Sentences with phrase «water escapes to space»

The dayside of a planet close to an M dwarf, however, might become so hot that water escapes to space; on the frigid nightside, the atmosphere could freeze to the surface.

Not exact matches

A global magnetic field might have funnelled enough energy into the atmosphere to push lighter particles escape into space, like steam from a pot of boiling water, for example.

As Mars Express flies in polar orbit, dipping to within 155 miles of the planet spinning beneath it, instruments made in Sweden, France, and Italy will map the composition of the atmosphere, looking in part for evidence that vestiges of that water are still escaping into space.

The preferential escape of lighter hydrogen over time would then lead to a skewed ratio of H2O to HDO on Mars, indicative of how much water has escaped into space.

If the energy delivered to Earth by the Sun or by impacts (or both) were 40 % greater, the Earth would experience a runaway greenhouse.3 That is, more water would evaporate from Earth's surface, so too much heat trying to escape into outer space would be blocked by water vapor in the atmosphere.

Had a Mars - size impact occurred, many small moons should have formed.e Also, the impactor's glancing blow would either be too slight to form our large Moon, or so violent that Earth would end up spinning too fast.f Besides, part of Earth's surface and mantle would have melted, but none of the indicators of that melting have been found.g Small particles splashed from Earth would have completely melted, allowing any water inside them to escape into the vacuum of space.

It has an alluring defiance defined by traits like noise, heat, harshness, and space limitation, and its shrill looks, eye - watering full - throttle urge, and exciting escapes to the limit will no doubt give those lucky 40 drivers goose bumps whenever they press down on the gas.

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(PS regarding Venus — as I have understood it, a runaway water vapor feedback would have occured when solar heating increasing to become greater than a limiting OLR value (Simpson - Kombayashi - Ingersoll limit — see http://chriscolose.wordpress.com/2010/08/23/climate-feedbacks-part-1/ — although I should add that at more «moderate» temperatures (warmer than today), stratospheric H2O increases to a point where H escape to space becomes a significant H2O sink — if that stage worked fast enough relative to solar brightening, a runaway H2O case could be prevented, and it would be a dry (er) heat.

What other things in the Earth system will change when it warms up that will affect how much SW radiation is reflected back into space [eg ice - albedo feedback, cloud changes] or affect what proportion of emitted LW radiation is allowed to escape to space [eg Water Vapour, cloud changes].

Of course, though some of the flux up at the tropopause escapes directly to space, and some is absorbed by CO2 (over the whole stratosphere in the wings of the CO2 band, concentrated towards the base of the stratosphere for larger optical thicknesses), some is absorbed by ozone (with variable concentration), and some by water vapor.

When it reaches a level high enough to cool it to it's «dew point» the water vapour condenses out in the form of clouds and rainfall and the Latent Heat of Condensation is released into the upper part of the atmosphere to accelerate the escape of radiant energy to space.

Rising water vapor content, particularly in the upper troposphere greatly reduce the amount of outgoing longwave radiation (OLR) which can escape to space.

Since the greenhouse effect is all about how energy escapes from the atmosphere to space, CO2 and other well - mixed greenhouse gases have more «leverage», so to speak, than does water.

We do not assume that albedo will increase on average to reject more heat, both through cloud SW rejection, and reduction of the distance water droplet LW needs to travel to escape to space.

The declining upper atmosphere water vapour allows heat to escape to space, offsetting the warming effect of increasing CO2 concentrations.

Additionally, while nearly 80 percent of the sunlight reflected from a roof can escape to outer space, the «thermal infrared» energy radiated by a hot, dark roof is trapped by greenhouse gases, such as CO2 and water vapor, warming the atmosphere.

The additional water vapor, acting as a greenhouse gas, absorbs energy that would otherwise escape to space and so causes further warming.

Arrival at this terminal state required passing through a «moist greenhouse» state in which surface water evaporates, water vapour becomes a major constituent of the atmosphere and H2O is dissociated in the upper atmosphere with the hydrogen slowly escaping to space [106].

A warming of 16 — 24 °C produces a moderately moist greenhouse, with water vapour increasing to about 1 % of the atmosphere's mass, thus increasing the rate of hydrogen escape to space.

That Venus had a primordial ocean, with most of the water subsequently lost to space, is confirmed by the present enrichment of deuterium over ordinary hydrogen by a factor of 100 [107], the heavier deuterium being less efficient in escaping gravity to space.

The heat provided by the Sun has to escape into space (within 12 - 24 hours in reality on average) so it is the total water vapour in the complete - all - the - way - the - top of the atmosphere that is in question here.

Scientists have proposed ways to clear space junk by launching water at it and have taken measures such as astronauts sleeping in escape pods in reaction to the growing space debris problem.

Because of the different intramolecular forces between water molecules as vapor in air, water, and ice, the wavelengths of emission and absorption are shifted; some of the radiation from the water / ice droplets at the top of a cloud can escape to space because the atmosphere above it is transparent at its wavelengths, whereas the same radiation from droplets at the bottom of a cloud will be absorbed and re-emitted in random directions from the droplets above, including back down to the originating droplets.