The Heaviest Element Ever Seen in an Exoplanet’s Atmosphere: Barium

exoplanet hot jupiter transiting its star
This artist’s impression shows an ultra-hot exoplanet as it is about to transit in front of its host star. Credit: ESO

Astronomers have spotted barium in the atmosphere of a distant exoplanet. With its 56 protons, you have to run your finger further down the periodic table than astronomers usually do to find barium. What does finding such a heavy element in an exoplanet atmosphere mean?

It means we’re still learning how strange exoplanets can be.

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2.46 Billion Years ago, a day on Earth was Only 17 Hours and the Moon was Much Closer

The ATV-4 is just visible as it passes into Earth's terminator. Credit: NASA TV.

As the ages pass the Moon slowly drifts away from the Earth. In conjunction the length of our day gradually gets longer. For the first time astronomers have been able to estimate the length of the day and the distance to the Moon as it was almost two and a half billion years ago. Back then, our day was only 17 hours long.

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Will Venus finally answer, ‘Are we alone?’

We recently examined how and why Saturn’s largest moon, Titan, could answer the longstanding question: Are we alone? It’s the only moon that possesses a thick atmosphere and the only planetary body other than Earth (so far) that has liquid bodies on its surface. These characteristics alone make Titan an enticing location to search for life beyond Earth. In contrast, what if life were to be found in one of the unlikeliest of places and on a planet that is known to possess some of the harshest conditions ever observed?

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Hubble Examines the Wreckage From the 2017 Kilonova

Artist's impression of two neutron stars colliding, known as a "kilonova" event. Credits: Elizabeth Wheatley (STScI)

In August 2017, astronomers observed a Gravitational Wave (GW) signal that resulted from the merger of two neutron stars – known as a “kilonova” event. The aftermath of this event (GW170817) was studied by 70 ground-based and space-based observatories in multiple wavelengths. This was the first time astronomers observed a binary neutron star merger in terms of electromagnetic radiation (particularly gamma rays) and GWs. The energy released by this merger was comparable to that of a supernova, leading astronomers to theorize that it must have resulted in a black hole.

Two years later, the Hubble Space Telescope observed the remnant and noted the powerful afterglow and gamma-ray bursts (GRBs) created by the merger, which was consistent with a black hole. However, it would take several more years of analysis before scientists could draw a complete picture of what resulted from this explosive event. Using data from Hubble and several radio observatories, a team of researchers detected a rapidly-rotating disk of material around the black hole and a structured relativistic jet emanating from it.

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Remembering the Gutsy and Hilarious Apollo Astronaut Jim McDivitt

An image of Jim McDivitt on Apollo 9, March 7, 1969, where McDivitt is conducting the world’s first docking of two crewed spacecraft with internal transfer – a technique that would become critical in the later missions to the moon. The image is from underexposed film and recovered by Andy Saunders, who used it for the cover shot of the new book “Apollo Remastered.” Credit: NASA / JSC / ASU / Andy Saunders.

Former NASA astronaut Jim McDivitt, who commanded the important Gemini IV and Apollo 9 missions – both crucial for NASA’s ability to reach the Moon — has died at age 93. His family said he passed away peacefully in his sleep on October 13, 2022.

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Scientists Discover a New Way Exoplanets Could Make Oxygen; Unfortunately, it Doesn’t Require Life

Oxygen is a valuable biosignature because Earth is oxygen-rich, and because life made all that oxygen. But if we find oxygen in an exoplanet atmosphere does that mean life made it? Or is there an abiotic source of oxygen? Image Credit: NASA

Finding oxygen in an exoplanet’s atmosphere is a clue that life may be at work. On Earth, photosynthetic organisms absorb carbon dioxide, sunlight, and water and produce sugars and starches for energy. Oxygen is the byproduct of that process, so if we can detect oxygen elsewhere, it’ll generate excitement. But researchers have also put pressure on the idea that oxygen in an exoplanet’s atmosphere indicates life. It’s only evidence of life if we can rule out other pathways that created the oxygen.

But scientists can’t rule them out.

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Planet Formation Doesn’t Have to be a Rush job After all

Astronomers believe that it can take 10 million years or more to build a planet like the Earth. But studies of protoplanetary disks show that they can only last 1 to 3 million years. How can planet formation finish if the material its made from disappears so quickly? A team of astronomers have proposed a solution: it’s a simple matter of bias in our observations.

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Arecibo Won’t Be Rebuilt

Damage to the 305-meter telescope at Arecibo Observatory, after its collapse on Dec. 1, 2020. The remains of the instrument platform are visible on the telescope’s dish. Credit: NSF.

The National Science Foundation announced last week that it won’t rebuild or replace the iconic Arecibo Observatory in Puerto Rico, which collapsed in 2020. Instead, the NSF says they have solicited calls for proposals to build a multidisciplinary educational center at the site.

Additionally, the plans do not appear to allow for any future science or observing from the other facilities at the Arecibo site, as the NSF said they will not provide any “operational support for current scientific infrastructure, such as the 12-meter radio telescope or Lidar facility,” also on location.

The announcement has been met with disappointment and disbelief.  

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Shortly Before They Collided, two Black Holes Tangled Spacetime up Into Knots

A binary black hole system, viewed from above. Image Credit: Bohn et al. (see http://arxiv.org/abs/1410.7775)

In February 2016, scientists at the Laser Interferometer Gravitational-Wave Observatory (LIGO) announced the first-ever detection of gravitational waves (GWs). Originally predicted by Einstein’s Theory of General Relativity, these waves are ripples in spacetime that occur whenever massive objects (like black holes and neutron stars) merge. Since then, countless GW events have been detected by observatories across the globe – to the point where they have become an almost daily occurrence. This has allowed astronomers to gain insight into some of the most extreme objects in the Universe.

In a recent study, an international team of researchers led by Cardiff University observed a binary black hole system originally detected in 2020 by the Advanced LIGO, Virgo, and Kamioki Gravitational Wave Observatory (KAGRA). In the process, the team noticed a peculiar twisting motion (aka. a precession) in the orbits of the two colliding black holes that was 10 billion times faster than what was noted with other precessing objects. This is the first time a precession has been observed with binary black holes, which confirms yet another phenomenon predicted by General Relativity (GR).

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NASA is Hoping They can Break the Sound Barrier… Quietly

Seventy-five years is a long time for a technology to mature. In the case of supersonic flight, the technology has matured dramatically since Chuck Yaeger first broke the sound barrier on October 14th, 1947. However, you might notice that currently, you can’t hop on a commercial supersonic jet. The reason is simple, close to seventy-five years after the technology was first developed, NASA thinks it might have a solution for its biggest hurdle.

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