FYI-018 · SCIENCE · Filed Sep 3, 2026
Why Is Venus Hotter Than Mercury? It Gets Less Sunlight
Why is Venus hotter than Mercury? Its clouds send over 75 percent of arriving sunlight straight back to space, and the surface still sits at 464C anyway.
Venus is wrapped in cloud, the cloud works like a blanket, the blanket holds in the Sun’s heat, and that is why the second planet from the Sun runs hotter than the first. Almost every explanation of Venus arrives at that sentence. The temperature at the end of it is right. The mechanism at the front of it is pointed the wrong way.
Venus’s clouds are sulfuric acid droplets, and sulfuric acid droplets are close to perfect scatterers of visible light. In a 2018 review of the Venus cloud system for Space Science Reviews, Dmitrij Titov and four co-authors put the effect in a single line: more than 75 percent of the incoming solar flux is returned back to space, and on average only about 3 percent of the sunlight arriving at the top of the atmosphere reaches the ground.
Which delivers the fact worth sitting with. Venus orbits 30 percent closer to the Sun than Earth and still takes in less solar energy than Earth does, because the cloud deck turns most of it around before it gets anywhere near the surface.
Why is Venus hotter than Mercury?
Venus is hotter than Mercury because Venus blocks heat on the way out rather than on the way in. Mercury has no atmosphere, so the sunlight its rock absorbs radiates straight back to space. Venus carries 92 bars of carbon dioxide that absorbs outgoing infrared, holding the surface near 464C against Mercury’s mean of 167C.
Mercury gets the sunlight and loses it every night
NASA places Mercury 0.4 astronomical units from the Sun and Venus at 0.72, so Mercury takes by far the harder beating. Its daytime surface reaches 430C. Its night side falls to about minus 180C, the same rock running from 800F in daylight to minus 290F after dark on NASA’s numbers.
Nothing there holds the heat. What passes for air on Mercury is an exosphere, a thin scatter of oxygen, sodium, hydrogen, helium and potassium atoms knocked off the rock by the solar wind and by meteoroid strikes. Sunlight lands, the ground warms, the ground radiates, and the energy leaves about as fast as it arrived.
| Measure | Mercury | Venus |
|---|---|---|
| Distance from the Sun | 0.4 AU | 0.72 AU |
| Atmosphere | thin exosphere of stray atoms | 96.5 percent carbon dioxide |
| Surface pressure | effectively none | about 92 bars |
| Mean surface temperature | 167C | 464C |
The clouds work as a mirror before they work as a blanket
The blanket picture was not invented out of nothing. Titov and his co-authors also record that sulfuric acid absorbs strongly at longer wavelengths, which makes the same clouds a strong greenhouse agent for thermal radiation beyond about 2.5 micrometres. Both descriptions are true at once, at different wavelengths.
What the popular version reverses is the order. The clouds meet sunlight first and reject three quarters of it, and only afterwards do they help hold in the infrared the surface gives off. Calling them a blanket names the second job and hides the first. Intuition about which way a mechanism runs gets flipped like this constantly, the same way a honeybee’s sting is a weapon that kills the bee using it.
Carbon dioxide blocks the exit
The 3 percent of sunlight that does reach the Venusian surface still has to leave, and it leaves as infrared. Above it sits an atmosphere that Stephen Kane and eleven co-authors, in a 2019 Journal of Geophysical Research review, describe as 92 bars of 96.5 percent carbon dioxide and 3.5 percent nitrogen. Carbon dioxide absorbs hard across exactly that infrared band.
Energy has to balance at the top of the atmosphere over the long run, so the surface keeps climbing until enough radiation finally escapes. That balance point is 464C, hot enough to melt lead. NASA’s Venus facts page gives 467C and puts the surface pressure at about 93 times Earth’s at sea level. Gas at that pressure is easy to file as background detail right up to the moment it becomes the whole story, which is also how a beached whale ends up rupturing.
Venus runs about 500 kelvin above its own light budget
Every planet has an equilibrium temperature: the value it would settle at if the sunlight it absorbed simply balanced the heat it radiated, with no atmosphere in the way. That number is the honest baseline for asking whether a world is running hot.
Cedric Gillmann and his co-authors, in a 2022 Space Science Reviews paper on the long-term evolution of Venus’s atmosphere, state it flatly: the surface temperature is 737 K, approximately 500 K higher than its equilibrium temperature. Earth’s own greenhouse boost, by NASA’s account on its energy budget page, is more than 30 degrees. Mercury, with no atmosphere at all, gets no boost and runs at whatever sunlight alone dictates.
Venus sits 30 percent closer to the Sun than Earth and still takes in less solar energy, because more than three quarters of the light reaching it never gets past the cloud tops. Everything after that is a question of how slowly the heat gets back out.
The ocean ending is still an open question
Most write-ups finish with Venus as a cautionary tale: an Earth-like world with oceans, cooked by a runaway greenhouse. The runaway greenhouse is well established as the explanation for how Venus lost its water, and Kane’s review says so directly. The oceans are the contested part. That same review notes it is unclear whether they condensed and later evaporated, or never condensed at all.
In December 2024, Tereza Constantinou, Oliver Shorttle and Paul Rimmer published a Nature Astronomy paper backing the second option. By calculating how fast Venus destroys atmospheric water, carbon dioxide and carbonyl sulfide, and how much volcanism must resupply to keep the atmosphere stable, they infer volcanic gases carrying at most a 6 percent water mole fraction, far drier than terrestrial magmas. Their conclusion is that Venus has never been liquid-water habitable.
That does not settle the argument. It does mean the tidy version, wet Venus with oceans lost to its own atmosphere, is a live hypothesis with a live competitor rather than a finding. A neat account can outlast the evidence for it: square passenger windows looked perfectly reasonable too, until fatal crashes traced the failures back to their corners.
Mercury takes the full blast of the Sun and hands all of it back before morning. Venus turns most of a weaker beam away at the cloud tops, keeps a sliver, and then declines to let go of it. The planet that rejects more than three quarters of the sunlight reaching it holds the hottest surface in the solar system, and that is one fact written twice. Strictly FYI.
Queries on file
Why is Venus hotter than Mercury?
Because Venus blocks heat leaving rather than sunlight arriving. Mercury has no atmosphere, so the sunlight its rock absorbs radiates straight back to space. Venus carries 92 bars of carbon dioxide that absorbs outgoing infrared, holding the surface near 464C against Mercury's mean of 167C.
Is Venus hotter than Mercury even though Mercury is closer to the Sun?
Yes. NASA puts Mercury 0.4 astronomical units from the Sun and Venus at 0.72, and Mercury's daytime surface does reach 430C. Venus wins on average because Mercury's night side collapses to about minus 180C while Venus stays at 464C.
Do Venus's clouds trap the Sun's heat?
For incoming light they do close to the opposite. A 2018 Space Science Reviews review by Dmitrij Titov and colleagues reports that more than 75 percent of arriving sunlight is returned to space and only about 3 percent reaches the ground. The trapping happens later, at infrared wavelengths, on the way out.
How hot is Venus, exactly?
NASA's solar system temperature table gives a mean surface temperature of 464C, and its Venus facts page quotes 467C, or 872F. That is hot enough to melt lead, under an atmosphere about 93 times heavier than Earth's at sea level.
Did Venus once have oceans?
That part is contested. A December 2024 Nature Astronomy paper by Tereza Constantinou, Oliver Shorttle and Paul Rimmer infers that Venus's interior is too dry for surface oceans ever to have formed, and concludes the planet has never been liquid-water habitable.
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