948.7 5.91 16239.2 9.68 1 648.5 Light Pink
  89 1620.1 1097.4 1956.8 5.93 14624.0 12.6 1 931.7 Orenge
  90 1629.9 1097.4 1964.9 5.95 12999.0 16.2 1 1295.0 Bright White
  91 1639.7 1097.4 1973.0 5.98 11364.2 20.9 1 1761.8 Big Flash
  92 1649.5 1097.4 1981.2 6.00 9719.6 26.9 1 2374.9 Huge Flash
  93 1659.3 17800.0 17877.2 54.17 8065.2 34.6 0.02 5269.6 Y.W.P.
  94 1669.1 17800.0 17878.1 54.18 6401.0 44.0 0.02 6776.5 Y.W.P.
  95 800.0 1200.0 1442.2 4.37 5601.0 49.3 −− −−− P.B.
  96 600.0 600.0 848.5 2.57 5001.0 53.4 −− −−− M.S.D.
  97 400.0 400.0 565.7 1.71 4601.0 56.3 −− −−− E.A.M.S.D.
  98 300.0 300.0 424.3 1.29 4301.0 58.6 −− −−− H.T.M.S.
  99 150.0 200.0 250.0 0.76 4151.0 59.8 −− −−− H.T.M.S.
                       
      These velocitys are calculated  G., W.C.  : Gray, White Cloud      
      to divide moving distance in  Y.W.P.    : Yellow White Photosphere    
      2 seconds by time.     P.B.      : Photosphere Burst      
      Those velocitys are put to M.S.D.   : Molten Substance Diffussion  
      suitable value.   E.A.M.S.D.: Explosion After Molten Substance Diffusion
      Calculated height by observed   H.T.M.S. : High Temperature Meteorites Shower
      elevation angle at sighting site.            
      When it became a photosphere,           
      since it became the sphere fully,           
      that form factor becomes small.       June 10, 2023
                       
        How to determine the coefficient of form          
    The shape of flying object gives influence for aerodynamic heating.  It is determined   
    aerodynamic heating coefficient of form  r = 1 through trial and error because meteorite is 
    almost sphere.                
                       
        The molten substance continued to spread after photosphere bursting.  So the yellow
    white photosphere became early for 1second. Ratios of air concentration to that on the 
    ground were reviewed, those numerical values were revised.    August 2, 2021
                       
        When lapse time were from 90 second to 92 second, it became the huge flash fireball 
    and the velocity became 1.98km/s (Mach 6.0). The ice of the meteorite vapored in large 
    amounts, it became a huge black cloud. When lapse time were from 93 second to 94 second, 
    it became a photosphere and it flew with the velocity 17.9km/s (Mach 54.2).    
                  August 2, 2021
                       
                       
                       
    Date      : June 7, 2020              
    Writer     : B.Engr.  Koji Makino              
    Review   : June 10, 2023              
                       
                       
        The confirmation with the actual temperature has not been performed about      
    calculative numerical values with aerodynamic heating temperatures from 93 second   
    to 94 second at the lapse time. Till 92 second, it is confirmed from the relation     
    between luminescent color and temperature above the ground.    August 2, 2021
                       
        When the temperature inside a photosphere exceeds 2862 ℃, the ferrum of an  
    interiority substance becomes gas and it will vapor. Since the interiority substance of   
    the photosphere turned into a molten substance and the waterish viscosity was shown, 
    it was surmised that the bulk temperature of a photosphere was probably 2200 ℃.   
    Supposing the form factor was 1, since the temperature would be too high, it set the  
    form factor to 0.02. Probably, the surface temperature of a photosphere will be     
    from 5000℃ to 7000℃.          June 10, 2023
                       
 
 
                   
         
         
         
         
         
         
         
         
         
         
         
         
         
         
         
         
         
                       
                       
 
 
                   
           
           
           
           
           
           
           
           
           
           
           
           
           
           
           
           
           
           
                       
                       
                       
    Date       : June 7, 2020              
    Writer      : B.Engr.  Koji Makino            
    Review    : June 10, 2023              
                       
        the Verification about the Altitude of 120km where          
            the Meteorite Start to Fall from.  
    (It is verified by comparing calculated distances with measured distances    
      on route map at each illuminant state whether it is suitable that the height of meteorite 
      start to fall from 120km. )              
                       
    Table 1 : Table of doing decision that caluculated horizontal distances compare with   
                 measured distances on the route map at each illuminant state from point of 
                 meteorite starting to fall             
                       
    Calculation of the horizontal distance from point of  Verification  
    starting meteorite fall, the height and the illuminant state (Measurement on the route map)  
    Elapsed Horizontal Distance Height Calculat- Route map Route map Deci-  
    time from direction from   ed temp. point name measure. sion  
    starting p. velocity starting p. illuminant   distance (within 2%  
    (s) (m/s) (m) (m) state   (mm) of error)  
    88 1097.4 96571 16239.2 Light Pink Lumi. Start 96.5 Agree.  
    89 1097.4 97669 14624.0 Orenge        
    90 1097.4 98766 12999.0 Bright White Bright White 98.5 Agree.  
    91 1097.4 99863 11364.2 Big Flash ---- ---- ----  
    92 1097.4 100961 9719.6 Huge Flash Huge Flash 102 Agree.  
    93 17800 118761 8065.2 Y.W.Photo. ---- ---- ----  
    94 17800 136561 6401.0 Y.W.Photo. ---- ---- ----  
    95 1200 137761 5601.0 P.B. ---- ---- ----  
    96 600 138361 5001.0 M.S.D.  M.S.D.  138 Agree.  
    97 400 138761 4601.0 E.A.M.S.D.  ---- ---- ----  
    98 300 139061 4301.0 H.T.M.S. ---- ---- ----  
    99 200 139261 4151.0 H.T.M.S. ---- ---- ----  
    The route map is scale 1/1000000.            
    1mm on the route map correspond to 1km in real distance value.        
    starting p. : starting point of meteorite fall                   Lumi. Start : Luminous Start  
    Y.W.Photo. : Yellow White Photosphere                   P.B.          : Photosphere Burst
    M.S.D.      : Molten Substance Diffusion                   Agree.       : Agreement    
    E.A.M.S.D.   : Explosion After Molten Substance Diffusion        
    H.T.M.S.   : High Temperature Meteorites Shower          
    Agreement means that calculated distance is equal with measured distance on the route map.
                       
       Comparation with calculated horizontal distance and measured distance from 
       starting point of merteorite fall            
       This numeric value match up with calculated height from witnessed elevation angle.
                       
    The molten substance continued to spread after photosphere bursting.        
    So the yellow white photosphere became early for 1second and the molten substance diffusion
    time was added on the table 1.       August 2, 2021  
                       
    ※ In the case of falling from height of 120km,  the calculated value of the distance    
         were suitable well with the measured distance on the route map at each illuminant  
         state point from the starting point.             
                       
    It is judged that the meteorite starting to          
            fall from height of 120km is suitable.  
                       
              Transl. date : August 28, 2020  
              Translator   : B.Engr.  Koji Makino  
              Transl. rev.  : June 12, 2023