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guajiro [1.7K]
3 years ago
7

12. Taking the age of Earth to be about 4×10^9 years and assuming its orbital radius of 1.5 ×10^11 m has not changed and is circ

ular, calculate the approximate total distance Earth has traveled since its birth (in a frame of reference stationary with respect to the Sun).

Physics
2 answers:
lana66690 [7]3 years ago
7 0

The approximate total distance Earth has traveled since its birth is 3.8×10²¹m.

The Earth moves in a circular orbit of radius <em>r</em> around the Sun and it takes 1 year to go once around the Sun. Thus in a year it travels a distance equal to <em>2πr, </em>which is the circumference of the Earth's orbit.

Therefore in <em>n</em> years that have elapsed, it would travel a distance <em>d</em> given by,

d=2\pi rn

Substitute 3.14 for <em>π, </em>1.5×10¹¹m for <em>r</em> and 4×10⁹ for n.

d=2\pi rn\\= 2(3.14)(1.5*10^1^1m)(4*10^9)\\ =3.768*10^2^1m=3.8*10^2^1m

Thus, the approximate total distance Earth has traveled since its birth is 3.8×10²¹m.

DaniilM [7]3 years ago
7 0

The approximate total distance Earth has traveled since its birth is about:

3.8 × 10²¹ m

\texttt{ }

<h3>Further explanation</h3>

Angular Speed can be formulated as follows:

\large {\boxed {\omega = \frac{ v } { R } }

<em>ω = Angular Speed ( rad/s² )</em>

<em>v = Tangential Speed of Particle ( m/s )</em>

<em>R = Radius of Circular Motion ( m )</em>

\texttt{ }

Linear Speed can be formulated as follows:

\large {\boxed {v = \frac{ 2 \pi R } { T } }

<em>T = Period of Circular Motion ( s )</em>

<em>v = Tangential Speed of Particle ( m/s )</em>

<em>R = Radius of Circular Motion ( m )</em>

Let us now tackle the problem !

\texttt{ }

<u>Given:</u>

total time taken = t = 4 × 10⁹ years

period of Earth's revolution = T = 1 year

orbital radius = R = 1.5 × 10¹¹ m

<u>Asked:</u>

total distance = d = ?

<u>Solution:</u>

<em>We will use following formula to solve this problem:</em>

\texttt{Total Distance = Number of Revolutions } \times \texttt{ Circumference of Earth's Orbit}

d = N \times ( 2 \pi R )

d = \frac{t}{T} \times ( 2 \pi R )

d = \frac{4 \times 10^9}{1} \times { 2 \pi \times 1.5 \times 10^{11} }

d = 4 \times 10^9 \times 2 \pi \times 1.5 \times 10^{11}

d = 1.2 \pi \times 10^{21} \texttt{ m}

d \approx 3.8 \times 10^{21} \texttt{ m}

\texttt{ }

<h3>Learn more</h3>
  • Impacts of Gravity : brainly.com/question/5330244
  • Effect of Earth’s Gravity on Objects : brainly.com/question/8844454
  • The Acceleration Due To Gravity : brainly.com/question/4189441

\texttt{ }

<h3>Answer details</h3>

Grade: High School

Subject: Physics

Chapter: Circular Motion

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