There are now more than 5,000 confirmed planets beyond our solar system, according to NASA.
The latest addition of 65 exoplanets to the NASA Exoplanet Archive contributed to the scientific milestone marked on Monday. This archive is the home to exoplanet discoveries from peer-reviewed scientific papers that have been confirmed using multiple methods of detecting the planets.
The pickings are rich for follow-up study to learn more about these worlds with new instruments, such as the recently launched James Webb Space Telescope, and upcoming Nancy Grace Roman Space Telescope.
“It’s not just a number,” said Jessie Christiansen, science lead for the archive and a research scientist with the NASA Exoplanet Science Institute at the California Institute of Technology in Pasadena, in a statement. “Each one of them is a new world, a brand-new planet. I get excited about every one because we don’t know anything about them.”
The first two worlds ever confirmed, discovered by astronomers Alexander Wolszczan and Dale Frail, were exoplanets 4.3 and 3.9 times the mass of Earth, whirling around a dead star known as a millisecond pulsar, which sends out ‘beats’ or pulses of radio waves on millisecond timescales.
A third exoplanet, much smaller at 0.02 times the mass of Earth, was discovered orbiting the star, since named Lich, in 1994. The exoplanets were named Poltergeist, Phobetor, and Draugr, respectively.
The discovery suggested that the galaxy had to be teeming with the things. Pulsars are a type of neutron star: the dead cores of massive stars that have ejected most of their mass, then collapsed under their own gravity. Their formation process is pretty extreme, often involving colossal explosions.
“If you can find planets around a neutron star, planets have to be basically everywhere,” Wolszczan says. “The planet production process has to be very robust.”
But there was a catch. The technique used to identify these exoplanets was based on the very regular timing of pulses from the star, which are altered very slightly by the gravitational influence of the orbiting bodies.
Alas, this technique is restricted to pulsars; it’s unsuitable for main-sequence stars that don’t have regular millisecond pulsations.
However, when astronomer William Borucki of NASA pioneered the transit method, which observes faint, regular dips in starlight as an exoplanet passes between us and the host star, exoplanet science exploded.
The Kepler Space Telescope, launched in 2009, contributed over 3,000 confirmed exoplanets to the list, with another 3,000 candidates waiting in the wings.
In addition to the transit method, astronomers can study the gravitational effect exoplanets exert on their host stars. As the objects orbit a mutual center of gravity, a star appears to ‘wobble’ slightly on the spot, altering the wavelengths of its light.
In addition, if you know the mass of the star, you can study how much it wobbles to infer the mass of the exoplanet; and, if you know how intrinsically bright a star is, you can infer the size of the exoplanet.
This is how we know that there are exoplanets out there in the Universe very, very different from those we have in our own home system.
Hot Jupiters are enormous gas giants on incredibly close orbits around their stars, the proximity resulting in exoplanet temperatures that can be even hotter than some stars.
Because studying exoplanets directly is very hard – they are small, very dim, very far away, and often very close to a bright star whose light drowns out anything the exoplanet might reflect – there’s still a lot we don’t know.
There are also still a lot of worlds out there beyond our current detection thresholds.
But in the years ahead, those thresholds will retreat against the advance of technology and new analysis techniques, and we may find a variety of worlds beyond our wackiest dreams. Maybe we’ll even find traces of life outside the Solar System.