New Horizons: Second mountain range in Pluto’s Heart + Images of Nix and Hydra

More images from New Horizons of Pluto and its Moons were released today:

NASA’s New Horizons Finds Second Mountain Range in Pluto’s ‘Heart’

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A newly discovered mountain range lies near the southwestern margin of Pluto’s Tombaugh Regio (Tombaugh Region), situated between bright, icy plains and dark, heavily-cratered terrain. This image was acquired by New Horizons’ Long Range Reconnaissance Imager (LORRI) on July 14, 2015 from a distance of 48,000 miles (77,000 kilometers) and sent back to Earth on July 20. Features as small as a half-mile (1 kilometer) across are visible. Image Credit: NASA/JHUAPL/SWRI

Pluto’s icy mountains have company. NASA’s New Horizons mission has discovered a new, apparently less lofty mountain range on the lower-left edge of Pluto’s best known feature, the bright, heart-shaped region named Tombaugh Regio (Tombaugh Region).

These newly-discovered frozen peaks are estimated to be one-half mile to one mile (1-1.5 kilometers) high, about the same height as the United States’ Appalachian Mountains. The Norgay Montes (Norgay Mountains) discovered by New Horizons on July 15 more closely approximate the height of the taller Rocky Mountains.

The new range is just west of the region within Pluto’s heart called Sputnik Planum (Sputnik Plain). The peaks lie some 68 miles (110 kilometers) northwest of Norgay Montes.

This newest image further illustrates the remarkably well-defined topography along the western edge of Tombaugh Regio.

“There is a pronounced difference in texture between the younger, frozen plains to the east and the dark, heavily-cratered terrain to the west,” said Jeff Moore, leader of the New Horizons Geology, Geophysics and Imaging Team (GGI) at NASA’s Ames Research Center in Moffett Field, California. “There’s a complex interaction going on between the bright and the dark materials that we’re still trying to understand.”

While Sputnik Planum is believed to be relatively young in geological terms – perhaps less than 100 million years old – the darker region probably dates back billions of years. Moore notes that the bright, sediment-like material appears to be filling in old craters (for example, the bright circular feature to the lower left of center).

This image was acquired by the Long Range Reconnaissance Imager (LORRI) on July 14 from a distance of 48,000 miles (77,000 kilometers) and sent back to Earth on July 20. Features as small as a half-mile (1 kilometer) across are visible. The names of features on Pluto have all been given on an informal basis by the New Horizons team.

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New Horizons ‘Captures’ Two of Pluto’s Smaller Moons

While Pluto’s largest moon, Charon, has grabbed most of the lunar spotlight, two of Pluto’s smaller and lesser-known satellites are starting to come into focus via new images from NASA’s New Horizons spacecraft.

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‘Capturing’ Nix and Hydra – July 21, 2015: Pluto’s moon Nix (left), shown here in enhanced color as imaged by the New Horizons Ralph instrument, has a reddish spot that has attracted the interest of mission scientists. The data were obtained on the morning of July 14, 2015, and received on the ground on July 18. At the time the observations were taken New Horizons was about 102,000 miles (165,000 km) from Nix. The image shows features as small as approximately 2 miles (3 kilometers) across on Nix, which is estimated to be 26 miles (42 kilometers) long and 22 miles (36 kilometers) wide.

Pluto’s small, irregularly shaped moon Hydra (right) is revealed in this black and white image taken from New Horizons’ LORRI instrument on July 14, 2015 from a distance of about 143,000 miles (231,000 kilometers). Features as small as 0.7 miles (1.2 kilometers) are visible on Hydra, which measures 34 miles (55 kilometers) in length.

Nix and Hydra – the second and third moons to be discovered – are approximately the same size, but their similarity ends there.

New Horizons’ first color image of Nix, in which colors have been enhanced, reveals an intriguing region on the jelly bean-shaped satellite, which is estimated to be 26 miles (42 kilometers) long and 22 miles (36 kilometers) wide.

Although the overall surface color of Nix is neutral grey in the image, the newfound region has a distinct red tint. Hints of a bull’s-eye pattern lead scientists to speculate that the reddish region is a crater.

