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MartyMurray

I have some issues with your reasoning of Question 2 Option B.

Quote:
So, contrary to what this choice says, the visible light part of the spectrum does not constitute the full range of frequencies that can penetrate Earth's atmosphere.

visible light does constitute the full range of frequencies that can penetrate Earth's atmosphere. Because "constitute" means "to be a part of" and not "whole of".
"Constitutes" means "to form or make up something" or "to be or be considered."

That other definition, "be (a part) of a whole," that appears on Google seems to me to be erroneous.

Quote:
So, option B really says that visible light is a part of the full range of frequencies that can penetrate Earth's atmosphere. Which is true according to the passage.
"Constitutes the full range" means "makes up the full range."

Quote:
Quote:
One reason we see the frequencies we do is that visible-spectrum light generally passes through our atmosphere without being absorbed or reflected.

So, the Full Range of frequencies is really Visible Light + Some Other Frequencies (because a majority (not all) gets reflected/absorbed).

I think the real issue with Option B is that if Option B were true, we should have been able to see those other frequencies, which the passage states that we don't.

Thoughts ?
Given the correct definition of "constitutes," choice (B) doesn't mean what you thought it meant. So, the choice works as I explained that it does.
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Light exists on a spectrum of frequencies extending from gamma rays at the highest frequencies to radio waves at the lowest, though human eyes are sensitive to only a narrow range of frequencies in the middle known as the visible spectrum. The different colors we see correspond to the different frequencies of light within that range. Given that there are so many frequencies of light, one might wonder why our eyes didn't evolve to be sensitive to more frequencies.

Gamma rays from space collide with Earth's atmosphere, which converts some of their energy to heat and creates a distinctive cascade of subatomic particles down toward the ground. However, the rays themselves are entirely absorbed before they can reach Earth's surface. Thus, Earth would appear to be pitch black to eyes that were only sensitive to gamma rays. Similarly, the majority of frequencies of light that are higher or lower than those in the visible spectrum-such as ultraviolet and most infrared frequencies, respectively-are mostly or entirely absorbed by Earth's atmosphere.

One reason we see the frequencies we do is that visible-spectrum light generally passes through our atmosphere without being absorbed or reflected. Another reason is that the Sun, in some respects an average star, emits most of its light at frequencies in the visible spectrum, whereas a hot star emits most of its light at ultraviolet frequencies and a very cool star emits most of its light at infrared frequencies. Indeed, to remarkably high precision, the human eye is most sensitive to the exact frequency in the yellow part of the spectrum at which the Sun is the brightest.

Even if there are living beings on other planets, it is not likely that they would see mainly at very different frequencies than we do. Virtually all gases that are abundant in the cosmos tend to allow frequencies in the visible spectrum to pass through while absorbing other frequencies, and all but the coolest stars put out much, if not most, of their light in the visible spectrum. If there are living beings on other planets, they probably see at roughly the same frequencies as we do, though there may be occasional exceptions.

1. The main purpose of the passage is to

A. present certain facts about the cosmos that indicate probable limits to the frequencies of light that living beings would be able to see
B. explain why certain frequencies of light outside the visible spectrum are not abundant in the cosmos
C. discuss the manner in which various forms of matter are affected by interaction with different frequencies of light
D. describe why average stars tend to emit more light at visible-spectrum frequencies than they do at other frequencies
E. discuss whether the temperature of the closest star to a planet affects the frequencies of light that living beings on that planet could potentially evolve to see


2. According to the passage, humans evolved eyes sensitive to a particular part of the spectrum of light in part because

A. Earth's atmosphere filters out most of the light emitted by the Sun
B. that part of the spectrum constitutes the full range of frequencies that can penetrate Earth's atmosphere
C. Earth is primarily composed of materials that do not absorb light in that part of the spectrum
D. the majority of the Sun's light is emitted at frequencies in that part of the spectrum
E. most other frequencies of light are reflected by Earth's atmosphere


3. Which of the following most accurately describes the purpose of the highlighted sentence in relation to the passage as a whole?

A. To indicate the author's surprise at the manner in which human eyes have developed in relation to the visible spectrum of light
B. To illustrate that the correspondence between human eyes' sensitivity and the frequencies of light comprising the visible spectrum is not merely coincidental
C. To assert that human eyes are more finely tuned to a particular part of the visible spectrum of light than are those of some other organisms on Earth
D. To explain why the gases that comprise Earth's atmosphere do not absorb the frequencies of light that the Sun emits most abundantly
E. To support the claim that the Sun is an average star with respect to the frequencies of light at which it is brightest


4. The reasoning in the final paragraph most strongly implies that the author makes which of the following assumptions?

A. The vast majority of the planets in the cosmos have atmospheres.
B. Living beings that evolve on planets orbiting hot stars are more likely to develop the capacity to see than are living beings that evolve on planets orbiting average-temperature stars.
C. Living beings are most likely to evolve on planets with atmospheres containing gases that are abundant in the cosmos.
D. If living beings evolve on planets orbiting the hottest stars, they will likely develop eyes that are sensitive to gamma rays.
E. The frequencies of light that pass through a planet's atmosphere without being absorbed are the frequencies that the nearest star emits most abundantly.


Responding to a pm:

Para 1: Light has frequencies from gamma to infra red. Why can't our eyes see all?
Para 2: Gamma and other non visible spectrum does not reach us
Para 3: Why we see what we see - Only visible spectrum reaches us and Sum emits most in visible spectrum
Para 4: Other beings on other planets are also likely to see visible spectrum only.


Question 1.

