Please explain why
all of the planets with atmospheres (including Earth) have a surface temperature that is much higher than their blackbody temperatures.
That is why established science does not list the radiative features of constituent gases as one of the factors that influence the equilibrium temperature
of planets with atmospheres.
Intrinsic to the whole scenario is the fact that the surface temperature
of a planet with an atmosphere is fixed by mass, gravity and insolation alone so that changes in the composition of the atmosphere can have no effect.
Not exact matches
With our
planet screaming its accelerating anguish via contaminated oceans, poisoned soils and polluted
atmosphere — we indifferently add 80 million
of ourselves annually and one billion more every 12 years.
One possible strategy for making Mars habitable over the long term is to «terraform» it — manipulate its environment so, in the simplest terms, the
planet warms up, ice turns into water, and plants can be introduced, which will convert the atmospheric carbon dioxide into oxygen,
with the goal
of creating a stable and breathable
atmosphere.
Each time one
of these waves
of light would pour into our
atmosphere, the
planet's vibration was raised to a slightly higher frequency, elevating our living Earth — along
with us earthlings — to a higher level.
Who knows, there might be other life forms out there on
planets with differnt types
of suns, other types
of atmosphere, maybe even based on something other than carbon... Religion can't answer those questions, but science, ever so slowly, is plugging away at the answers.
There are hundreds
of billions
of stars in our galaxy, each
with planets, that large
of a number even if a tiny fraction had an
atmosphere and even if a fraction
of them had water (as we know it is required, but life may not require it on other
planets) it would be amazing if there wasn't a carbon based lifeform somewhere else in our galaxy, let alone in the universe
with billions
of galaxies each
with billions
of stars and trillions
of planets.
In 2007, the tiny Comet Holmes grew and expanded so much that the gassy diameter
of the comet's coma, or
atmosphere, became larger than the diameter
of the sun,
with particles reaching all
of the
planets.
It's no mystery why carbon dioxide (CO2) levels fluctuate
with the seasons: As greenery grows in the spring and summer, it soaks up the
planet - warming gas, and when trees shed their leaves in the autumn, some
of that gas returns to the
atmosphere.
With greater knowledge
of the composition
of exoplanet
atmospheres and their dynamics, astronomers hope to figure out which formation theories can explain the diversity
of planet types revealed over the past 2 decades.
The move, part
of a climate science planning report sent today to Congress, will likely further normalize discussion
of deliberate tinkering
with the
atmosphere to cool the
planet, and
of directly collecting carbon from the sky, both topics once verboten in the climate science community.
By combining observations from the ground and in space, the team observed a plume
of low - energy plasma particles that essentially hitches a ride along magnetic field lines — streaming from Earth's lower
atmosphere up to the point, tens
of thousands
of kilometers above the surface, where the
planet's magnetic field connects
with that
of the sun.
Researchers have found a host
of Earth - like
planets, and are trying to understand what conditions might be like at the surface
of a
planet with a rocky core and a thick
atmosphere.
The slope
of the gap trends downward,
with most
of the largest rocky worlds nestling close to their stars, suggesting the
planets started out
with thick
atmospheres that their stars blew away.
Patrick Dufour
of the University
of Montreal in Canada and colleagues have now found a white dwarf
with the most contaminated
atmosphere yet, suggesting it ate something as big as a dwarf
planet.
The new maps
of Jupiter are the first created under the outer
Planet Atmospheres Legacy (OPAL) program, which will provide Hubble
with time each year to study the outer
planets.
Now he is looking for something far more familiar: a smallish rocky
planet with an
atmosphere that bears the chemical imprint
of life, like the abundant (and otherwise inexplicable) oxygen that plants pump into our own air.
But Earth's
atmosphere, which now contains an abundance
of greenhouse gases, differs in composition compared
with three centuries ago, and solar physicists say they're unsure how a long solar hiatus would affect the
planet's 21st century climate.
The Carbon cycle is a geological process that regulates the CO2 - level in the
atmosphere and
with that, the temperature
of the
planet's surface: In the ocean, CO2, in its dissolved form, undergoes a chemical reaction and is then transported into Earth's mantle.
There's no true surface on Neptune, since its
atmosphere gradually merges
with the water, but a trip above the clouds will afford you a gorgeous glimpse
of the
planet's six rings and 13 moons.
With knowledge only of the luminosity of the star (1/600 that of the sun), the mass of the planet (1.3 times that of Earth), and the length of its orbit (11.2 days), the team was able to predict that, with a variety of possible atmospheres, it would be possible for Proxima b to harbor liquid water on its surf
With knowledge only
of the luminosity
of the star (1/600 that
of the sun), the mass
of the
planet (1.3 times that
of Earth), and the length
of its orbit (11.2 days), the team was able to predict that,
with a variety of possible atmospheres, it would be possible for Proxima b to harbor liquid water on its surf
with a variety
of possible
atmospheres, it would be possible for Proxima b to harbor liquid water on its surface.
Alternatively, he says, the
planet could have an
atmosphere, albeit a very strange one filled
with clouds
of evaporated rock.