“Additional compositional data has already been taken of Nix, but is not yet downlinked. It will tell us why this region is redder than its surroundings,” said mission scientist Carly Howett, of the Southwest Research Institute, Boulder, Colorado. She added, “This observation is so tantalizing, I’m finding it hard to be patient for more Nix data to be downlinked.”

Meanwhile, the sharpest image yet received from New Horizons of Pluto’s satellite Hydra shows that its irregular shape resembles the state of Michigan. The new image was made by the Long Range Reconnaissance Imager (LORRI) on July 14, 2015 from a distance of 143,000 miles (231,000 kilometers), and shows features as small as 0.7 miles (1.2 kilometers) across. There appear to be at least two large craters, one of which is mostly in shadow. The upper portion looks darker than the rest of Hydra, suggesting a possible difference in surface composition. From this image, mission scientists have estimated that Hydra is 34 miles (55 kilometers) long and 25 miles (40 kilometers) wide.

“Before last week, Hydra was just a faint point of light, so it’s a surreal experience to see it become an actual place, as we see its shape and spot recognizable features on its surface for the first time,” said mission science collaborator Ted Stryk, of Roane State Community College in Tennessee.

Images of Pluto’s most recently discovered moons, Styx and Kerberos, are expected to be transmitted to Earth no later than mid-October.

Nix and Hydra were both discovered in 2005 using Hubble Space Telescope data by a research team led by New Horizons project scientist Hal Weaver, Johns Hopkins University Applied Physics Laboratory, Laurel, Maryland. New Horizons’ findings on the surface characteristics and other properties of Nix and Hydra will help scientists understand the origins and subsequent history of Pluto and its moons.

Apollo 11 lunar landing anniversary

46 years ago today humans landed on another celestial object for the first time. Here are a couple of videos about Apollo 11:

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On The Space Show this afternoon, Rand Simberg and Bill Simon spoke about the Evoloterra ceremony to mark “The Story of When We First Left Earth“. My wife and I did the ceremony a couple of years ago with friends and really enjoyed it: Our Evoloterra evening.

$100M initiative announced for the search for extraterrestrial intelligent life

Announcement of a major donation to the search for extraterrestrial intelligence (SETI) with the Breakthrough Initiative:

Yuri Milner and Stephen Hawking Announce $100 Million Breakthrough
Initiatives to Dramatically Accelerate Search for
Intelligent Life in the Universe
10-year, Multi-disciplinary Search Effort Will Harness World’s Largest Telescopes
to Mine Data from Nearest Million Stars, Milky Way and 100 Galaxies

LONDON, July 20, 2015 /PRNewswire/ — Yuri Milner was joined at The Royal Society today by Stephen Hawking, Martin Rees, Frank Drake, Geoff Marcy, Pete Worden and Ann Druyan to announce the unprecedented $100 million global Breakthrough Initiatives to reinvigorate the search for life in the universe.

10-year, Multi-disciplinary Search Effort Will Harness World’s Largest Telescopes to Mine Data from Nearest Million Stars, Milky Way and 100 Galaxies

The first of two initiatives announced today, Breakthrough Listen, will be the most powerful, comprehensive and intensive scientific search ever undertaken for signs of intelligent life beyond Earth. The second, Breakthrough Message, will fund an international competition to generate messages representing humanity and planet Earth, which might one day be sent to other civilizations.

Breakthrough Listen

  • Biggest scientific search ever undertaken for signs of intelligent life beyond Earth.
  • Significant access to two of the world’s most powerful telescopes – 100 Meter Robert C. Byrd Green Bank Telescope in West Virginia, USA (“Green Bank Telescope”)1 and 64-metre diameter Parkes Telescope in New South Wales, Australia (“Parkes Telescope”).
  • 50 times more sensitive than previous programs dedicated to SETI research.
  • Will cover 10 times more of the sky than previous programs.
  • Will scan at least 5 times more of the radio spectrum – and 100 times faster.
  • In tandem with a radio search, Automated Planet Finder Telescope at Lick Observatory in California, USA (“Lick Telescope”)2 will undertake world’s deepest and broadest search for optical laser transmissions.
  • Initiative will span 10 years.
  • Financial commitment is $100,000,000.

