ESO’s VLT spots brand-new type of star formation
ESO Public Information Officer
Garching bei München, Germany
Astronomers have for a long time studied the glowing, cosmic clouds of gas and dust catalogued as NGC 6334 and NGC 6357, this gigantic new image from ESO’s Very Large Telescope Survey Telescope being only the most recent one. With around two billion pixels this is one of the largest images ever released by ESO. The evocative shapes of the clouds have led to their memorable names: the Cat’s Paw Nebula and the Lobster Nebula, respectively. Credit: ES
Written by Elizabeth Landau
Jet Propulsion Laboratory, Pasadena, Calif.
October 21, 2016
This artist’s concept depicts ”heartbeat stars,” which have been detected by NASA’s Kepler Space Telescope and others. Image credit: NASA/JPL-Caltech
Matters of the heart can be puzzling and mysterious – so too with unusual astronomical objects called heartbeat stars.
Heartbeat stars, discovered in large numbers by NASA’s Kepler space telescope, are binary stars (systems of two stars orbiting each other) that got their name because if you were to map out their brightness over time, the result would look like an electrocardiogram, a graph of the electrical activity of the heart. Scientists are interested in them because they are binary systems in elongated elliptical orbits. This makes them natural laboratories for studying the gravitational effects of stars on each other.
In a heartbeat star system, the distance between the two stars varies drastically as they orbit each other. Heartbeat stars can get as close as a few stellar radii to each other, and as far as 10 times that distance during the course of one orbit.
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Written by George McGinn
Cosmology and Space Research
September 27, 2016 at 4:32pm EST
In one of the most promising places in the Solar System where life may exist, astronomers using NASA’s Hubble Space Telescope have photographed what appears to be water vapor plumes escaping Jupiter’s moon Europa.
The team from the Space Telescope Science Institute (STScI) in Baltimore saw finger-like projections when viewing Europa as it past in front of Jupiter, according to team leader William Sparks.
The discovery occurred by accident as the team’s original proposal was to observe Europa to determine if it had an atmosphere or exosphere.
An exosphere of neon was detected on Earth’s Moon on August 17, 2015 based on study the data from the Lunar Atmosphere and Dust Environment Explorer (LADEE) spacecraft.
Note from George McGinn: Yesterday I watched NASA’s briefing, and the Juno Spacecraft did something nearly impossible. The largest danger to the mission is the immense radiation. Jupiter’s version of Earth’s Van Allen belt have been catching huge amounts of solar radiation for 4.5 billion years. The gravity of Jupiter is so strong that it pulls more charged particles than would directly hit it. The Juno team estimated that the spacecraft will be exposed to radiation at LD25 (LD is Leathal Dose and 25 means 25 times, so 25 times the lethal dose to a human), or having 1 million dental X-rays all at once (in a space of 2 seconds). This is equal to 260 rads.
I applaud the Juno’s team, who worked almost 12 years to get this spacecraft safely in orbit. I am excited to see finally how deep the atmosphere goes, what gases make up Jupiter, and if there is a solid or semi-solid center, or just compressed gases. And can all that gas create the large magnetic field, or what is in the center, the speed of spin, and the chemical makeup.