Space Stories: New Horizon Questions, A Dark Spot on Neptune, and Prioritizing Exoplanets

Image (Credit): NASA’s New Horizons spacecraft. (NASA/Johns Hopkins University Applied Physics Laboratory/Southwest Research Institute)

Here are some recent stories of interest.

Space.com : “NASA’s New Horizons Mission Faces an Uncertain Future (op-ed)

With its budget being trimmed for 2024, NASA is making some weighty decisions… and one includes drastically trimming New Horizons funds by replacing the current science staff with a new team in an effort to save about $3 million—a rounding error in terms of the planetary science budget...As it stands, New Horizons will exit the Kuiper Belt around 2028 and should continue operating until 2050.

ScienceDaily : “Mysterious Neptune Dark Spot Detected from Earth for the First Time

Using ESO’s Very Large Telescope (VLT), astronomers have observed a large dark spot in Neptune’s atmosphere, with an unexpected smaller bright spot adjacent to it. This is the first time a dark spot on the planet has ever been observed with a telescope on Earth. These occasional features in the blue background of Neptune’s atmosphere are a mystery to astronomers, and the new results provide further clues as to their nature and origin.

Universe Today : “TESS has Found Thousands of Possible Exoplanets: Which Ones Should JWST Study?

We will soon have more than 10,000 worlds where life might be able to survive. It’s an amazing idea, but with so many exoplanets we don’t have the resources to search for life on all of them. So how do we prioritize our search? That’s the focus of a recent paper on the pre-print server arxiv. In it, the team strives to identify the “best in class” candidates for exoplanets that could be further studied by the spectroscopic cameras of the James Webb Space Telescope (JWST). Their list could not only help astronomers find evidence of life but also help us understand the range of atmospheres exoplanets have.

The Black Hole Sagittarius A*

Image (Credit): The first image of Sagittarius A*, the supermassive black hole at the center of our galaxy. (EHT Collaboration)

The Event Horizon Telescope (EHT), an array linking together eight existing radio observatories across the planet, has created the first image of the supermassive black hole at the center of the Milky Way galaxy. Named Sagittarius A* after a radio signal coming from a location in the direction of the constellation of Sagittarius (the A and * came later), the black hole is 27,000 light-years away and estimated to be four million times more massive than our Sun. The presence of the black hole was not in question, but capturing an image such as this took many years of work.

A press release from the European Southern Observatory (ESO) quoted EHT Project Scientist Geoffrey Bower from the Institute of Astronomy and Astrophysics, Academia Sinica, Taipei:

We were stunned by how well the size of the ring agreed with predictions from Einstein’s Theory of General RelativityThese unprecedented observations have greatly improved our understanding of what happens at the very centre of our galaxy, and offer new insights on how these giant black holes interact with their surroundings.

For more on the recent breakthrough, you may want to view the ESO Press Conference on the new Milky Way results from the EHT team (here on Youtube), which is followed by a public question and answer event.

Another Exoplanet Discovered Nearby

Source/Credit: Artist rendering of a candidate exoplanet orbiting Proxima Centauri from the ESO.

Earlier this month, astronomers utilizing the European Space Observatory’s (ESO) Very Large Telescope identified what appears to be a third exoplanet orbiting Proxima Centauri, the closest star to our solar system at about 4.2 light years away. The ESO press release shared the following details:

The newly discovered planet, named Proxima d, orbits Proxima Centauri at a distance of about four million kilometres, less than a tenth of Mercury’s distance from the Sun. It orbits between the star and the habitable zone — the area around a star where liquid water can exist at the surface of a planet — and takes just five days to complete one orbit around Proxima Centauri.

The star is already known to host two other planets: Proxima b, a planet with a mass comparable to that of Earth that orbits the star every 11 days and is within the habitable zone, and candidate Proxima c, which is on a longer five-year orbit around the star.

…At just a quarter of the mass of Earth, Proxima d is the lightest exoplanet ever measured using the radial velocity technique, surpassing a planet recently discovered in the L 98-59 planetary system. The technique works by picking up tiny wobbles in the motion of a star created by an orbiting planet’s gravitational pull. The effect of Proxima d’s gravity is so small that it only causes Proxima Centauri to move back and forth at around 40 centimetres per second (1.44 kilometres per hour).

It’s great to learn a little more about our nearest neighbor.