Thursday, August 20, 2026

What Can We Actually Find on an Exoplanet? Part 4: Looking For Us

Earth at night, its city lights tracing the footprint of human civilization. Industry leaves atmospheric technosignatures an alien astronomer might detect. Credit: NASA (public domain).

Some signs of an alien civilization are easier to spot than signs of life itself. On technosignatures, from CFCs and industrial gases to the pandemic dip in pollution, and why Earth's most detectable moment might be right now.



Wednesday, August 19, 2026

Webb Captures the Treasure Chest at the Heart of the Carina Nebula

Hubble image of the Carina Nebula (NGC 3372), which lies just 7500 light-years away in the constellation Carina (the Keel). Credit: NASA/ESA/UC Berkeley/STScI/NOAO/AURA/NSF

This NASA/ESA/CSA James Webb Space Telescope Picture of the Month takes us to a fantastical realm within our home galaxy, where piercing starlight and billowing winds sculpt dust clouds into inventive shapes. This scene is from the Carina Nebula, which lies just 7500 light-years away in the constellation Carina (the Keel).



Pluto Planetary Science is the Gift that Keeps on Giving

Pluto as seen by New Horizons during its 2015 flyby. Sputnik Planitia is a heart-shaped region that appears to be resurfaced by upwelling liquid nitrogen from below. That action creates what look like convection cells outlined by darker lines that could be flow channels. Credit: NASA/JHU/APL/New Horizons mission

Something's wetting the surface of dwarf planet Pluto along the northern edge of Sputnik Planitia, and planetary scientists have found a good explanation for it. A recent study of new Horizons images taken during the 2015 flyby revealed evidence that liquid nitrogen is rising up through cracks in Sputnik Planitia. That's the giant heart-shaped glacial basin we see in all the Pluto images taken by the spacecraft.



The Fastest Star in the Milky Way Will Test Relativity

These panels are Very Large Telescope images of the star S301 orbiting the Milky Way's SMBH, SgrA*. S301 is the fastest moving S star ever found, and also the closest to the black hole. The star can be used to measure the black hole's spin. S301's orbit is shown with an elliptical curve. In each frame, the solid curve shows the path that the star has already completed up to that point, whereas the dashed one marks the path it will follow afterwards. Image Credit: ESO/GRAVITY collaboration

Astronomers have discovered another S star, the population of stars that orbits the Milky Way's SMBH. This one is the fastest of them all, and also comes closest to the SMBH. It will let astronomers test relativity, especially the Lense-Thirring effect.



What Can We Actually Find on an Exoplanet? Part 3: Reading the Face of a Planet

Earth's full disk, the "Blue Marble." Oceans, continents, clouds, and vegetation, all of which can in principle be read off a single distant pixel of light. Credit: NASA (public domain).

A single pixel of light holds astonishing detail. How ocean glint, rotational mapping, and the vegetation red edge let us read a distant planet's oceans, continents, and even forests, all without ever resolving it as more than a point.



Tuesday, August 18, 2026

Life On Earth May Have Had A Cold Start

Earth as seen from the International Space Station.  Credit: NASA Johnson

Nitrous oxide (otherwise known as laughing gas) is likely a key atmospheric component of life in the cosmos.



Even Near a Supermassive Black Hole, Stars Enrich the Interstellar Medium

The JWST used NIRCam and MIRI to capture this region near the Milky Way's SMBH. The star IRS 3 is in this field. It's an AGB star, and researchers are studying it to investigate the connection between material cast off from these types of stars and the interstellar medium. The researchers were surprised to find water and dust here, even though powerful radiation from the SMBH inhibit them. Image Credit: ESA/Webb, NASA & CSA, F. Peißker, J. Lu, F. Yusef-Zadeh, N. B. Sabha, C. Chan. Licence: CC BY 4.0 INT or ESA Standard Licence

Astronomers know that evolved AGB stars shed their outer layers, contributing to the makeup of the interstellar medium. But new JWST observations show this can happen even near a supermassive black hole, where powerful radiation could obliterate molecules.