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[Translate to English:] Eis im Treibhaus

Greenhouse Earth

Is the greenhouse effect indispensable or physically incomplete?

Is the Earth a Greenhouse – Yes or No?

The short answer: No.
And that is a good thing.

The crucial question, however, is: Why was the greenhouse hypothesis proposed—and what is the physical explanation behind it?
And this is exactly where it becomes interesting.

What is undisputed

Solar radiation continuously reaches the Earth’s atmosphere. Part of it is reflected, while another part is absorbed by clouds, particles, and water vapor. A key role is also played by the scattering of light within the atmosphere.

Through scattering by air molecules (Rayleigh scattering) shortwave radiation is preferentially distributed in all directions. As a result, the entire airspace is, in a sense, “filled with light,” and the sky appears blue. Without these scattering processes, there would be no uniformly illuminated sky. Instead, we would be looking into a black void, with a glaring sun as the only significant light source.

If the composition of the atmosphere changes—for example due to water vapor, dust, or aerosols (smog, Saharan dust)—the scattering behavior also changes. The proportion of longer-wavelength radiation increases, and the light becomes more diffuse:
The sky appears hazy, milky, or gray. Even the red colors of sunrise and sunset can be explained by these physical processes.

The Earth rotates—and with it, (figuratively speaking) a vast band of solar energy moves around the globe once per day. While one half of the atmosphere is exposed to radiation and heated, the other half remains in shadow and cools down.

This creates a continuous cycle of warming (radiative forcing from the Sun) and cooling (radiative emission from the Earth), which acts like a driving force that keeps the air in motion and powers our weather. The incoming and outgoing heat fluxes involved are enormous. More on this here.

Solar vs. Terrestrial Energy Flow

⇒ The incoming solar radiation flux primarily consists of short-wavelength radiation in the form of light and heat.

⇒ The Earth's thermal radiation flux re-emits this absorbed energy back into space as long-wavelength infrared radiation.

These energy flows penetrate and influence the atmosphere. The atmosphere is therefore an active medium in which radiation and energy are continuously converted and distributed across both space and time.

In addition, solar energy reaches the Earth's surface not only directly but also indirectly, in part, as diffuse radiation.

This makes it clear:
Even at this fundamental level, the climate system is not a simple radiative equilibrium, but a complex interaction of:

  • Radiation
  • Scattering
  • Absorption
  • and spatial redistribution of energy

And this is the decisive point:
Anyone who wants to understand the climate system must consider more than just radiative balances.

It must also be emphasized that we do not live under a “glass dome” like in a greenhouse. The “blue sky” is primarily an optical phenomenon. It cannot retain energy in the form of thermal radiation, regardless of direction or wavelength, like a solid enclosure (cf. the rapid temperature drop during clear, cold nights).

Where the Classical Greenhouse Explanation Falls Short

The common explanation of the greenhouse effect focuses primarily on radiative processes: Solar energy reaches the Earth, is converted into heat, and is partly emitted again as infrared radiation. “Greenhouse gases” absorb part of this thermal radiation and re-emit it—according to the theory, also back toward the Earth’s surface. Water vapor is also considered a greenhouse gas within this framework.

⇒ This principle appears physically correct.
But: it describes only part of the system, as shown on the following pages.

The Earth's radiation temperature as the basis for the greenhouse hypothesis

A key reference value in climate physics is the so-called radiation temperature of the Earth, commonly given as about 255 K (−18 °C). This value also forms the basis for the greenhouse hypothesis, which states: Without the natural greenhouse effect, the Earth would not have a comfortable average temperature of about 15°C, but rather a freezing -18°C! 
Reason to examine it more closely:

A temperature of 255 K approximately corresponds to conditions at an altitude of about 5,400 m above sea level. This is the region of the atmosphere where roughly 50% of the air mass lies below and 50% above. For context: The mass of the Earth's atmosphere is approximately 5.1 × 1018 kg. And like any mass, the mass of air also has an average temperature at which it radiates, and this temperature can be determined.

The radiation temperature at this altitude therefore indicates the average temperature of the atmospheric mass, not the “Earth’s surface temperature”. Moving downward from this altitude toward the surface, air mass and air pressure increases—and with it temperature: at sea level, this results in an average pressure of about 1,013 hPa and a temperature of 288 K. 

And this without invoking any “Greenhouse Gases.”

More on the relationship between air pressure and temperature and its calculation here.

The frequently cited radiation temperature of 255 K therefore demonstrates neither the simplicity of the system nor the greenhouse effect, but rather the complexity of the atmosphere. It shows that the Earth does not radiate directly into space from its surface, but through a several-kilometer-thick atmospheric layer, the atmospheric mass.

This crucial point is often insufficiently considered—or entirely neglected—in simplified climate representations.
What Follows from This:

  • The atmosphere is not a static heat blanket
  • It is a vertically structured, dynamic system
  • Energy exchange occurs not only through radiation, but also through convection, phase changes of water, and air movement

This makes it clear:
The widely spread idea that the Earth’s surface simply warms due to “back-radiated heat” falls short. In reality, it is a complex interaction of radiation, compressional heating, temperature decrease with altitude, air pressure, water vapor, cloud formation, oceans, and atmospheric dynamics.

Learn more about the Earth's climate system here: