Astronomers Spot an Orphaned Protostar

The HH 24 Complex (image credit: Reipurth et al.)

Astronomers have performed an impressive suite of observations at multiple wavelengths of the same system, dubbed the HH 24 complex. This complex hosts stars in the process of being born and the impacts of their violent interactions with each other, including the ejection of one of their siblings.

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How Life Reshapes the Habitable Zone

An artist's impression of a warm, wet early Mars. Image Credit: Daein Ballard. CC-BY-SA-3.0

Astronomers are very interested in the Habitable Zone of distant stars, which is the orbital radius where liquid water, and therefore potentially life, can exist on a planet in that region. But life itself changes the characteristics of a planet. New research suggestions that life is even capable of redefining what the Habitable Zone can mean.

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UFO Update Says Pentagon’s Case Count Is Rising Rapidly

UFO encounter video
Cockpit video shows an anomalous aerial encounter in 2015. Credit: U.S Navy Video

A new report to Congress says the Pentagon’s task force on UFOs — now known as unidentified aerial phenomena, or UAPs — has processed more reports in the past couple of years than it did in the previous 17 years. But that doesn’t mean we’re in the midst an alien invasion.

The unclassified report was issued this week by the Office of the Director of National Intelligence, or ODNI, in collaboration with the Department of Defense’s All-Domain Anomaly Resolution Office, or AARO. The office was created by congressional mandate, and this week’s report serves as an update to a preliminary assessment of the Pentagon’s UAP reports issued in 2021.

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NASA Satellites can Pinpoint the Exact Locations of Excessive CO2 Emissions

Carbon dioxide in Earth's atmosphere if half of global-warming emissions are not absorbed. Credit: NASA/JPL/GSFC

In 2013, the National Oceanic and Atmospheric Administration (NOAA) reported that atmospheric concentrations of carbon dioxide (CO2) had reached four-hundred parts per million (ppm) for the first time since the Pliocene Era (ca. three million years ago). According to the IPCC’s Sixth Assessment Report (AR6), “excess carbon dioxide” in our atmosphere will result in a global average temperature increase of between 1.5 and 2 °C (2.7 and 3.6 °F) by 2030. This will significantly affect ecological systems worldwide, including species extinction, droughts, wildfires, extreme weather, and crop failures.

Aside from curbing emissions, these changes call for mitigation and adaptation strategies and climate monitoring. This is the purpose of NASA’s Orbiting Carbon Observatory (OCO) 2 and 3 missions, twin satellites that make space-based observations of CO2 in Earth’s atmosphere to understand the characteristics of climate change better. Using the world’s fifth-largest coal-fired power plant as a test case, a team of researchers used data from OCO 2 and 3 to detect and track changes in CO2 and quantify the emissions produced below.

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One Day There Could be a Pipeline of Oxygen Flowing From the Moon’s South Pole

Graphic depiction of the Lunar South Pole Oxygen Pipeline. Credits: Peter Curreri

The Artemis program intends to put humans on the Moon for the first time since NASA’s Apollo missions. But Artemis has a larger scope than just landing people there, setting up some science experiments, gathering Moon rocks, playing a little golf, then leaving. The intent is to establish a consistent presence.

That will require resources, and one of those critical resources is oxygen.

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Astronomers Used a Fast Radio Burst to Probe the Structure of the Milky Way

Artist's impression of the huge halo of hot gas surrounding the Milky Way Galaxy. Credit: NASA

In the past decade and a half, hundreds of Fast Radio Bursts (FRBs) have been detected by astronomers. These transient energetic bursts occur suddenly, typically last for just a few milliseconds, and are rarely seen again (except in the rare case of repeating bursts). While astronomers are still not entirely sure what causes this phenomenon, FRBs have become a tool for astronomers hoping to map out the cosmos. Based on the way radio emissions are dispersed as they travel through space, astronomers can measure the structure and distribution of matter in and around galaxies.

Using the Deep Synoptic Array (DSA) at the Owens Valley Radio Observatory (OVRO), a team of astronomers from Caltech and Cornell University used an intense FRB from a nearby galaxy to probe the halo of hot gas that surrounds the Milky Way. Their results show that our galaxy has significantly less visible (“baryonic” or “normal”) matter than previously expected. These findings support theories that matter is regularly ejected from our galaxy due to stellar winds, supernovae, and accreting supermassive black holes (SMBHs).

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TESS has Found A Second Earth-Sized World in This System. Exoplanet Science is Maturing

Newly discovered Earth-size planet TOI 700 e orbits within the habitable zone of its star in this illustration. Its Earth-size sibling, TOI 700 d, can be seen in the distance. Credit: NASA/JPL-Caltech/Robert Hurt

For planet-hunters, finding an Earth-sized exoplanet must be special. NASA estimates there are about 100 billion planets in the Milky Way, but the large majority of the 5,000+ exoplanets we’ve found are extremely inhospitable. So finding one that’s similar to ours is kind of comforting.

In this case, it’s even more interesting because it’s the second Earth-sized planet orbiting the same star.

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NASA is Continuing to Build the Titan Dragonfly Helicopter. Here are its Rotors

Ingenuity, the helicopter assisting NASA’s Mars Perseverance rover on its mission, has been a huge success. It gathered the achievement of the first controlled flight on another heavenly body, has performed spectacularly over its 28 flights and holds records for both speed and distance. But it might not for long, as a much bigger, more capable helicopter is currently under development. And when it eventually explores Titan in the next decade, it has an excellent chance to smash many of Ingenuity’s records.

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JWST Pioneer Passes Along Advice for Future Space Telescope Builders

John Mather
Nobel-winning physicist John Mather is the senior project scientist for NASA's James Webb Space Telescope. (NASA Photo / Chris Gunn)

After a quarter-century of development, NASA’s James Webb Space Telescope is a smashing success. But senior project scientist John Mather, a Nobel-winning physicist who’s played a key role in the $10 billion project since the beginning, still sees some room for improvement.

Mather looked back at what went right during JWST’s creation, as well as what could be done better the next time around, during a lecture delivered today at the American Astronomical Society’s winter meeting in Seattle.

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Astronomers Begin to Understand Strange “Backsplash” Galaxies

SMACS cluster from JWST shows evidence of dark matter
The galaxy cluster SMACS 0723 as seen by NIRCam on JWST. It's gravitational lensing properties (from its mass and from the mass of dark matter) are helping astronomers identify 88 distant galaxies in this field of view for further study. Courtesy NASA, ESA, CSA, STScI

Clusters of galaxies do not appear in an instant. Instead they gradually form through the accumulation of many galaxies. But when galaxies fall in they don’t just stop moving. Instead, they keep moving around. These are called backsplash galaxies, and astronomers are using them to help understand the formation history of their home clusters.

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