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avanturin [10]
3 years ago
6

A Person whose weight is 5.20 x 10^2 N is being pulledup

Physics
1 answer:
Gnoma [55]3 years ago
6 0

Answer:

Explanation:

Given

Weight of Person W=5.20\times 10^{2} N

Cave is h=35.1 m deep

Breaking stress T=569 N

Net Force on Person

F_{net}=569-520=49 N

a_{net}=\frac{F_{net}}{\frac{W}{g}}

a_{net}=\frac{49}{\frac{520}{9.8}}

a_{net}=0.923 m/s^2

The shortest time such that the person can be taken out of cave

h=ut+\frac{1}{2}at^2

where

h=distance moved

t=time

a=acceleration

35.1=0+\frac{1}{2}(0.923)(t)^2

t^2=76.05

t=\sqrt{76.05}

t=8.72\ s                    

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Answer: frequency is 20000hz

Explanation:

Velocity=340m/s

Wavelength=0.017m

Frequency=velocity ➗ wavelength

Frequency=340 ➗ 0.017

Frequency=20000hz

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3 years ago
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What are (a) the charge and (b) the charge density on the surface of a conducting sphere of radius 0.12 m whose potential is 230
slamgirl [31]

Answer:

(a) q=3.07 nC

(b) σ=17 nC/m²

Explanation:

Given data

Radius r=0.12m

Potential V=230 V

To find

(a) Charge q

(b) Charge density σ

Solution

For Part (a)

As we know that potential is:

V_{potential}=k_{constat}\frac{q_{charge}}{r_{radius}} \\\\q_{charge}=\frac{V_{potential*r_{radius}}}{k_{constant}}

Substitute the given values

q_{charge}=\frac{(0.12m)(230V)}{9*10^{9} }\\ q_{charge}=3.07*10^{-9}C\\or\\q_{charge}=3.07nC

For Part (b)

The charge density is given by:

σ=q/(4πr²)

Substitute the given values and value of q to find charge density

So

=\frac{3.07*10^{-9}C}{4\pi (0.12m)^2}\\ =1.69*10^{-8}C/m^2\\or\\=17nC/m^2

σ=17 nC/m²

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3 years ago
What is the relationship between distance, time and acceleration
Evgesh-ka [11]

Answer:

total distance travelled

Explanation:

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4 years ago
When on object’s spectral lines are shifted from their rest wavelengths to longer wavelengths, we say that the object’s spectrum
neonofarm [45]

Answer:

Both statements are true.

Explanation:

When a celestial object (stars, galaxies) is moving away from an observer its spectral lines¹ will be shifted to the red part of the spectrum² (longer wavelength), in the other hand if the celestial body is moving toward the observer, the spectral lines will be shifted to the blue part of the spectrum (shorter wavelength). That is known as the Doppler shift.

This Doppler shift can be explained with the Doppler Effect³, which is defined for the case of light as:    

\frac{\Delta \lambda}{\lambda_{0}} = \frac{v}{c}    (1)

Where \Delta \lambda is the wavelength shift, \lambda_{0} is the rest wavelength, v is the velocity of the source and c is the speed of light.

This redshift in distant galaxies is a strong evidence for the expansion of the universe. Equation 1 also allows the measurement of radial velocity from celestial objects.  

Summary:  

Blueshift:

\lambda

Redshift:

\lambda >\lambda_{0}

¹Spectral lines: Determines the presence of particular elements in the photosphere of an star.

²Spectrum: Decomposition of light in its characteristic colors (wavelengths).

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4 0
4 years ago
What best accounts for the periodic trends seen in ionization energy?
NeX [460]

Answer:

Atomic size

Explanation:

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  • By and large, components on the right side of the periodic table have a higher ionization vitality in light of the fact that their valence shell is almost filled.
  • Components on the left half of the periodic table have low ionization energies as a result of their readiness to lose electrons and become cations.  
  • Another factor that influences ionization vitality is electron protecting. Electron protecting portrays the capacity of a molecule's internal electrons to shield its decidedly charged core from its valence electrons.
  • When moving to one side of a period, the quantity of electrons increments and the quality of protecting increments.
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  • The ionization energy of the components inside a period for the most part increments from left to right. This is because of valence shell security.  
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