Answer:
Seismology.
Explanation:
B 0.56 s
C 4.3s
D 70s
B 0.56 s is the time period of a twirlers baton.
Centripetal acceleration is defined as the property of the motion of an object which traversing a circular path.
Any object that is moving in a circle and has an acceleration vector pointed towards the center of that circle is known as Centripetal acceleration.
The centripetal acceleration is given by:
a = 4π²R/T²
Given values are:
a = 47.8 m/s²
D = 0.76 m so , R = 0.76/2 = 0.38m
Using this formula,
47.8*T² = 4π² x0.38
T² =
T = 0.56 s
Therefore,
A twirlers baton is 0.76 m long and spins around its center. The end of the baton has a centripetal acceleration of 47.8 m/s2 which have time period of 0.56 s.
Learn more about Centripetal acceleration here:
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.
Answer:
C. 4.3 seconds
Explanation:
Answer:
Heat flux = (598.3î + 204.3j) W/m²
a) Magnitude of the heat flux = 632.22 W/m²
b) Direction of the heat flux = 18.85°
Explanation:
- The correct question is the first image attached to this solution.
- The solution to this question is contained on the second and third images attached to this solution respectively.
Hope this Helps!!!
Answer:
Use proportions to find the scale of the first photo, then use that scale and other given information to fill in the equation
S=f/(H-h)
Where:
S = scale of the photo
f = focal length of the camera (in feet)
H = flying height
h = average elevation
The magnifying power of an astronomical telescope will be:
"0.095".
According to the question,
Radius of curvature, R = 5.5 mm
Focal length of eyepiece, = 2.9 cm
We know that,
→ Focal length of mirror,
F₀ =
By substituting the values,
=
= 2.75 mm or,
= 0.278 cm
hence,
The telescope's magnification be:
=
=
= 0.095
Thus the above approach is correct.
Find out more information about magnification here:
Answer:
0.095
Explanation:
An astronomical telescope is a telescope used for viewing far distance object. It uses two lenses called the objective lens and the eyepiece lens.
Each lens has its own focal length
Let the focal length of the objective lens be Fo
Focal length of the eyepiece be Fe
Magnification of an astronomical telescope = Fo/Fe
Since the telescope uses a reflecting mirror having radius of curvature of 5.5mm instead of an objective lens, then we will replace Fo as the focal length of the mirror.
Focal length of a mirror Fo = Radius of curvature/2
Fo = R/2
Fo = 5.5/2
Fo = 2.75mm
Converting 2.75mm to cm gives 2.75/10 = 0.275cm
Fo = 0.275cm; Fe = 2.9cm
Magnification of the telescope = 0.275/2.9
Magnification of the astronomical telescope = 0.095
3. Thu Tran, another Physics 2A student, grabs the ball and kicks it straight up to Hoai Nguyen, who is still up on the building rooftop. Assuming that the ball is kicked at 0.50 m above the ground and it goes on a vertical path, what is the minimum velocity required for the ball to make it to the building rooftop? Ignore air resistance. (Hint: the ball will pass the rooftop level with a higher speed...)
Answer:
1. 53.415 m
2. 32.373 m/s
3. 30.82 m/s
Explanation:
Let g = 9.81 m/s2. We can use the following equation of motion to calculate the distance traveled by the ball in 3.3s, and the velocity it achieved
1.
2.
3. If the ball is kicked at 0.5 m above the ground then the net distance between the ball and the roof top is
53.415 - 0.5 = 48.415 m
For the ball to at least make it to the roof top at speed v = 0 m/s. We can use the following equation of motion to calculate the minimum initial speed
where v = 0 m/s is the final velocity of the ball when it reaches the rooftop, is the initial velocity, is the distance traveled, g = -9.81 is the gravitational acceleration with direction opposite with velocity