Title: Exoplanetology
Content:  The temperature of an exoplanet can be estimated by measuring the intensity of the light it receives from its parent star. For example, the planet OGLE-2005-BLG-390Lb is estimated to have a surface temperature of roughly −220 °C (50 K). However, such estimates may be substantially in error because they depend on the planet's usually unknown albedo, and because factors such as the greenhouse effect may introduce unknown complications. A few planets have had their temperature measured by observing the variation in infrared radiation as the planet moves around in its orbit and is eclipsed by its parent star. For example, the planet HD 189733b has been estimated to have an average temperature of 1,205 K (932 °C) on its dayside and 973 K (700 °C) on its nightside.
Title: Habitable exoplanet
Content:  The temperature among the habitable exoplanets discovered so far are estimated to range from 182 Kelvin (Kepler 186f) to 285 Kelvin (Tau Ceti e).
Title: Gliese 436 b
Content:  The planet's surface temperature is estimated from measurements taken as it passes behind the star to be 712 K. This temperature is significantly higher than would be expected if the planet were only heated by radiation from its star, which was prior to this measurement, estimated at 520 K. Whatever energy tidal effects deliver to the planet, it does not affect its temperature significantly. A greenhouse effect would result in a much greater temperature than the predicted 520–620 K. In 2019, USA Today reported that the exoplanet's burning ice continued to have scientists "flabbergasted." Its main constituent was initially predicted to be hot "ice" in various exotic high-pressure forms, which would remain solid despite the high temperatures, because of 
Title: Earth analog
Content:  There are several factors that can determine planetary temperatures and therefore several measures that can draw comparisons to that of the Earth in planets where atmospheric conditions are unknown. Equilibrium temperature is used for planets without atmospheres. With atmosphere, a greenhouse effect is assumed. Finally, surface temperature is used. Each of these temperatures is affected by climate, which is influenced by the orbit and rotation (or tidal locking) of the planet, each of which introduces further variables. Below is a comparison of the confirmed planets with the closest known temperatures to Earth.
Title: Planetary equilibrium temperature
Content:  The planetary equilibrium temperature is a theoretical temperature that a planet would be a black body being heated only by its parent star. In this model, the presence or absence of an atmosphere (and therefore any greenhouse effect) is irrelevant, as the equilibrium temperature is calculated purely from a balance with incident stellar energy. Other authors use different names for this concept, such as equivalent blackbody temperature of a planet, or the effective radiation emission temperature of the planet. Planetary equilibrium temperature differs from the global mean temperature and surface air temperature, which are measured observationally by satellites or surface-based instruments, and may be warmer than an equilibrium temperature due to greenhouse effects.
Title: Kepler-42
Content:  to small size of the star, causing these planets to block a larger proportion of starlight during their transits. Not all of the orbital parameters of the system are known. For example, as with all transiting planets that have not had their properties established by means of other methods such as the radial velocity method, the orbital eccentricity remains unknown. Based on the orbits of the planets and the luminosity and effective temperature of the host star, the equilibrium temperatures of the planets can be calculated. Assuming an extremely high albedo of 0.9 and absence of greenhouse effect, the outer planet Kepler-42 d would have an equilibrium temperature of about 280 K, similar to Earth's 255 K. Estimates for the known planets are in the tables below:
Title: Planetary equilibrium temperature
Content:  The equilibrium temperature is neither an upper nor lower bound on actual temperatures on a planet. There are several reasons why measured temperatures deviate from predicted equilibrium temperatures.
Title: Climate of Mars
Content:  a low of about −153 C at the poles. Actual temperature measurements at the Viking landers' site range from −17.2 C to −107 C. The warmest soil temperature estimated by the Viking Orbiter was 27 C. The Spirit rover recorded a maximum daytime air temperature in the shade of 35 C, and regularly recorded temperatures well above 0 C, except in winter. It has been reported that "On the basis of the nighttime air temperature data, every northern spring and early northern summer yet observed were identical to within the level of experimental error (to within ±1 °C)" but that the "daytime data, however, suggests a somewhat different 
Title: HD 153950 b
Content:  The temperature of the exoplanet is likely to vary during its orbit, temperatures would likely range from 275–375 K as it approaches its periastron/apastron of its orbit. This would also likely apply to a potentially habitable hypothetical moon orbiting the gas giant exoplanet (see below).
Title: Super-Earth
Content:  Since the atmospheres, albedo and greenhouse effects of super-Earths are unknown, the surface temperatures are unknown and generally only an equilibrium temperature is given. For example, the black-body temperature of the Earth is 255.3 K (−18 °C or 0 °F ). It is the greenhouse gases that keep the Earth warmer. Venus has a black-body temperature of only 184.2 K (−89 °C or −128 °F ) even though Venus has a true temperature of 737 K (464 °C or 867 °F ). Though the atmosphere of Venus traps more heat than Earth's, NASA lists the black-body temperature of Venus based on the fact that Venus has an extremely high albedo (Bond albedo 0.90, Visual geometric albedo 0.67), giving it a lower black body temperature than the more absorbent (lower albedo) Earth.

Question: Verify the following claims with "True" or "False": planets have a mean temperature of 154 kelvins and a maximum temperature of 165 kelvins.
Answer: True