There is only one part to this question and I need to know the impacts. Thank you!! **Problem Statement:**If you stood on Earth during its formation, during which it captured about \(2.1 \times 10^{11}\) particles per second, and watched a region covering \(260 \, \text{m}^2\), how many impacts would you expect to see in an hour? *(Notes: The surface area of a sphere is \(4\pi r^2\). Hint: Assume that Earth had its current radius of 6,378 km.)***Input Box:**[ ] impacts**Detailed Explanation:**To solve the problem, you need to calculate the number of particle impacts on a specified area over a given time. 1. **Calculate the Total Surface Area of the Earth:** - The formula for the surface area of a sphere is \(4\pi r^2\). - Given the radius \(r = 6,378 \, \text{km}\), convert it to meters for consistency: \(r = 6,378,000 \, \text{m}\). - Substitute the value: \( \text{Surface Area} = 4\pi (6,378,000 \, \text{m})^2\).2. **Determine Impacts Per Second:** - Total particles captured per second by the Earth = \(2.1 \times 10^{11}\).3. **Calculate the Impacts for the Selected Area:** - Find the proportion of impacts for \(260 \, \text{m}^2\) by using the ratio of the selected area to the total surface area. - \( \frac{260 \, \text{m}^2}{\text{Surface Area of Earth}} \times (2.1 \times 10^{11}) = \text{Impacts per second on 260} \, \text{m}^2\).4. **Calculate the Expected Impacts in an Hour:** - Multiply the impacts per second by the number of seconds in an hour (3600 seconds) to find the total impacts in one hour.Putting these steps together, you can determine the expected number of impacts.

Given, N=2.1×1011 s-1A=260m2Re=6378 km

Answered: If you stood on Earth during its…

Similar questions

When NASA new horizons found that Plutos moon Charon orbits Pluto every 7.9 days at an average distance of 20900.0 km. What is the combined mass (in kg) of Pluto and Charon?
Which of these has not been suggested as a method to possibly deflect an asteroid from hitting Earth? O Using its own gravity to "tow" it. O Hitting it with explosions or impacts to push it. O Painting it. O Using rockets to push it. O All of these are possible methods to deflect an asteroid.
‘The angular diameter of a body was 0.35 degrees and at a distance of 160 million kilmmeters, then what is the diameter of the TR
Galileo is often credited with the early discovery of four of Jupiters many moons.The moons orbiting Jupiter follow te same laws of motion as the planets orbiting the sun.One of the moons is called Io - its distance from Jupiter's center is 4.2 units and it orbits Jupiter in 1.8 Earth-days.Another moon is caled Ganymede;it is 10.7 units from Jupiters center. Make a prediction of the period of Ganymede using Keplers law of periods.
An asteroid orbits the Sun with semi- major axis = 10 AU and eccentricity e = %3D %3D 0.6. Calculate the ratio of the maximum to the minimum amount of energy it receives from the Sun per second during its orbit. Select one: а. 8 O b. 64 О с. 2 O d. 16 е. 4
15. An object is dropped above the surface of planet Nexus and falls 11.2 meters in 2.4 seconds. What is the mass of the planet Nexus ? (assume: I the radius of the plane Nexus is 3.45-100 meters and G = Nm²/kg, initial velocity of the object is 0 m/s) 6.670-10-¹1 16. An object is launched at a velocity of 33 m/s in a direction making an angle 34° upward with the horizontal. What is the total flight time of the object? (assume g 9.81 m/s²)
2. A comet is traveling in outer space with a velocity of 2000 m/s. How long will it take to travel 300,000 meters? 2000 s 0.0006 s 6,000,000 s 150 s
19.
What’s the objects mass?
If earth starts revolving with more speed then normal , what happens??
4 Hello, I have questions about the physics, can you please help me with your diagram and explanation? I am highly appreciate it and thank you very much! In 1843, a comet passed extremely close to the sun, mass Ms: its distance from the perihelion was d = 6.1*10^3 * a0, where a0 is the radius of the Earth's orbit. Accurate measurements showed that the eccentricity of the comet was e=1-x with x = 9.4*10^-5. Given u = 30 km/s is the speed of revolution of the Earth around the Sun. (a) Express the product GMs as a function of u and a0. (b) Considering that the trajectory of the comet is quasi-parabolic, calculate its speed of passage vp at the perihelion. (c) Deduce the speed Va of transition to aphelion as a function of Vp and x. Do the digital application. (d) In what year will this comet return to the solar system?
Why do Moon travellers tie heavy weight on their backs before landing on the Moon?

SEE MORE QUESTIONS