I think in 10 years we'll have several examples
of planets in habitable zones around small stars, and we'll have data to work
with to understand their
atmospheres.
Fingers
of thick haze thousands
of kilometres across feel their way around the
planet,
with various bands
of the
atmosphere circling at different speeds.
If Proxima b proves to have an
atmosphere, Loeb and Kreidberg have also proposed using Webb to probe for the infrared signature
of ozone in Proxima Centauri's glare as a possible sign that the
planet's air is filled
with oxygen — something that, on Earth, is mostly produced by life.
For about a minute, running on half a hair dryer's worth
of power, the orbiter - cum - probe beamed direct measures
of the
planet's
atmosphere, along
with final probes
of its gravity and magnetic field, to mission control at the Jet Propulsion Laboratory (JPL) in Pasadena, California.
The
planets of the TRAPPIST - 1 system could be complex worlds
with volcanoes,
atmospheres and warm subsurface oceans.
Sara Seager
of MIT, who collaborates
with Deming, is trying to figure out which spectral signatures in a
planet's
atmosphere would provide the best evidence for signs
of life.
While lower - energy ultraviolet radiation breaks up water molecules — a process called photodissociation — ultraviolet rays
with more energy (XUV radiation) and X-rays heat the upper
atmosphere of a
planet, which allows the products
of photodissociation, hydrogen and oxygen, to escape.
The dearth
of gas means inner
planets remain largely rocky,
with thin
atmospheres.
The
planet «could have a thick
atmosphere with lots
of water, either in the
atmosphere, in oceans or both,» Caldwell says.
When that materialmostly particles no larger than grains
of sandcomes into contact
with our
planet's
atmosphere it burns up, creating meteors, or shooting stars.
However, this research applies this model to a
planet with conditions far from that present on Earth,
with temperatures exceeding one thousand degrees and an
atmosphere spanning pressures orders
of magnitude larger.
As we flood the
atmosphere with more CO2, and average global temperatures rise, some areas
of the
planet are getting wetter.
In the case
of Venus, you're seeing that the effects that were going on were drawing away the oxygen disproportionately and leaving the
planet enriched
with carbon dioxide in it's
atmosphere.
Other observations, made
with the Hubble Space Telescope and published yesterday in Nature Astronomy, found no signs
of hydrogen in the
atmospheres of planets d, e, and f, but were inconclusive for TRAPPIST - 1g.
«Here was a
planet with all the elements needed to support life in its
atmosphere,
with evidence
of liquid water in the past, and yet there was no life --[as if] Mars had the lights on, but nobody was home,» he says.
In a decade, NASA hopes to launch a network
of space - based telescopes that will be able to pinpoint Earth - like
planets in other solar systems and see whether life has altered their
atmosphere in the same way it has here on Earth — flooding it
with oxygen, for example.
Plugging in the numbers, the punch line is: If there is a rocky
planet transiting a nearby bright M - star
with signs
of life in its
atmosphere, we will be able to find it.
With them it will peer through the creaking, dusty cosmic eons to study much that astronomers using Hubble and other telescopes have barely begun to glimpse: the universe's very first galaxies, nascent stars and
planets in mid-creation in nebulous wombs, the
atmospheres of worlds both within and beyond our solar system.
In March, one team predicted a «meteor hurricane» on Mars,
with billions
of bits
of dust streaking through the Red
Planet's
atmosphere each hour for about 5 hours.
Photosynthetic microbes filled the
atmosphere with oxygen billions
of years ago but they renovated the
planet without awareness.
The lander was armed
with a robot arm to burrow into the soil, a laser to analyse the
atmosphere and oodles
of other high - tech gadgets to analyse the past and present Martian climate and help unravel the
planet's ancient history.
It takes rocket science to launch and fly spacecraft to faraway
planets and moons, but a deep understanding
of how materials perform under extreme conditions is also needed to enter and land on
planets with atmospheres.
Just weeks before the historic encounter
of comet C / 2013 A1 (Siding Spring)
with Mars in October 2014, NASA's Mars
Atmosphere and Volatile Evolution (MAVEN) spacecraft entered orbit around the Red
Planet.
With that objective in mind, the NASA team has programmed the sensor - laden Juno to measure the chemical composition
of the
planet's
atmosphere and to map its gravitational and magnetic fields.
Furthermore, the spectra
of the carbon monoxide molecules indicate that unlike many other hot Jupiters, the
planet's
atmosphere has no temperature inversion; instead, temperature drops
with increasing altitude.
And
with good reason: The largest
of those moons, 3,200 - mile - wide Titan, has an
atmosphere that may be similar to that
of our own
planet in its younger days, and Enceladus, a 300 - mile - wide ball, has a geologically active surface.
The oceans will boil away and the
atmosphere will dry out as water vapor leaks into space, and temperatures will soar past 700 degrees Fahrenheit, all
of which will transform our
planet into a Venusian hell - scape choked
with thick clouds
of sulfur and carbon dioxide.