Skip to main content

The Physics Behind Carnival Rides

The Physics Behind Carnival Rides

Image result for the paratrooper ride





A ride known as "The Paratrooper" is a must have at every carnival. The Paratrooper is, as pictured below, the ride that sends its riders spinning through the air. The Paratrooper often has 10 seats that stem out from its center at consistent angle intervals, forming a circle. These seats are supported by arms connected to the center of the ride. When the ride starts, the machine lifts the seats and their occupants high into the air and begins rotating, slowly amassing speed until it reaches its maximum velocity. At this point, the machine begins to tilt so that its riders are no longer perpendicular with the ground. 

Understandably, this ride causes great thrill for those that ride it. However, what many of these riders fail to realize and appreciate are the aspects of physics that occur during this ride and enable it to be the ride that it is. During the short half a minute to minute ride, riders experience centrifugal force and gravitational pull, as well as the ride's velocity and acceleration.


On July 31, 1979 at a Canadian amusement park, one of these rides malfunctioned and a seat came loose, sending it and its occupants flying through the air. With the assumption that, at its maximum speed, the ride is spinning at 20 miles per hour, and that the riders were 10.668 meters in the air at the time that their seat came loose, how far did they travel through the air. Moreover, if the length of one of the ride's arms is 5.33 meters long, how much centrifugal force are the riders experiencing?

A rider of the Paratrooper experiences a centrifugal force of 14.995 m/s^2. Moreover, at the spend of 20 miles per hour, those unfortunate riders would have traveled through the air, 13.1865 meters away.

Work:
20 mph = 32186.9 meters per hour
32186.9 / 3600 = 8.94 meters per second

Ac = V^2 / r
Ac = 8.94^2 / 5.33 
Ac = 14.995 m/s^2

delta(y) = Vi(t) + 1/2At^2
-10.668 = 0(t) + 1/2(-9.8)t^2
-10.668 = -4.9t^2
-10.668 / -4.9 t^2
2.177 = t^2
t = 1.475 seconds 

delta(x) = V(t)
delta(x) = 8.94(1.475)
delta(x) = 13.1865 meters


Comments

Popular posts from this blog

Physics of Black Holes...Or Lack Thereof

Isabella Jacavone To comprehend how the universe works, we must dwell into the most basic building blocks of existence; matter, energy, space, and time. NASA's  Physics of the Cosmos program involves cosmology, astrophysics, and fundamental physics intended to answer questions about the elusiveness of complex concepts such as black holes, neutron stars, dark energy, and gravitational waves. In this blog post, I'd like to elaborate on a subject that is very intriguing  to me; Black holes. And more specifically, what would happen if we got near one. A black hole is anything but a hole, but rather an immense amount of matter compacted into an extremely small area. A black hole is caused when, hypothetically, a star four times more massive than our sun collapses into a sphere no bigger than 600 square km. To put that in perspective, that's about the size of New York City. B lack holes were predicted by Einstein's theory of general relativity, which showed that when a...

The Physics of Spiderman

Over this past weekend after I finished working on my homework, I decided to relax and watch a few movies before going asleep. Among the movies I watched was Spider-Man 3 from 2007 and despite the movie flaws I was interested by the scenes that showed Spider Man shooting through the sky with the use of his webs that come out of his wrists. Due to this, I decided to make my blog post about the physics of Spider-Man's slingshot. After doing some research, I discovered just how much information there is on the physics of Spider-Man and how elements of Spider-Man can be used as examples for most topics learned in mechanics. For this investigation, I will not be using the horrible cliche and terrible CGI infested mess that Spider-Man 3 is but instead the all around superior Spider-Man movie of Spider-Man 2 to investigate the physics of Spider-Man's web propelled slingshot.  I want to talk about what happens in terms of physics when Spider-Man launches himself across a dista...

2017 Physics Nobel Prize - Capturing Gravitational Waves

 2017 Physics Nobel Prize - Capturing Gravitational Waves Gravitational Waves Captured by LIGO Who?  Rainer Weiss, Barry C. Barish, and Kip S. Thorne - LIGO/VIRGO Collarboration What?  Observation of gravitational waves for the first time using LIGO (Laser Interferometer Gravitational-Wave Observatory. Where?  Two locations in the US - Hanford and Livingston. (See figure 1) Figure 1: LIGO in the US When?  14 September 2015 HOW?  The scientists captured gravitational waves by using an interferometer. The LIGO interferometer is a more glamorous interferometer than the original Michelson interferometer. It works through using light waves to measure gravitational interference (i.e. waves). First, one needs to understand the parts of an interferometer. The LIGO interferometer (and most) is shaped as an L. It has two 4 km vacuum tunnel arms with a mirror at each end. At the center of the arms, there is a beam splitter. Th...