Roman Telescope Could Turn up Over 100,000 Planets Through Microlensing

Recently we reported on a haul of 2,200 new exoplanets from the 2 year primary mission of the Transiting Exoplanet Survey Satellite (TESS). But that is just the tip of the iceberg in terms of exoplanet hunting.  If calculations from NASA are correct the Nancy Grace Roman Space Telescope could detect up to 100,000 new exoplanets when it launches in 2025.

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InSight Detects Two Significant Quakes from the Cerberus Fossae Region on Mars

NASA’s InSight lander felt the distant rumble of two major ‘marsquakes’ in March, originating from a region near the Martian equator known as the Cerberus Fossae. Registering magnitudes of 3.1 and 3.3 on March 7th and March 18th respectively, the quakes cement the Cerberus Fossae’s reputation as one of the most geologically active places on the Red Planet today. A pair of similarly strong marsquakes rocked the same region back in 2019.

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A new way to see Inside Neutron Stars

The song of a binary tells us about neutron stars. Credit: University of Bath

Imagine trying to study an object light-years away that is less than 20 kilometers in diameter. The object is so dense that it’s made of material that can’t exist naturally on Earth. This is the challenge astronomers face when studying neutron stars, so they have to devise ingenious ways to do it. Recently a team figured out how to study them by using the power of resonance.

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A Lake in a Martian Crater was Once Filled by Glacial Runoff

Artist's impression of Mars during the Noachian Era. Credit: Ittiz/Wikipedia Commons

All across the Martian surface, there are preserved features that tell the story of what Mars once looked like. These include channels that were carved by flowing water, delta fans where water deposited sediment over time, and lakebeds where clay and hydrated minerals are found. In addition to telling us more about Mars’ past, the study of these features can tell us about how Mars made the transition to what it is today.

According to new research led by Brown Ph.D. student Ben Boatwright, an unnamed Martian crater in Mars southern highlands showed features that indicate the presence of water, but there is no indication of how it got there. Along with Brown professor Jim Head (his advisor), they concluded that the crater’s features are likely the result of runoff from a Martian glacier that once occupied the area.

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Interstellar Comet Borisov is so Pristine, it’s Probably Never Been Close to a Star Before

This image was taken with the FORS2 instrument on ESO’s Very Large Telescope in late 2019, when comet 2I/Borisov passed near the Sun. Since the comet was travelling at breakneck speed, around 175 000 kilometres per hour, the background stars appeared as streaks of light as the telescope followed the comet’s trajectory. The colours in these streaks give the image some disco flair and are the result of combining observations in different wavelength bands, highlighted by the various colours in this composite image.

By comparing our local Comet Hale-Bopp to the interstellar visitor 2I/Borisov, a team of astronomers have concluded that the interloper is perhaps one of the most pristine comets we’ve ever seen.

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Satellites Have Brightened the Skies by About 10% Across the Entire Planet

starlink satellite streaks
An image of the NGC 5353/4 galaxy group made with a telescope at Lowell Observatory in Arizona, USA on the night of Saturday 25 May 2019. The diagonal lines running across the image are trails of reflected light left part of a Starlink satellite constellation.

New research has found that as the number of satellites in Earth orbit continues to increase, their accumulated light pollution will brighten the night sky – making it much harder to do fundamental astronomy.

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TESS has Found 2,200 Potential Exoplanets so far

Exoplanetology has been on a tear recently.  This is largely due to an abundance of data collected by a new generation of satellites, one of which is the Transiting Exoplanet Survey Satellite (TESS).  Now the project has reached a new milestone with another release of data – 2,200 planet candidates collected, far surpassing the 1,600 expected candidates in the mission’s first two years.  Now comes a potentially even more daunting task – following up with each of them.

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If Astronomers see Isoprene in the Atmosphere of an Alien World, There’s a Good Chance There’s Life There

Artists’s impression of the rocky super-Earth HD 85512 b. Credit: ESO/M. Kornmesser

It is no exaggeration to say that the study of extrasolar planets has exploded in recent decades. To date, 4,375 exoplanets have been confirmed in 3,247 systems, with another 5,856 candidates awaiting confirmation. In recent years, exoplanet studies have started to transition from the process of discovery to one of characterization. This process is expected to accelerate once next-generation telescopes become operational.

As a result, astrobiologists are working to create comprehensive lists of potential “biosignatures,” which refers to chemical compounds and processes that are associated with life (oxygen, carbon dioxide, water, etc.) But according to new research by a team from the Massachusetts Institute of Technology (MIT), another potential biosignature we should be on the lookout for is a hydrocarbon called isoprene (C5H8).

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In a Comprehensive new Test, the EmDrive Fails to Generate any Thrust

Artist's concept of an interstellar craft. Credit and Copyright: Mark Rademaker

The EmDrive is a hypothetical rocket that proponents claim can generate thrust with no exhaust. This would violate all known physics. In 2016, a team at NASA’s Eagleworks lab claimed to measure thrust from an EmDrive device, the news of which caused quite a stir. The latest attempt to replicate the shocking results has resulted in a simple answer: the Eagleworks measurement was from heating of the engine mount, not any new physics.

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Clear Signs of Recent Erosion on Mars

Erosion can take many forms.  Most commonly known is water wearing away the sides of creeks or lakes.  But wind can erode just as effectively, especially if it carries dust particles that can eat away at otherwise solid objects.  While this wind-driven process is most commonly observed on Earth, it plays a role in the history of most other rocky bodies that have an atmosphere.  Recently, a team lead scientists from the Planetary Science Institute found evidence for some erosion from between 50,000 and a few million years ago in Mars’s polar ice cap.  That is a blink of the eye by geological standards.

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