Evidence of forming planet discovered 335 light years from Earth

Evidence of forming planet discovered 335 light years from Earth
This graphic is an artist’s conception of the young massive star HD100546 and its surrounding disk. Credit: P. Marenfeld & NOAO/AURA/NSF

An international team of scientists led by a Clemson University astrophysicist has discovered new evidence that planets are forming around a star about 335 light years from Earth.

The team found emission that strongly suggests a planet is orbiting a relatively young star known as HD100546. The candidate planet is the second that astronomers have discovered orbiting the star.

Theories of how planets form are well-developed. But if the new study's findings are confirmed, the activity around HD100546 would mark one of the first times astronomers have been able to directly observe planet formation happening.

New discoveries from the star could allow astronomers to test their theories and learn more about the formation of solar systems, including our own, said Sean Brittain, an associate professor of astronomy and astrophysics at Clemson.

"This system is very close to Earth relative to other disk systems," he said. "We're able to study it at a level of detail that you can't do with more distant stars. This is the first system where we've been able to do this.

"Once we really understand what's going on, the tools that we are developing can then be applied to a larger number of systems that are more distant and harder to see."

For more than a decade, the team has focused some of Earth's most powerful telescopes on a disk-shaped cloud of gas and dust that surrounds HD100546.

The star is about 2.5 times larger and 30 times brighter than the sun, Brittain said. It's in the constellation Musca, or The Fly, and can only be seen from the Southern Hemisphere.

Brittain made three trips to Chile as far back as 2003 to gather data for the research. He used telescopes at the Gemini Observatory and the European Southern Observatory.

The new planet astronomers believe they have found what would be an uninhabitable gas giant at least three times the size of Jupiter, Brittain said. Its distance from the star would be about the same distance that Saturn is from the sun.

The team used a technique called "spectro-astrometry," which enables small changes in the position of the carbon monoxide emission to be measured. A source of excess carbon monoxide emission was detected that appears to vary in position and velocity. The varying position and velocity are consistent with orbital motion around the star.

The favored hypothesis is that emission comes from a "circumplanetary" disk of gas orbiting a giant planet, Brittain said.

"Another possibility is that we're seeing the wake from tidal interactions between the object and the circumstellar disk of gas and dust orbiting the star," he said.

Members of the team reported their findings in a recent edition of The Astrophysical Journal.

The name of the article is "NIR Spectroscopy of the HAeBe Star 100546. III. Further Evidence of an Orbiting Companion?" The authors are Brittain; John S. Carr of the Naval Research Laboratory in Washington, D.C.; Joan R. Najita of the National Optical Astronomy Observatory in Tucson, Arizona; and Sascha P. Quanz and Michael R. Meyer, both of ETH Zurich, Institute for Astronomy.

The next step in the study would be to take a picture using the new high-contrast imagers on the European Southern Observatory's Very Large Telescope or Gemini South Telescope, Brittain said.

Circumplanetary disks of rotating viscous material have long been thought to surround giant planets at birth, but little observational evidence for their existence has been found outside the solar system. They are believed to be the birthplaces of planetary moons, such as those that orbit Jupiter.

"There are different models of circumplanetary disks, but we've never seen one," Brittain said.

Disks form in all kinds of environments in the universe as a consequence of a fundamental law of physics known as "the conservation of angular momentum."

The law states that a spinning object will keep spinning just as hard unless a force acts on it. If the object gets smaller, it will spin faster and vice versa.

The same principle that causes ice skaters to speed up when they pull in their arms and legs also causes disks to form around objects as material falls on to them. This is true for disks around supermassive black holes at the center of galaxies, circumstellar disks around young stars and circumplanetary disks around forming planets.

Mark Leising, the chair of Clemson's astronomy and astrophysics department, said Brittain's work will raise the department's international profile.

"I congratulate Dr. Brittain and his team on their excellent work," Leising said. "Astronomers are now very good at finding already-formed planets around many nearby stars, but it has been difficult to watch the planets in the process of forming.

"Using very clever techniques and the most advanced telescopes on Earth, they have accomplished that. It's great to see our faculty working with leading institutions around the world to make discoveries at the forefront of astronomy."

