Dozens of space-based telescopes operate near Earth and provide incredible images of the universe. But imagine a telescope far away in the outer solar system, 10 or even 100 times farther from the Sun than Earth. The ability to look back at our solar system or peer into the darkness of the distant cosmos would make this a uniquely powerful scientific tool.
I’m an astrophysicistwho studies the formation of structure in the universe. Since the 1960s, scientists like me have been considering the important scientific questions we might be able to answer with a telescope placed in the outer solar system.
So what would such a mission look like? And what science could be done?
Where a telescope is located matters nearly as much as its power. In many cases, the farther from the Sun, the better. Beinahegut/WikimediaCommons
A tiny telescope far from home
The scientific strength of a telescope far from Earth would come primarily from its location, not its size. Plans for a telescope in the outer solar system would put it somewhere beyond the orbit of Saturn, roughly a billion or more miles from Earth.
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We’d need only send a very small telescope – with a lens roughly the size of a small plate – to achieve some truly unique astrophysical insights. Such a telescope could be built to weigh less than 20 pounds (9 kilograms) and could be piggybacked on virtually anymission to Saturn or beyond.
Though small and simple compared with telescopes likeHubbleorJames Webb, such an instrument operating away from the bright light of the Sun couldmake measurementsthat are difficult oroutright impossible from a vantage point near the Earth.
The Sun has a disc of dust and gas surrounding it, much like the pinkish haze seen in this image and graphical representation of a nearby red dwarf star and its dust cloud. NASA/ESA/J. Debes
Outside looking in
Unfortunately for astronomers, getting a selfie of the solar system is a challenge. But being able to see the solar system from an outside vantage point would reveal a lot of information, in particular about the shape, distribution and composition of the dust cloud that surrounds the Sun.
Imagine a street lamp on a foggy evening – by standing far away from the lamp, the swirling mists are visible in a way that someonestanding under the streetlight could never see.
For years astrophysicists have been able to take images of and study the dust discs in solar systemsaround other stars in the Milky Way. But these stars are very far away, and there arelimits to what astronomers can learn about them. Using observations looking back toward the Sun, astronomers could compare the shape, features and composition of these distant dust clouds with detailed data on Earth’s own solar system. This data would fill gaps in knowledge about solar dust clouds and make it possible to understand the history of production, migration and destruction of dust in other solar systems that there is no hope of traveling to in person.
The universe is full of galaxies – as seen in this image called the Hubble Ultra Deep Field – and measuring the cumulative light from these is hard to do from Earth. NASA/JPL
Deep darkness of space
Another benefit of placing a telescope far from the Sun is the lack of reflected light. The disc of dust in the plane of the planets reflects the Sun’s light back at Earth. This creates a haze that is between100 and 1,000 times brighter than light from other galaxiesand obscures views of the cosmos from near Earth. Sending a telescope outside of this dust cloud would place it in a much darker region of space making it easier to measure the light coming from outside the solar system.
Once there, the telescope could measure the brightness of the ambient light of the universe over a wide range of wavelengths. This could provide insights into howmatter condensed into the first stars and galaxies. It would also enable researchers to test models of the universe by comparing the predicted sum of light from all galaxies with a precise measurement. Discrepancies could point to problems with models of structure formation in the universe or perhaps toexotic new physics.
From far enough away, it would be possible to use the Sun as a giant lens, similar to the gravitational lensing seen here as light from a distant blue galaxy is bent around a nearer orange galaxy seen in the center. ESA/Hubble/NASA
Into the unknown
Finally, increasing a telescope’s distance from the Sun would also allow astronomers to do unique science that takes advantage of aneffect called gravitational lensing, in which a massive object distorts the path light takes as it moves past an object.
One use of gravitational lensing is tosearch for and weigh rogue planets– planets that roam interstellar space after being ejected from their home solar systems. Since rogue planets don’t emit light on their own, astrophysicists can look for theireffect on the light from background stars. To differentiate between the distance of the lensing object and its mass requires observations from a second location far from Earth.
Gravitational lensing caused by a planet passing in front of a distant star will bend light from that star, and that can also be used to detect dark planets that have been ejected from solar systems. NASA Ames/JPL-Caltech/T. Pyle via WikimediaCommons
In 2011, scientists used a camera on the EPOXI mission to the asteroid belt to discover and weigh aNeptune-sized object floating free among stars in the Milky Way galaxy. Only a few rogue planets have been found, but astronomers suspect they are very common and could hold clues to theformation of solar systems and prevalence of planets around stars.
But perhaps the most interesting use for a telescope in the outer solar system would be the potential to use thegravitational field of the Sun itself as a giant lens. This kind of measurement may allow astrophysicists to actually map planets in other star systems. Perhaps one day we will be able to name continents on an Earth-like planet around a distant star.
Coming soon?
Since Pioneer 10 became the first human-made object to cross Jupiter’s orbit in 1973, there have been only a handful of astrophysical studies done from beyond the orbit of Earth. Missions to the outer solar system are rare, but many teams of scientists are doingstudies to show how an extrasolar telescope project would workand what could be learned from one.
Every 10 years or so, leaders in the astrophysics and astronomy fields gather to set goals for the following decade. That plan for the 2020s is scheduled to be released on Nov. 4, 2021. In it, I expect to see discussions about the next telescope that could revolutionize astronomy. Taking a telescope to the outer solar system, while ambitious, is well within the technological ability of NASA or other space agencies. I hope that one day soon a tiny telescope out on a lonely mission in dark reaches of the solar system will provide us incredible insights into the universe.
Article byMichael Zemcov, Associate Professor of Physics,Rochester Institute of Technology
This article is republished fromThe Conversationunder a Creative Commons license. Read theoriginal article.
Story byThe Conversation
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