LINE OF SIGHT ON SURFACE OF SUN
INTRODUCTION
Sun is a star which is
in the center of our solar system that has a mean radius of 695,700 km.
Although the equatorial radius is not equal to its polar radius, we can
approximate the Sun as a sphere. Any object on the surface of sphere has a
finite view due to the curvature of the sphere. Thus any one can view only up
to a finite distance before the horizon. The horizon is itself defined on the
height of the object, the greater the height the more the view. In this
article, we intend to determine the line of sight for an average human being on
the surface of Sun assuming that he can withstand extreme temperature and
gravity conditions.
ASSUMPTIONS
1. The
surface of Sun is smooth
2. Sun
is a homogeneous sphere
3. The
atmosphere is clear and vision is not obscured
4. Light
does not undergo diffraction and refraction
5. Space
time around Sun is not curved but flat
6. The
observer is at ground level
CALCULATION
From Figure .1,
R – Radius of Sun [m]
R = 695,700 Km = 695,700,000
m (Eq. 1)
h – Height of the
observer [m]
h = 5 feet
= 1.5 m (Eq.
2)
{⸪ 1 feet = 0.3 m}
d – Observable distance
by observer [m]
We can apply
Pythagorean Theorem,
d2 = (R+h)2
– R2 (Eq. 3)
d2 = 2Rh + h2
d = √ (2Rh+h2)
(Eq. 4)
Now substitute
equations (1), (2) in equation (4)
d = √ (2*695700000*1.5+1.52)
d = 45,684.7896 m
d
= 45.6847 Km = [28.3701 miles]
This is the distance
that can be viewed by an observer on the surface of Sun provided there aren't any solar storms to obscure the vision.
CONCLUSION
We thus determined the
line of sight or field of view for an observer on the surface of Sun.
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