1. The main purpose of the passage is to

A. present certain facts about the cosmos that indicate probable limits to the frequencies of light that living beings would be able to see
B. explain why certain frequencies of light outside the visible spectrum are not abundant in the cosmos
C. discuss the manner in which various forms of matter are affected by interaction with different frequencies of light
D. describe why average stars tend to emit more light at visible-spectrum frequencies than they do at other frequencies
E. discuss whether the temperature of the closest star to a planet affects the frequencies of light that living beings on that planet could potentially evolve to see

Option (A) covers all the paragraphs. The passage starts with why we only see the visible spectrum and ends with why others would also likely see only the visible spectrum. Hence it discusses certain facts about the cosmos that indicate probable limits to the frequencies of light that living beings would be able to see.
The whole passage is about what living beings can see and options (B), (C) and (D) do not mention it at all.
Option (E) focuses on one aspect - whether temperature of a star affects the frequencies living beings can see. But that is just one aspect of our discussion.

Answer (A)


Question 2.

2. According to the passage, humans evolved eyes sensitive to a particular part of the spectrum of light in part because

A. Earth's atmosphere filters out most of the light emitted by the Sun
B. that part of the spectrum constitutes the full range of frequencies that can penetrate Earth's atmosphere
C. Earth is primarily composed of materials that do not absorb light in that part of the spectrum
D. the majority of the Sun's light is emitted at frequencies in that part of the spectrum
E. most other frequencies of light are reflected by Earth's atmosphere

Answer would be found in para 2 and 3 which discuss the reasons.

A. Earth's atmosphere filters out most of the light emitted by the Sun

Not correct. We are given that Sun emits most of its light at frequencies in the visible spectrum (which is not filtered out).

B. that part of the spectrum constitutes the full range of frequencies that can penetrate Earth's atmosphere

Given:
the majority of frequencies of light that are higher or lower than those in the visible spectrum-such as ultraviolet and most infrared frequencies, respectively-are mostly or entirely absorbed by Earth's atmosphere.
Hence this option is not correct. The passage says that "majority" of other frequencies are mostly absorbed, not ALL. Hence the visible spectrum is not the FULL range of frequencies that can penetrate Earth's atmosphere.

C. Earth is primarily composed of materials that do not absorb light in that part of the spectrum

Composition of Earth is not discussed. Composition of the atmosphere (what stands between us and the light) is discussed.

D. the majority of the Sun's light is emitted at frequencies in that part of the spectrum

Correct. Given:
Another reason is that the Sun, in some respects an average star, emits most of its light at frequencies in the visible spectrum.

E. most other frequencies of light are reflected by Earth's atmosphere

Not reflected, absorbed.
Given:
Similarly, the majority of frequencies of light that are higher or lower than those in the visible spectrum-such as ultraviolet and most infrared frequencies, respectively-are mostly or entirely absorbed by Earth's atmosphere.


Answer (D)


Question 3.

3. Which of the following most accurately describes the purpose of the highlighted sentence in relation to the passage as a whole?

A. To indicate the author's surprise at the manner in which human eyes have developed in relation to the visible spectrum of light
B. To illustrate that the correspondence between human eyes' sensitivity and the frequencies of light comprising the visible spectrum is not merely coincidental
C. To assert that human eyes are more finely tuned to a particular part of the visible spectrum of light than are those of some other organisms on Earth
D. To explain why the gases that comprise Earth's atmosphere do not absorb the frequencies of light that the Sun emits most abundantly
E. To support the claim that the Sun is an average star with respect to the frequencies of light at which it is brightest


Given: Another reason is that the Sun, in some respects an average star, emits most of its light at frequencies in the visible spectrum, whereas a hot star emits most of its light at ultraviolet frequencies and a very cool star emits most of its light at infrared frequencies. Indeed, to remarkably high precision, the human eye is most sensitive to the exact frequency in the yellow part of the spectrum at which the Sun is the brightest.

With the highlighted sentence, the author is establishing the correspondence of the sensitivity of our eyes to a certain frequency with the amount of light the Sun emits at that frequency. The highlighted sentence shows that we are most sensitive to the frequency which is emitted the most (and hence makes the Sun appear brightest).
Hence option (B) works.

Answer (B)


Question 4.

4. The reasoning in the final paragraph most strongly implies that the author makes which of the following assumptions?

A. The vast majority of the planets in the cosmos have atmospheres.
B. Living beings that evolve on planets orbiting hot stars are more likely to develop the capacity to see than are living beings that evolve on planets orbiting average-temperature stars.
C. Living beings are most likely to evolve on planets with atmospheres containing gases that are abundant in the cosmos.
D. If living beings evolve on planets orbiting the hottest stars, they will likely develop eyes that are sensitive to gamma rays.
E. The frequencies of light that pass through a planet's atmosphere without being absorbed are the frequencies that the nearest star emits most abundantly.

Given:
Virtually all gases that are abundant in the cosmos tend to allow frequencies in the visible spectrum to pass through while absorbing other frequencies, and all but the coolest stars put out much, if not most, of their light in the visible spectrum. If there are living beings on other planets, they probably see at roughly the same frequencies as we do, though there may be occasional exceptions.

The author concludes that beings on other planets probably see at roughly the same frequencies as we do based on the characteristics of the gases that are abundant in the cosmos. So she assumes that the atmospheres of planets where living beings have evolved are likely to contain gases that are abundant in the cosmos. Hence option (C) makes sense.

Note that option (A) is incorrect because the author does not conclude about the vast majority of planets. She concludes only about the planets with living beings.

Answer (C)
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