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| Astronomers have now witnessed four baby planets in the V1298 Tau system in the process of becoming super-Earths and sub-Neptunes. Image Credit: Astrobiology Center, NINS |
Thanks to the discovery of thousands of exoplanets to date, we know that planets bigger than Earth but smaller than Neptune orbit most stars. Oddly, our sun lacks such a planet. That’s been a source of frustration for planetary scientists, who can’t study them in as much detail as they’d like, leaving one big question: How did these planets form?
Now we know the answer.
An international team of astrophysicists from UCLA and elsewhere has witnessed four baby planets in the V1298 Tau system in the process of becoming super-Earths and sub-Neptunes. The findings are published in the journal Nature.
“I’m reminded of the famous ‘Lucy’ fossil, one of our hominid ancestors that lived 3 million years ago and was one of the ‘missing links’ between apes and humans,” said UCLA professor of physics and astronomy and second author Erik Petigura. “V1298 Tau is a critical link between the star- and planet-forming nebulae we see all over the sky, and the mature planetary systems that we have now discovered by the thousands.”
How planets form
Planets form when a cloud of gas and dust, called a nebula, contracts under the force of gravity into a young star and a swirling disk of matter called a protoplanetary disk. Planets form from this disk of gas, but it’s a messy process. There are many ways a planet can grow or shrink in size during its infancy --- a period of a few hundred million years. This led to major questions about why so many mature planets were between the sizes of Earth and Neptune.
The star V1298 Tau is only about 20 million years old compared to our 4.5-billion-year-old sun. Expressed in human terms, it’s equivalent to a 5-month-old baby. Four giant, rapidly evolving planets between the sizes of Neptune and Jupiter orbit the star, but unlike growing babies, the new research shows that these planets are contracting in size and are steadily losing their atmospheres. Petigura and co-author Trevor David at the Flatiron Institute led the team that first discovered the planets in 2019.
“What’s so exciting is that we’re seeing a preview of what will become a very normal planetary system,” said John Livingston, the study’s lead author from the Astrobiology Center in Tokyo, Japan. “The four planets we studied will likely contract into ‘super-Earths’ and ‘sub-Neptunes’—the most common types of planets in our galaxy, but we’ve never had such a clear picture of them in their formative years.”
Observations, hunches and a stroke of good luck lead to a big discovery
The team made the discovery by observing the transits of the planets around their star from a network of ground-and space-based telescopes for nearly a decade. A transit is when a planet crosses in front of its star, dimming it slightly. By tracking the transit over time, scientists determine the trajectory and timing of the object’s orbit. By studying the details of the transits of all the planets in a system, scientists can learn a lot about what the planets are made of and how they interact with one another.
But the V1298 Tau system didn’t make this easy. In fact, the team wouldn’t have made their discovery at all if it weren’t for following hunches and a stroke of good luck.
“We had two transits for the outermost planet separated by several years, and we knew that we had missed many in between. There were hundreds of possibilities which we whittled down by running computer models and making educated guesses,” said Petigura.
The answer came as so much news does now. A Slack message from Livingston popped up on Petigura’s screen: “Hey, we got it from the ground!”
Livingston had recovered another transit of the elusive outermost planet using a ground-based telescope, pinning down its orbital period.
“I couldn’t believe it! The timing was so uncertain that I thought we would have to try half a dozen times at least. It was like getting a hole-in-one in golf,” said Petigura.
“The effort became more and more tantalizing as we went along,” said Livingston, who earned his undergraduate degree in astrophysics at UCLA. “We nearly had to resort to brute force to crack the mystery of the outer planet, only to get it right on our first try.”
How to weigh a baby planet
Once they sorted out the shapes and timing of the orbits of the four planets, the researchers could make sense of how the planets tugged on each other due to gravity, sometimes slowing down and sometimes speeding up, and leading to transits, sometimes occurring early and other times late. These transit and timing variations allowed the team to measure the masses of all four planets for the first time, which is akin to weighing them.
The shocking result? Despite being 5 to 10 times the radius of Earth, the planets had masses only 5 to 15 times larger than Earth. This means they are very low-density, comparable to Styrofoam, whereas the Earth has the density of rock.
“The unusually large radii of young planets led to the hypothesis that they have very low densities, but this had never been measured,” said Trevor David, a co-author from the Flatiron Institute who led the initial discovery of the system in 2019. “By weighing these planets for the first time, we have provided the first observational proof. They are indeed exceptionally ‘puffy,’ which gives us a crucial, long-awaited benchmark for theories of planet evolution.”
“Our measurements reveal they are incredibly lightweight — some of the least dense planets ever found. It’s a critical step that turns a long-standing theory about how planets mature into an observed reality,” said Livingston.
Measuring the masses and sizes of planets at a critical moment in their development helps astronomers understand how they evolve over time. The V1298 planets have already lost a significant amount of their upper gaseous layers and are destined to lose more.
“These planets have already undergone a dramatic transformation, rapidly losing much of their original atmospheres and cooled faster than what we’d expect from standard models,” said James Owen, a co-author from Imperial College London who led the theoretical modeling. “But they’re still evolving. Over the next few billion years, they will continue to lose their atmosphere and shrink significantly, transforming into the compact systems of super-Earths and sub-Neptunes we see throughout the galaxy.”
Title: A young progenitor for the most common planetary systems in the Galaxy
Authors: John H. Livingston, Erik A. Petigura, Trevor J. David, Kento Masuda, James Owen, David Nesvorný, Konstantin Batygin, Jerome de Leon, Mayuko Mori, Kai Ikuta, Akihiko Fukui, Noriharu Watanabe, Jaume Orell Miquel, Felipe Murgas, Hannu Parviainen, Judith Korth, Florence Libotte, Néstor Abreu García, Pedro Pablo Meni Gallardo, Norio Narita, Enric Pallé, Motohide Tamura, Atsunori Yonehara, Andrew Ridden-Harper, Allyson Bieryla, Alessandro A. Trani, Eric E. Mamajek, David R. Ciardi, Varoujan Gorjian, Lynne A. Hillenbrand, Luisa M. Rebull, Elisabeth R. Newton, Andrew W. Mann, Andrew Vanderburg, Guðmundur Stefánsson, Suvrath Mahadevan, Caleb Cañas, Joe Ninan, Jesus Higuera, Kamen Todorov, Jean-Michel Désert, and Lorenzo Pino
Source/Credit: University of California, Los Angeles | Holly Ober
Reference Number: ps010726_01
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