The apparent backward movement of a planet is called
a. kepler's first law of motion.
b. heliocentric motion.
c. eccentricity.
d. retrograde motion.

A).  Kepler's first law of planetary motion ... "Each planet moves
      in an elliptical orbit, with the Sun at one focus of the ellipse."

B).  Heliocentric motion ... motion in an orbit around the Sun.

C).  Eccentricity ... what makes an ellipse different from a circle.
       The eccentricity of a circle is zero.       
       The eccentricity of the Earth's orbit is very small.
       The eccentricity of a comet's orbit is big.

D).  Retrograde motion ... the apparent, temporary, backward
       motion of a planet on its path through the stars.

4.5 x 10¹⁴ Hz

666.7 nm

1.8 x 10⁵ J

The color of the emitted light is red

Explanation:

E = energy of photons of light = 2.961 x 10⁻¹⁹ J

f = frequency of the photon

Energy of photons is given as

E = h f

2.961 x 10⁻¹⁹ = (6.63 x 10⁻³⁴) f

f = 4.5 x 10¹⁴ Hz

c = speed of light = 3 x 10⁸ m/s

λ = wavelength of photon

Using the equation

c = f λ

3 x 10⁸ = (4.5 x 10¹⁴) λ

λ = 0.6667 x 10⁻⁶ m

λ = 666.7 x 10⁻⁹ m

λ = 666.7 nm

n = number of photons in 1 mole = 6.023 x 10²³

U = energy of 1 mole of photons

Energy of 1 mole of photons is given as

U = n E

U = (6.023 x 10²³) (2.961 x 10⁻¹⁹)

U = 1.8 x 10⁵ J

The color of the emitted light is red