Bunuel
Most known exoplanets lie too far from Earth to be observed directly and must instead be identified using indirect detection methods, such as measuring starlight distortions or subtle gravitational wobbles. However, these methods can generate reliable signal data only if the planet’s host star emits light in stable and consistent patterns over time. Therefore, few exoplanets are likely to produce detectable signals that can be consistently detected unless they are close enough to Earth to be observed directly.
The conclusion above follows logically if which of the following is assumed?
A. Indirect detection methods are less reliable than direct observation when gathering data about planetary atmospheres.
B. There are no alternative methods of detecting reliable signal data from exoplanets other than through shifts in starlight distortions or gravitational wobbles
C. Reliable interpretation of signal-related data depends more on the characteristics of the host star than on the exoplanet itself.
D. Exoplanets orbiting stars with consistent emission patterns are less common than those orbiting stars with inconsistent emissions.
E. Some exoplanets orbit stars with stable emissions but still fail to produce reliably detectable signals.
The exoplanets remain too far from the Earth, and there is no possibility of direct observation. So, Is there a possibility of identify the Exoplanet ? But, the exoplanet can be measured using 1. Starlight Distortion and 2. Subtle Gravitational Wobble.
Are these measurements reliable ?? Yes. But, ONLY when the planets HOST STAR emit light in Stable consistent pattern over time. So, the conclusion is ONLY few exoplanets are likely to produce detectable signals ( Consistent Detection).
The conclusion remains logical when we assume which of the following options :
A. Indirect detection methods are less reliable than direct observation when gathering data about planetary atmospheres.
There is no where a comparison between direct observation and indirect detection. So this cannot be an assumption.
B. There are no alternative methods of detecting reliable signal data from exoplanets other than through shifts in starlight distortions or gravitational wobbles. If there are no alternative methods to detect reliable signal data from exoplanets except through the two methods mentioned. So, only through the signals which we detect via host stars in exoplanets. The conclusion logically flows, only if there are NO alternative methods to detect reliable signal, suppose if there are alternative ways to detect signals then the need for indirect dectection seems irrelevant to the question.
C. Reliable interpretation of signal-related data depends more on the characteristics of the host star than on the exoplanet itself.
This is clearly mentioned in the question stem, which cannot be assumed. Hence, eliminating it.
D. Exoplanets orbiting stars with consistent emission patterns are less common than those orbiting stars with inconsistent emissions.
If the exoplanet orbiting stars emitting consistent patterns are less compared to inconsistent emission patterns, this assumption cannot be used to arrive at the conclusion logically. Hence eliminating it.
E. Some exoplanets orbit stars with stable emissions but still fail to produce reliably detectable signals.
If stable stars fail to emit detectable signals, then The conclusion doesn’t hold good. Hence wrong.
Option B