Get an Inside Look at Space Perspective’s Stratospheric Lounge (With Bar)

Interior design for Spaceship Neptune
A high-angle overview shows the interior design for Space Perspective's Spaceship Neptune passenger capsule. (Space Perspective

Mood lighting, swanky seats, plants, a bar … and a restroom with an out-of-this-world view: Those are the sorts of perks you’d expect on a luxury cruise, but the cruise that Space Perspective plans to offer with those amenities will take you 100,000 feet up, lofted by a balloon.

The Florida-based venture has just unveiled the interior design for its Spaceship Neptune capsule, which is meant to carry up to eight passengers and a pilot into the stratosphere for a look at the curving Earth beneath the black sky of space.

Space Perspective says more than 600 customers have put in their reservations at a price of $125,000 for trips that are due to begin in 2024. And to whet your appetite for the adventure, the company is offering an interactive 3-D visualization of the capsule that you can wander through virtually.

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Weird! Measurement of W Boson Doesn’t Match Standard Model of Physics

CDF at Fermilab
The Collider Detector at Fermilab recorded high-energy particle collisions from 1985 to 2011. (Fermilab Photo)

A decade ago, physicists wondered whether the discovery of the Higgs boson at Europe’s Large Hadron Collider would point to a new frontier beyond the Standard Model of subatomic particles. So far, that’s not been the case — but a new measurement of a different kind of boson at a different particle collider might do the trick.

That’s the upshot of fresh findings from the Collider Detector at Fermilab, or CDF, one of the main experiments that made use of the Tevatron particle collider at the U.S. Department of Energy’s Fermilab in Illinois. It’s not yet time to throw out the physics textbooks, but scientists around the world are scratching their heads over the CDF team’s newly reported value for the mass of the W boson.

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Perseverance’s Software Lets it Move Swiftly Across the Surface of Mars

Mars rovers are not known for being particularly speedy.  Spirit and Opportunity managed a max speed of a whopping 5 cm per second, while Curiosity clocked in at a max speed of .1 kph.  Over their long mission times, even those speeds opened up many potential areas to explore. But Perseverance is leaving them in the dust as it makes its way up to a river delta where it will begin its next round of sample collection.

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Perseverance Finally Spots its Own Parachute on the Surface of Mars

The parachute of the Perseverance rover lies on the Martian regolith in the distance. Sol 404 - MastCam-Z image. Credit: NASA/JPL-Caltech/ASU/Kevin M. Gilk

More than 13 months after the Perseverance rover landed on Mars (on February 18, 2021), the rover’s cameras have finally spotted some of the parts of the Mars 2020 landing system that got the rover safely to the ground.  The parachute and backshell were imaged by Perseverance’s MastCam-Z, seen off in the distance, just south of the rover’s current location. The image was taken on Sol 404, or April 6, 2022 on Earth.

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Supernova Remnant Cassiopeia A is Lopsided

Coloured image of Cassiopeia A based on data from the space telescopes Hubble, Spitzer and Chandra. Image Credit: NASA/JPL-Caltech [via Wikimedia]

Cassiopeia A is the remnant of a supernova that exploded 11,000 light-years away. The light from the exploding star likely reached Earth around 1670 (only a couple of years before Newton invented the reflecting telescope.) But there are no records of it because the optical light didn’t reach Earth.

The Cass A nebula ripples with energy and light from the ancient explosion and is one of the most-studied objects in deep space. It’s an expanding gas shell blasted into space when its progenitor star exploded.

But Cass A isn’t expanding evenly, and astronomers think they know why.

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Space Force is Releasing Decades of Tracking Data on a Thousand Bright Meteor Fireballs

Bright Fireball Credit: Adrian West

When a meteoroid enters the Earth’s atmosphere at a very high speed it heats up. This heating up produces a streak of light and is termed a meteor. When a meteor is bright enough, about the brightness of Venus or brighter, it becomes a fireball. Sometimes these fireballs explode in the atmosphere, becoming bolides. These bolides are bright enough to be seen even during the day.

Studying bolides as they pass through the atmosphere can help model larger asteroids, something of interest to the Planetary Defense Coordination Office (PDCO) which is run by NASA. These asteroids can be deadly if they are large enough, and learning how to predict their behavior is essential to protecting our planet from a devastating impact with long-term implications for the survival of many species on Earth.

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Jupiter and Ganymede are Connected by Magnetic Fields

Credit: SwRI

On July 5th, 2016, NASA’s Juno spacecraft arrived at Jupiter and began its four-year mission (which has since been extended to 2025) to study the gas giant’s atmosphere, composition, magnetosphere, and gravitational environment. Juno is the first dedicated mission to study Jupiter since the Galileo probe studied the system between 1995 and 2003. The images and data it has sent back to Earth have revealed much about Jupiter’s atmosphere, aurorae, polar storms, internal structure, and moons.

In addition, the Juno mission has allowed astronomers to learn more about how magnetic interaction between some of Jupiter’s moons and its atmosphere leads the gas giant to experience aurorae around its northern and southern poles. After analyzing data from Juno’s payload, a team of researchers from the Southwest Research Institute (SwRI) observed how streams of electrons from Ganymede (Jupiter’s largest moon) leave an “auroral footprint” in Jupiter’s atmosphere.

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Astronauts are Practicing Landing at the Moon's South Pole

The European Space Agency (ESA) is learning how to touch down safely at the South Pole of the Moon, without ever leaving Earth. Actual Moon landings seem to be on the horizon in the next decade via the Artemis program, and astronauts are going to have to learn to handle the unique challenges of landing in the Moon’s polar environment. With low angle sunlight and deep, permanently shadowed craters, the Moon’s South Pole poses difficulties no Apollo mission ever faced. To get hands-on experience with this environment without risking human life, ESA is putting astronauts through their paces on high-tech simulators.

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It’s Been Three Months in Deep Space, and Webb’s Mid-Infrared Instrument is Still Cooling Down

The James Webb Space Telescope continues to cool down out at its location at Lagrange Point 2, about 1.5 million kilometers from Earth. Since JWST is an infrared telescope, it needs to operate at extremely low temperatures, less than 40 K (-223 degrees Celsius, -369.4 degrees Fahrenheit). But one instrument needs to be even colder.  

To operate at peak efficiency, Webb’s Mid-Infrared Instrument (MIRI) must be cooled to a chilly 7 K (-266 C, -447 F).  And it will need a little help to reach those frigid temps.

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Dying Star Puffs out six Smoke Rings

Artist view of V Hya in its death throes. Credit: ALMA (ESO/NAOJ/NRAO)/S. Dagnello (NRAO/AUI/NSF)

Our Sun’s days are numbered. In about 5 billion years the Sun will expand into a red giant, casting off its outer layers before settling down to become a white dwarf. It’s the inevitable fate of most sunlike stars, and the process is well understood. But as a recent study shows, there are still a few things we have to learn about dying Suns.

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