“The Genesis Planet” –Did Hubble Observe the Oldest Planet in the Milky Way? (Friday’s Most Popular)

 

 

Artist's_impression_of_pulsar_planet_B1620-26c

 

The existence of a 13-billion year old planet, if in fact it still exists, highlights the fact that our Solar System exits in a universe that is estimated to be between 13.5 and 14 billion years old. A few intrepid astronomers have concluded that the most productive to look for planets that can support life is around dim, dying stars white dwarfs so prevalent in globular cluster M4 shown above.


“In the quest for extraterrestrial biological signatures, the first stars we study should be white dwarfs,” said Avi Loeb, theorist at the Harvard-Smithsonian Center for Astrophysics (CfA) and director of the Institute for Theory and Computation. Even dying stars could host planets with life – and if such life exists, we might be able to detect it within the next decade.

In July 2003, Hubble helped make the astounding discovery of a planet called PSR B1620-26b (an artist’s impression above), 2.5 times the mass of Jupiter, which is located in globular cluster M4 shown in the image below taken by Hubble Space Telescope. It contains several tens of thousands stars and is noteworthy in being home to many white dwarfs—the cores of ancient, dying stars whose outer layers have drifted away into space. It is the first planet found in a globular cluster, and one of the oldest known extrasolar planets, believed to be about 12.7 billion years old.

PSR B1620-26 b orbits a pair of stars just outside the core of M4: a pulsar, a neutron star, and a white dwarf with a mass of 0.34 solar masses orbiting each other at a distance of 1 AU about once every six months.  Each orbit of the planet takes about 100 years. Because all stars in a cluster form at about the same time, and planets form together with their host stars, it is likely that PSR B1620-26 b is also about 12.7 billion years old,  nearly three times as old as Earth.

 

M4JM

 

“A globular cluster might be the first place in which intelligent life is identified in our galaxy,” observed Rosanne DiStefano of the Harvard-Smithsonian Center for Astrophysics (CfA) in January, 2016. Globular star clusters are extraordinary in almost every way. The globulars, which are found in the halo of a galaxy, contain considerably more stars than the less dense galactic, or open clusters, which are found in the disk. They’re densely packed, holding a million stars in a ball only about 100 light-years across on average. They’re old, dating back almost to the birth of the Milky Way. And according to new research, they also could be extraordinarily good places to look for space-faring civilizations.

When a star like the Sun dies, it puffs off its outer layers, leaving behind a hot core called a white dwarf. A typical white dwarf is about the size of Earth. It slowly cools and fades over time, but it can retain heat long enough to warm a nearby world for billions of years. Since a white dwarf is much smaller and fainter than the Sun, a planet would have to be much closer in to be habitable with liquid water on its surface.

A habitable planet would circle the white dwarf once every 10 hours at a distance of about a million miles.* Before a star becomes a white dwarf it swells into a red giant, engulfing and destroying any nearby planets. Therefore, a planet would have to arrive in the habitable zone after the star evolved into a white dwarf. A planet could form from leftover dust and gas (making it a second-generation world), or migrate inward from a larger distance.

If planets exist in the habitable zones of white dwarfs, we would need to find them before we could study them. The abundance of heavy elements on the surface of white dwarfs suggests that a significant fraction of them have rocky planets. Loeb and his colleague Dan Maoz (Tel Aviv University) estimate that a survey of the 500 closest white dwarfs could spot one or more habitable Earths.

The best method for finding such planets is a transit search – looking for a star that dims as an orbiting planet crosses in front of it. Since a white dwarf is about the same size as Earth, an Earth-sized planet would block a large fraction of its light and create an obvious signal.

More importantly, we can only study the atmospheres of transiting planets. When the white dwarf’s light shines through the ring of air that surrounds the planet’s silhouetted disk, the atmosphere absorbs some starlight. This leaves chemical fingerprints showing whether that air contains water vapor, or even signatures of life, such as oxygen.

Astronomers are particularly interested in finding oxygen because the oxygen in the Earth’s atmosphere is continuously replenished, through photosynthesis, by plant life. Were all life to cease on Earth, our atmosphere would quickly become devoid of oxygen, which would dissolve in the oceans and oxidize the surface. Thus, the presence of large quantities of oxygen in the atmosphere of a distant planet would signal the likely presence of life there.

NASA’s James Webb Space Telescope (JWST), scheduled for launch by the end of this decade, promises to sniff out the gases of these alien worlds. Loeb and Maoz created a synthetic spectrum, replicating what JWST would see if it examined a habitable planet orbiting a white dwarf. They found that both oxygen and water vapor would be detectable with only a few hours of total observation time.

“JWST offers the best hope of finding an inhabited planet in the near future,” said Maoz. Recent research by CfA astronomers Courtney Dressing and David Charbonneau showed that the closest habitable planet is likely to orbit a red dwarf star (a cool, low-mass star undergoing nuclear fusion). Since a red dwarf, although smaller and fainter than the Sun, is much larger and brighter than a white dwarf, its glare would overwhelm the faint signal from an orbiting planet’s atmosphere. JWST would have to observe hundreds of hours of transits to have any hope of analyzing the atmosphere’s composition.

“Although the closest habitable planet might orbit a red dwarf star, the closest one we can easily prove to be life-bearing might orbit a white dwarf,” said Loeb.

The Daily Galaxy via Arxiv, and Harvard-Smithsonian CfA

Image Credit: Top of page, pulsar planet B1620-26c https://upload.wikimedia.org/wikipedia/commons/4/44/Artist’s_impression_of_pulsar_planet_B1620-26c.jpg; M4 image via NASA, STScI, WikiSky (center of the cluster)

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