Category Astronomy/Space

If the potential for Intelligent life to exist somewhere in the universe is so large, Where is Everybody?

This dwarf galaxy is named NGC 5949. It sits at a distance of around 44 million light-years from Earth, placing it within the Milky Way's cosmic neighborhood. Credit: ESA/Hubble & NASA

This dwarf galaxy is named NGC 5949. It sits at a distance of around 44 million light-years from Earth, placing it within the Milky Way’s cosmic neighborhood. Credit: ESA/Hubble & NASA

In a new paper, an astrophysicist argues that species such as ours go extinct soon after attaining high levels of technology. The universe is incomprehensibly vast, with billions of other planets circling billions of other stars. The potential for intelligent life to exist somewhere out there should be enormous. That’s the Fermi paradox in a nutshell. Daniel Whitmire, a retired astrophysicist who teaches mathematics at the University of Arkansas, once thought the cosmic silence indicated we as a species lagged far behind.

“I taught astronomy for 37 years,” said Whitmire...

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New Mission going to the Space Station to explore mysteries of ‘Cosmic Rain’

From its new vantage point on the International Space Station's Japanese Experiment Module - Exposed Facility, the Cosmic Ray Energetics and Mass (ISS-CREAM) mission, shown in the inset illustration, will study cosmic rays to determine their sources and acceleration mechanisms. Credit: NASA

From its new vantage point on the International Space Station’s Japanese Experiment Module – Exposed Facility, the Cosmic Ray Energetics and Mass (ISS-CREAM) mission, shown in the inset illustration, will study cosmic rays to determine their sources and acceleration mechanisms. Credit: NASA

A new experiment set for an Aug. 14 launch to the International Space Station will provide an unprecedented look at a rain of particles from deep space, called cosmic rays, that constantly showers our planet. The Cosmic Ray Energetics And Mass mission destined for the International Space Station (ISS-CREAM) is designed to measure the highest-energy particles of any detector yet flown in space...

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Cassini to begin final five orbits around Saturn

This artist's rendering shows Cassini as the spacecraft makes one of its final five dives through Saturn's upper atmosphere in August and September 2017. Credit: NASA/JPL-Caltech

This artist’s rendering shows Cassini as the spacecraft makes one of its final five dives through Saturn’s upper atmosphere in August and September 2017. Credit: NASA/JPL-Caltech

NASA’s Cassini spacecraft will enter new territory in its final mission phase, the Grand Finale, as it prepares to embark on a set of ultra-close passes through Saturn’s upper atmosphere with its final five orbits around the planet.

Cassini will make the first of these five passes over Saturn at 12:22 a.m. EDT Monday, Aug. 14. The spacecraft’s point of closest approach to Saturn during these passes will be between about 1,010 and 1,060 miles (1,630 and 1,710 kilometers) above Saturn’s cloud tops.

The spacecraft is expected to encounter atmosphere dense enough to require the use of its small rocket thrusters to mai...

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NASA Watches the Sun put a Stop to its Own Eruption

Failed solar eruption. Credit: NASA’s Goddard Space Flight Center/Genna Duberstein, producer.

Failed solar eruption. Credit: NASA’s Goddard Space Flight Center/Genna Duberstein, producer.

On Sept. 30, 2014, multiple NASA observatories watched what appeared to be the beginnings of a solar eruption. A filament – a serpentine structure consisting of dense solar material and often associated with solar eruptions – rose from the surface, gaining energy and speed as it soared. But instead of erupting from the Sun, the filament collapsed, shredded to pieces by invisible magnetic forces. Because scientists had so many instruments observing the event, they were able to track the entire event from beginning to end, and explain for the first time how the Sun’s magnetic landscape terminated a solar eruption.

The study makes use of a wealth of data captured by NASA’s Solar Dynamics Observator...

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