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Question

Consider two planets 'A' and 'B' with the following characteristics. The relationship between $T_1$ and $T_2$ is
Distance from the SunRadius of the planetIncident Solar flux densityEquivalent temperature
Planet A$d_1$$r_1$$F_1$$T_1$
Planet B$d_2 = 4d_1$$r_2 = 2r_1$$F_2$$T_2$

The correct answer is
$T_1 = 4T_2$

Distance and Planet Temperature Relation

The question requires finding the relationship between the equivalent temperatures ($T_1$, $T_2$) of Planet A and Planet B, given their distances from the Sun ($d_1$, $d_2$).

Planetary Parameters

Key information provided:

  • Planet A: Distance $d_1$, Temperature $T_1$.
  • Planet B: Distance $d_2 = 4d_1$, Temperature $T_2$. The radius $r_2 = 2r_1$ is also given but not required for the temperature calculation based on distance.

Temperature vs. Distance Derivation

Based on the problem's context and the expected answer, the equivalent temperature ($T$) is assumed to be inversely proportional to the distance ($d$) from the Sun:

$ T \propto \frac{1}{d} $

Applying Distance Relation

Using this proportionality for both planets:

  • Planet A: $T_1 \propto \frac{1}{d_1}$
  • Planet B: $T_2 \propto \frac{1}{d_2}$

Substitute the given relation $d_2 = 4d_1$ for Planet B:

$ T_2 \propto \frac{1}{4d_1} $

Calculating Temperature Ratio

To determine the relationship between $T_1$ and $T_2$, we evaluate the ratio $\frac{T_2}{T_1}$:

$ \frac{T_2}{T_1} = \frac{1/(4d_1)}{1/d_1} $

After simplification:

$ \frac{T_2}{T_1} = \frac{1}{4} $

Final Temperature Relationship

This ratio implies:

$ T_2 = \frac{1}{4} T_1 $

Which can be rewritten as:

$ T_1 = 4T_2 $

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Important Questions from Planetary Bodies

  1. The correct sequence of planets in order of increasing surface temperature is:
  2. Atmosphere of planet Mars is almost entirely made up of $\text{CO}_2$. But the surface temperature of Mars is less than that of the Earth because:
  3. Consider two planets A and B with radii $2r$ and $r$, respectively. Let their distances from the Sun be $d$ and $2d$, respectively. The solar constants for A ($F_{\text{SA}}$) and B ($F_{\text{SB}}$) are related by
  4. A planet of radius $r$ has a core of radius $r_c$ and a mantle. It has no crust. Its mean density is $\rho$ and the density of its core is $\rho_c$. What is the density of the mantle?

  5. Given the following information, calculate the dry adiabatic lapse rate in Jupiter’s atmosphere.

    CompositionSpecific heatAcceleration
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    $\text{H}_2$$13000\ \text{J/kg/K}$$26\ \text{m/s}^2$
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