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Europe’s PLATO Telescope: Hunting Earth-like Planets Beyond Our Solar System

How many Earth-like planets exist throughout the universe? This is what recent talk given at the National Astronomy Meeting 2024 hopes to address as Dr. David Brown, who is a scientist on the European Space Agency’s (ESA) PLATO (PLAnetary Transits and Oscillations of stars) mission, provided an update on the mission and the goals it hopes to achieve. This comes as PLATO is currently scheduled to launch in December 2026 with the goal of finding Earth-like planets throughout the universe, which could greatly expand our knowledge of exoplanets, as well.

“PLATO’s goal is to search for exoplanets around stars similar to the Sun and at orbital periods long enough for them to be in the habitable zone,” said Dr. Brown. “One of the main mission objectives is to find another Earth-Sun equivalent pair, but it is also designed to carefully and precisely characterize the exoplanets that it finds (i.e. work out their masses, radii, and bulk density).”

Pillars of Creation star in New Visualization from NASA’s Hubble and Webb Telescopes

Made famous in 1995 by NASA’s Hubble Space Telescope, the Pillars of Creation in the heart of the Eagle Nebula have captured imaginations worldwide with their arresting, ethereal beauty.

Now, NASA has released a new 3D visualization of these towering celestial structures using data from NASA’s Hubble and James Webb space telescopes. This is the most comprehensive and detailed multiwavelength movie yet of these star-birthing clouds.

“By flying past and amongst the pillars, viewers experience their three-dimensional structure and see how they look different in the Hubble visible-light view versus the Webb infrared-light view,” explained principal visualization scientist Frank Summers of the Space Telescope Science Institute (STScI) in Baltimore, who led the movie development team for NASA’s Universe of Learning.

Life-Detection Potential on Europa and Enceladus: Amino Acid Insights

Based on our experiments, the ‘safe’ sampling depth for amino acids on Europa is almost 8 inches (around 20 centimeters) at high latitudes of the trailing hemisphere (hemisphere opposite to the direction of Europa’s motion around Jupiter) in the area where the surface hasn’t been disturbed much by…


How deep will future landers to Jupiter’s moon, Europa, and Saturn’s moon, Enceladus have to dig to find organic molecules aka the building blocks of life? This is what a recent study published in Astrobiology hopes to address as an international team of researchers investigated whether near-surface organic molecules on Europa and Enceladus could survive the intense solar and cosmic radiation since neither moon has a magnetic field like the Earth to shield it. This study holds the potential to help scientists better understand the conditions for finding life beyond Earth and the methods for finding that life, as well.

Image of Jupiter’s moon, Europa, obtained by NASA’s Juno spacecraft in September 2022. (Credit: NASA/JPL-Caltech/SwRI/MSSS Image processing: Kevin M. Gill CC BY 3.0)

Image of plumes emanating from the south pole of Enceladus obtained by NASA’s Cassini spacecraft. (Credit: NASA/JPL/Space Science Institute)

For the study, the researchers exposed several amino acids in ices and dead organisms using liquid nitrogen to varying levels of radiation to ascertain how fast they degrade under these harsh conditions. The goal was to determine if organic molecules could survive the harsh environments on Europa and Enceladus since neither moon possesses a magnetic field like the Earth to shield their surfaces from harmful cosmic radiation. The team discovered that while certain amino acids experienced initial declines at low doses, no further declines were observed for increased doses, which they note could bode well for sampling from the surfaces of Europa or Enceladus.

First of its kind Detection made in Striking New Webb Image

For the first time, a phenomenon astronomers have long hoped to directly image has been captured by NASA’s James Webb Space Telescope’s Near-Infrared Camera (NIRCam). In this stunning image of the Serpens Nebula, the discovery lies in the northern area (seen at the upper left) of this young, nearby star-forming region.

Astronomers found an intriguing group of protostellar outflows, formed when jets of gas spewing from newborn stars collide with nearby gas and dust at high speeds. Typically these objects have varied orientations within one region. Here, however, they are slanted in the same direction, to the same degree, like sleet pouring down during a storm.

The discovery of these aligned objects, made possible due to Webb’s exquisite spatial resolution and sensitivity in near-infrared wavelengths, is providing information into the fundamentals of how stars are born.

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