Rogue planets, which do not orbit a star, could host life in hidden oceans which are protected from the cold of space by thick ice and heated by the planet’s core
Humanity has yet to find the presence of extraterrestrial life, but that may be because it’s not looking in the right spot.
Rogue planets, those that do not orbit stars, could be ripe to host life on hidden ‘Earth-like oceans,’ a study suggests.
リサーチ, which stems from フロリダ Institute of Technology astrobiologist Manasvi Lingam, suggests that rogue planets may have conditions ripe for life that are sandwiched between the cold of space and the planet’s core.
The cold of space would be too much for any potential oceans to stay liquid, but a planet’s biosphere would be protected from the cold via a layer of ice.
The planet’s core would heat the planet, creating the aforementioned Earth-like oceans.
Rogue planets (artist’s depiction) could be ripe to host life on hidden ‘Earth-like oceans’
‘We normally think of planets bound to stars, such as Mars, that could support life, but in reality, these types of life-supporting planets could just be floating out there in the vast void of space with rich biospheres,’ Lingam said in a ステートメント.
The researcher believes that for every solar system discovered, there could be between 30 そして 40 rogue planets traveling through space.
現在まで, scientists have found more than 3,000 star systems that have planets orbiting them, による NASA.
The cold of space would be too much for oceans to stay liquid, but a planet’s biosphere would be protected from the cold via a layer of ice. The planet’s core would heat the planet, creating the aforementioned Earth-like oceans
Some scientists have speculated there could be tens of billions of solar systems in the Milky Way and perhaps as many as 100 billion solar systems in the universe.
A number of so-called rogue planets have been found in recent years, including one that is roughly Earth-sized roaming across the Milky Way.
7月に, four ‘free-floating’ planets were found by NASA’s Kepler Space Telescope.
A 2019 調査 推定 there could be as many as 50 billion rogue planets in the Milky Way alone, giving researchers ample opportunity to find celestial bodies that have Earth-like oceans.
The researchers will next find out what types of extreme conditions life can survive on Earth, including low temperatures and low pressure, by looking at microbes that don’t need sunlight to survive.
It may one day be possible to travel to these rogue planets, according to Lingam, who published a paper on the topic in Advances in Space Research.
‘You might be able to get to a rogue planet in a few decades, そして, rather than looking for other planets around other stars, this might be the best chance to study these planets,’ Lingam added.
‘Through a combination of gravity assists and suitable propulsion systems, you could reach the rogue planet in 20 年かそこら.
‘Once you have a probe on the surface, you can beam the data back and it would probably take a few months to learn what it looks like on the surface.’
The study was highlighted in the September/October 2021 の問題 Discover Magazine.
Scientists study the atmosphere of distant exoplanets using enormous space satellites like Hubble
Distant stars and their orbiting planets often have conditions unlike anything we see in our atmosphere.
To understand these new world’s, and what they are made of, scientists need to be able to detect what their atmospheres consist of.
They often do this by using a telescope similar to Nasa’s Hubble Telescope.
These enormous satellites scan the sky and lock on to exoplanets that Nasa think may be of interest.
ここに, the sensors on board perform different forms of analysis.
One of the most important and useful is called absorption spectroscopy.
This form of analysis measures the light that is coming out of a planet’s atmosphere.
Every gas absorbs a slightly different wavelength of light, and when this happens a black line appears on a complete spectrum.
These lines correspond to a very specific molecule, which indicates it’s presence on the planet.
They are often called Fraunhofer lines after the German astronomer and physicist that first discovered them in 1814.
By combining all the different wavelengths of lights, scientists can determine all the chemicals that make up the atmosphere of a planet.
The key is that what is missing, provides the clues to find out what is present.
It is vitally important that this is done by space telescopes, as the atmosphere of Earth would then interfere.
Absorption from chemicals in our atmosphere would skew the sample, which is why it is important to study the light before it has had chance to reach Earth.
This is often used to look for helium, sodium and even oxygen in alien atmospheres.
This diagram shows how light passing from a star and through the atmosphere of an exoplanet produces Fraunhofer lines indicating the presence of key compounds such as sodium or helium