CAN LIGHT ESCAPE FROM THE SUN?

Not in my ill-conceived and erroneous calculation:

[1]Chandrasekhar,
"An Introduction To the Study Of Stellar Structure"

p487    MASS of Sun = 1.985 x 10**33 gm

[2]Abell, "Exploration of the Universe"

p704    RADIUS of Sun = 6.960 * 10**10 cm

[3]Bate, Mueller and White  "Fundamentals of Astrodynamics"

p35     ESCAPE SPEED = (2GM/r)**(1/2)

p4      G = 6.670 x 10**-8  dyne cm x cm/ (gm x gm)

[4]Sears, Zemansky "University Physics" Part 1

p662    c = 3 x 10 ** 4  m/sec

[5]Sears, Zemansky "University Physics" Part 1

p80     dyne = gm * cm / (sec * sec)
p462    dyne = 2.247*10-6 lb.

Q: WHEN IS THE ESCAPE SPEED EQUAL TO c (THE SPEED OF LIGHT)
A:
            ESCAPE SPEED = (2GM/r)**(1/2)                              [3]

            c**2 = 2GM / distance from star center 

            distance from star center when speed of light escapes

                 =  (2GM) / c**2

                 =  2 * 6.667 * 10**-8 sec*sec*dyne*cm*cm * M /        [3]
                      (9 * 10**8) m*m  gm*gm                           [4]
                  
                 =  2 * 6.667 * 10**-8 sec*sec*dyne*cm*cm * M /
                     (9 * 10**8) m*m  gm*gm * 10*4 cm/m * cm/m 
                   
                 =  2 * 6.667 * 10**-8 sec*sec*(gm*cm/sec/sec)*cm*cm * M /
                     (9 * 10**12) cm*cm  gm*gm                         [5]
                 =  2 * 6.667  cm * M /
                     (9 * 10**20)   gm 

                 =  1.48  * 10**-20 cm/gm * M

                 =  1.48  * 10**-20  cm/gm *  1.985 * 10**33  Sun g    [1]

                 =  2.940 * 10**13  cm (for one Sun mass )

    Sun radius   =  6.960 * 10**10  cm                                 [2]
  
    distance / Sun radius ratio = 422 times number of Sun Masses

    distance of lost horizon = 422 * k sun mass(es) * radius of sun in cm
                             = 422 * Ksuns * Rsun cm
                    
    Since I believe light does escape from the sun, k = 1 can't be true
    or we would not see the sun.    
    The high density (mass per volume) of the neutron star must be
    considered along with all the relativistic effects.