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2 years ago

What is the value of x

Geography

2 answers:

levacccp [35]2 years ago

5 0

Answer:

since no numbers you will assume it is 1

Explanation:

AysviL [449]2 years ago

5 0

I don't know. What is the value of x? But if we are talking about geography than X equals the lines of longitude.

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A boundary between nonsedimentary and sedimentary rocks is an example of what type of unconfirmity

Degger [83]

Answer:

Non-conformity

Explanation:

An unconformity is a time gap or break in stratigraphic record of sedimentary rock layers. It is usually depicted by a period of non-deposition or erosion.

There are different types of unconformity:

>Disconformity

>Non-conformity

>Para-conformity

>Angular unconformity

Non-conformity is a type of unconformity marked by different rock types. The boundary between such rock types is an unconformity surface. For example, the boundary between an igneous rock that caps a sedimentary sequence is an unconformity.

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3 years ago

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Describe two ways demand for petroleum has been reduced.

tigry1 [53]

Answer:

The most striking feature of the oil market is the low price elasticity of demand.

The supply of oil is also fairly inelastic.

Oil price swings tend to be dramatic and often impact the rest of the economy.

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3 years ago

This photo shows ruins at Machu Picchu.

fredd [130]

The incas the built it

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3 years ago

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Imagine that you have obtained spectra for several galaxies and have measured the observed wavelength of a hydrogen emission lin

Lerok [7]

Answer:

A. z (galaxy 1) = -0.00515, z (galaxy 2) = -0.01707, z (galaxy 3) = -0.04008

B. v (galaxy 1) = -0.00517c, v (galaxy 2) = -0.01707c, v (galaxy 3) = -0.0401c

C. d (galaxy 1) = -21 Mpc,d (galaxy 2) = -69.4 Mpc, d (galaxy 3) = -163 Mpc

Explanation:

We begin by listing out the parameters we were given:

λ (obsv) = 656.3 nm, λ (emit 1) = 659.7 nm, λ (emit 2) = 667.7 nm,

λ (emit 3) = 683.7 nm

A) Using the Redshift formula, we have:

z = [λ (obsv) - λ (emit)] ÷ λ (emit)

For galaxy 1:

z = [λ (obsv) - λ (emit 1)] ÷ λ (emit 1)

z = (656.3 - 659.7) ÷ 659.7 = -0.00515

z = -0.00515

For galaxy 2:

z = [λ (obsv) - λ (emit 2)] ÷ λ (emit 2)

z = (656.3 - 667.7) ÷ 667.7 = -0.01707

z = -0.01707

For galaxy 3:

z = [λ (obsv) - λ (emit 3)] ÷ λ (emit 3)

z = (656.3 - 683.7) ÷ 683.7 = -0.04008

z = -0.04008

B) Using the Doppler formula, we have:

(Δλ ÷ λ) = v ÷ c

v = c * (Δλ ÷ λ)

but, z = (Δλ ÷ λ)

⇒ v = c * z

speed of light (c) = 3 x $10^{8}$ m/s

For galaxy 1:

v = c * z

Substitute z into the equation calculated from A) above

v = 3 x $10^{8}$ * (-0.00515)

v = -1.55 x $10^{6}$ m/s

v = -0.00517c

For galaxy 2:

v = c * z

Substitute z into the equation calculated from A) above

v = 3 x $10^{8}$ * (-0.01707)

v = -5.12 x $10^{6}$ m/s

v = -0.01707c

For galaxy 3:

v = c * z

Substitute z into the equation calculated from A) above

v = 3 x $10^{8}$ * (-0.04008)

v = -12.03 x $10^{6}$ m/s

v = -0.0401c

N.B: the negative value of velocity connotes that the galaxies are moving away from us (not towards us)

C) Using Hubbleʹs law, we have:

v = H · d

where:

v = velocity of a galaxy (km/s), d = distance (Mpc),

H = Hubble's constant (km/s/Mpc) = 73.8 km/sec

d = v ÷ H

We use the velocities calculated in B) above

For galaxy 1:

v = -1.55 x $10^{3}$ km/s

d = -1.55 x $10^{3}$ ÷ 73.8

d = -21 Mpc

For galaxy 2:

v = -5.12 x $10^{3}$ km/s

d = -5.12 x $10^{3}$ ÷ 73.8

d = -69.4 Mpc

For galaxy 3:

v = -12.03 x $10^{3}$ km/s

d = -12.03 x $10^{3}$ ÷ 73.8

d = -163 Mpc

N.B: distance cannot be a negative value

4 0

3 years ago

Based on the graph, what year would you estimate that the Cold War ended and why?

tigry1 [53]

Answer:

1991, because that is when the Soviet Union began producing fewer nuclear weapons.

Explanation:

OR C

5 0

3 years ago