Evidence of another planet forming was previously found farther out from HD100546. A blob of gas and dust that has grown denser over time was discovered about the distance Pluto is from the sun.

"It is in the process of collapsing," Brittain said. "Maybe in a million years you'll have another planet and disk."

The outer candidate planet would be a about the size of Jupiter. It's among the evidence that points to multiple and perhaps sequential .

A team that was led by Quanz and included Meyer reported the discovery of the outer candidate planet last year in The Astrophysical Journal Letters.

Explore further

Young binary star system may form planets with weird and wild orbits

More information: Astrophysical Journal paper - dx.doi.org/10.1088/0004-637X/791/2/136 , Preprint on Arxiv: arxiv.org/abs/1409.0804

Astrophysical Journal Letters paper - iopscience.iop.org/2041-8205/766/1/L1/ , Preprint on Arxiv: arxiv.org/abs/1302.7122

Provided by Clemson University
Citation: Evidence of forming planet discovered 335 light years from Earth (2014, September 4) retrieved 19 August 2019 from https://phys.org/news/2014-09-evidence-planet-years-earth.html
This document is subject to copyright. Apart from any fair dealing for the purpose of private study or research, no part may be reproduced without the written permission. The content is provided for information purposes only.

Feedback to editors

User comments

Sep 04, 2014
Theories of how planets form are well-developed.

Yet completely devoid of any experimental evidence and that which observational evidence is tenuous at best.

Sep 05, 2014
Theories of how planets form are well-developed.

Yet completely devoid of any experimental evidence and that which observational evidence is tenuous at best.

The evidence is clear that you are an idiot.

Sep 05, 2014
Theories of how planets form are well-developed.

Yet completely devoid of any experimental evidence and that which observational evidence is tenuous at best.

The evidence is clear that you are an idiot.

And it is clear you never respond with anything but a low brow comment.

Sep 05, 2014
Perhaps the one where they discovered gravity on the quantum scale so that particle interactions can be properly modelled.

And where is the experiment showing that is needed? Doesn't exist. Classical GR works very well and there is no reason to believe it would find difficulty with molecular clouds.

You ask for experiments that cannot occur but you're just ignoring observational science. You put lab experiments on a pedestal. Where is the lab experiment showing how some plasma redshift can produce a redshift of say z=1? Doesn't exist. Where is the lab experiment showing plasma can explain even some the issues of dark matter? Doesn't exist, all simulation, riddled with flaws I might add. I guess by your measure it isn't valid either.

Astronomy is by it's very nature an observational science. You can do lab analogies but you have to assume the physics scales correctly. You can't stick a solar mass of hydrogen in a vacuum chamber and watch it evolve.

Sep 08, 2014
The observed instances of BH's, DM and DE then if you please.

Sagittarius A* for black holes. Rotation curves and offset lending centres for dark matter. BAO, SN 1a and the CMB power spectrum for both DM and DE.

What's that? It's all inferred based on the mainstream interpretation of gravity as the fundamental force directing motion in the cosmos?

All results are based on some existing theory, yes. Try building a model without an assumption like that, it's literally impossible. As it happens it is a well grounded assumption given that electric are screened and magnetic forces are anisotropic.

Tweaks? What other simpler model is there that explains all the data? None. So arguments to simplicity don't apply. "These results challenge theory" does not equate to "everything we know is wrong". The only people who claim to know everything are the nutcases. Take plasma models as an example. They claim the CMB is local, the SZ effect proves otherwise, and yet it is ignored.

Sep 08, 2014
Precisely. Inference and assumption..

All science starts with an assumption, it's called a hypothesis. Unless it's EU pseudoscience where you stop at the hypothesis and call it a day.

the reason you need to find gravity on the quantum scale is that it is freely admitted that it is overwhelmed at that scale by other forces

Gravity has been seen on the quantum scale with neutron experiments.

you have to find a way for gravity to overwhelm the other forces on this scale

No. You're trying to pretend that scale isn't a factor here, that's compete and utter rubbish. By that same logic the nuclear forces never overwhelm the electromagnetic force (because they don't on this scale) and nuclei beyond hydrogen do not exist. Proof that your argument is nonsense. It is not anyone's job to meet your demands, if you believe otherwise prove it.

Please sign in to add a comment. Registration is free, and takes less than a minute. Read more