The episode, “We Need to Talk About That “First Exomoon” Discovery,” is basically an hour-long monologue by Dr. Kipping as he discussed the discovery, compares it to earlier similar discoveries, goes over the current definition of a exomoon, and quotes other astronomers regarding their position on the discovery.
The bottom line is that the media may have overplayed the discovery, similar discoveries happened in the past, and the lack of a good definition for an exomoon makes any decision on this new discovery troublesome.
Dr. Kipping has a particular interest in exomoons, and he admits this bias at the start of the show, but he does a good job covering all of the terrain. It is an informative one-man debate reminiscent of the difficulties in defining Pluto.
I recommend you check it out.
Note: The episode can also be found on YouTube. Also, go to this earlier story for more by Dr. Kipping on exomoons.
Image (Credit): On July 31, 2026, NASA officials and others pose for a photo before cutting the ribbon to open the Flight Dynamics Research Facility at NASA’s Langley Research Center in Hampton, Virginia. (NASA/Keegan Barber)
Here are some recent space-related stories of interest.
Friday was a historic day for NASA’s Langley Research Center in Hampton, Virginia. A stellar lineup of VIPs from NASA, GSA, Congress, Virginia and Langley employees celebrated the ribbon-cutting ceremony for NASA’s newest and most advanced wind tunnel: the Flight Dynamics Research Facility. The $53 million, 25,000-square-foot FDRF, built by BL Harbert International, is the first wind tunnel added to NASA’s wind tunnel assets in 40 years. The project was started in June 2022, with construction completed in March 2026.
On July 27, technicians at NASA’s Kennedy Space Center in Florida installed a memory card containing 1,350,144 names as part of a commemorative plaque on the Nancy Grace Roman Space Telescope. The names were submitted by people globally, including astronauts from Artemis II and Artemis III. The memory card will travel with the Roman observatory to the Sun-Earth Lagrange point 2, or L2, about one million miles from Earth, where the Sun’s and Earth’s gravity balance out.
An international research team has discovered evidence of a moonlike body. It marks the first time such an object has been detected outside our solar system—though just how close it comes to being a moon is a question researchers are still grappling with. Although more than 6,000 exoplanets have been discovered to date, there’s been a lack of definitive evidence of moons in other planetary systems. The new findings challenge that by focusing on an object orbiting the brown dwarf CD-35 2722 B in a system 73 light-years away.
This time last year I highlighted a paper that discussed a possible exomoon circling an exoplanet called WASP-49Ab located about 635 light-years away . It was spotted by the European Southern Observatory’s Very Large Telescope in Chile.
Well, now the James Webb Space Telescope (JWST) has provided data related to another possible exomoon orbiting a hot Jupiter-like exoplanet called WASP-39b. It is located about 700 million light-years away.
In a Scientific American article titled “Have Astronomers Finally Found an Exomoon?” we learn that a paper is being released shortly outlining the argument for this potential “hypervolcanic exomoon.” This presumed IO-like exomoon is being cooked by the parent sun.
Recent infrared spectroscopy from the James Webb Space Telescope (JWST) has spurred analyses of common volcanic gases such as carbon dioxide (CO2), sulfur dioxide (SO2), alongside alkali metals sodium (Na I) and potassium (K I) surrounding the hot Saturn WASP-39 b. We report more than an order-of-magnitude of variability in the density of neutral Na, K, and SO2 between ground-based measurements and JWST, at distinct epochs, hinting at exogenic physical processes similar to those sourcing Io’s extended atmosphere and torus. Tidally-heated volcanic satellite simulations sputtering gas into a cloud or toroid orbiting the planet, are able to reproduce the probed line-of-sight column density variations. The estimated SO2 flux is consistent with tidal gravitation predictions, with a Na/SO2 ratio far smaller than Io’s. Although stable satellite orbits at this system are known to be < 15.3 hours, several high-resolution alkali Doppler shift observations are required to constrain a putative orbit. Due to the Roche limit interior to the planetary photosphere at ~ 8 hours, atmosphere-exosphere interactions are expected to be especially important at this system.
It is a dense summary, but also a hopeful finding that may lead to more focused searches for exomoons.
The addition of exomoons to the list of new discoveries will only increase the chances that some form of life can be found among he many solar systems we can study. Interestingly enough, we are still probing our own solar system’s moons with the same hope.
Image (Credit): An artist’s rendering of a volcanic moon orbiting WASP-49 b. (NASA/ JPL-Caltech)
The search for new exoplanets in our galaxy continues, but now it may include the first exomoon. This was something that was expected to occur at some point as the detection methods became better over time.
The exomoon in question is believed to be a volcanic moon orbiting a giant planet about 635 light-years away. Detected using the European Southern Observatory’s Very Large Telescope in Chile, the exomoon is discussed in a paper written by researchers with NASA’s Jet Propulsion Laboratory and Caltech in California. The clue was a cloud of sodium that did not appear to come from the host exoplanet.
The new discovery is being compared to Jupiter’s volcanic moon Io, which is the most volcanically active world in the solar system.
If you want to learn more about exomoons, I recommend a Cool Worlds video narrated by Assistant Professor of Astronomy David Kipping who provides five reasons that the study of exomoons is so important.
Once upon a cosmic time, scientists assumed that stars apply an eternal magnetic brake, causing an endless slowdown of their rotation. With new observations and sophisticated methods, they have now peeked into a star’s magnetic secrets and found that they are not what they expected. The cosmic hotspots for finding alien neighbors might be around stars hitting their midlife crisis and beyond. This groundbreaking study, shedding light on magnetic phenomena and habitable environments, has been published in The Astrophysical Journal Letters.
In a system with two known planets, astronomers spotted something new: a small object transiting across the Sun-sized star. This turned out to be another planet: extra hot and Earth-sized…The newly-spotted planet, called HD 63433 d, is tidally locked, meaning there is a dayside which always faces its star and a side that is constantly in darkness. This exoplanet, or planet outside of our solar system, orbits around the star HD 63433 (TOI 1726) in the HD 63433 planetary system. This scorching world is the smallest confirmed exoplanet younger than 500 million years old. It’s also the closest discovered Earth-sized planet this young, at about 400 million years old.
Does the size of an exomoon help determine if life could form on an exoplanet it’s orbiting? This is something a February 2022 study published in Nature Communications hopes to address as a team of researchers investigated the potential for large exomoons to form around large exoplanets (Earth-sized and larger) like how our Moon was formed around the Earth. Despite this study being published almost two years ago, its findings still hold strong regarding the search for exomoons, as astronomers have yet to confirm the existence of any exomoons anywhere in the cosmos. But why is it so important to better understand the potential for large exomoons orbiting large exoplanets?