Unprecedented scope

The program will include a survey of the 1,000,000 closest stars to Earth. It will scan the center of our galaxy and the entire galactic plane. Beyond the Milky Way, it will listen for messages from the 100 closest galaxies. The telescopes used are exquisitely sensitive to long-distance signals, even of low or moderate power:

  • If a civilization based around one of the 1,000 nearest stars transmits to us with the power of common aircraft radar,Breakthrough Listen telescopes could detect it.
  • If a civilization transmits from the center of the Milky Way, with any more than 12 times the output of interplanetary radars we use to probe the Solar System, Breakthrough Listen telescopes could detect it.
  • From a nearby star (25 trillion miles away), Breakthrough Listen’s optical search could detect a 100-watt laser (energy output of normal household light bulb).

Open Data, Open Source, Open Platform

The program will generate vast amounts of data. All data will be open to the public. This will likely constitute the largest amount of scientific data ever made available to the public. The Breakthrough Listen team will use and develop the most powerful software for sifting and searching this flood of data. All software will be open source. Both the software and the hardware used in the Breakthrough Listen project will be compatible with other telescopes around the world, so that they could join the search for intelligent life. As well as using the Breakthrough Listen software, scientists and members of the public will be able to add to it, developing their own applications to analyze the data.

Crowdsourced processing power

Breakthrough Listen will also be joining and supporting SETI@home, University of California, Berkeley’s ground breaking distributed computing platform, with 9 million volunteers around the world donating their spare computing power to search astronomical data for signs of life. Collectively, they constitute one of the largest supercomputers in the world.

Breakthrough Message

  • International competition to create digital messages that represent humanity and planet Earth.
  • The pool of prizes will total $1,000,000.
  • Details on the competition will be announced at a later date.
  • This initiative is not a commitment to send messages. It’s a way to learn about the potential languages of interstellar communication and to spur global discussion on the ethical and philosophical issues surrounding communication with intelligent life beyond Earth.

Project Leadership

  • Martin Rees, Astronomer Royal, Fellow of Trinity College; Emeritus Professor of Cosmology and Astrophysics, University of Cambridge.
  • Pete Worden, Chairman, Breakthrough Prize Foundation.
  • Frank Drake, Chairman Emeritus, SETI Institute; Professor Emeritus of Astronomy and Astrophysics, University of California, Santa Cruz; Founding Director, National Astronomy and Ionosphere Center; Former Goldwin Smith Professor of Astronomy,Cornell University.
  • Geoff Marcy, Professor of Astronomy, University of California, Berkeley; Alberts SETI Chair.
  • Ann Druyan, Creative Director of the Interstellar Message, NASA Voyager; Co-Founder and CEO, Cosmos Studios; Emmy andPeabody award winning Writer and Producer.
  • Dan Werthimer, Co-founder and chief scientist of the SETI@home project; director of SERENDIP; principal investigator for CASPER.
  • Andrew Siemion, Director, Berkeley SETI Research Center.

Yuri Milner said: “With Breakthrough Listen, we’re committed to bringing the Silicon Valley approach to the search for intelligent life in the Universe. Our approach to data will be open and taking advantage of the problem-solving power of social networks.”

Stephen Hawking said: “I strongly support the Breakthrough Initiatives and the search for extraterrestrial life.”

Frank Drake said: “Right now there could be messages from the stars flying right through the room, through us all. That still sends a shiver down my spine. The search for intelligent life is a great adventure. And Breakthrough Listen is giving it a huge lift.”

“We’ve learned a lot in the last fifty years about how to look for signals from space. With the Breakthrough Initiatives, the learning curve is likely to bend upward significantly,” added Frank Drake.

Ann Druyan said: “The Breakthrough Message competition is designed to spark the imaginations of millions, and to generate conversation about who we really are in the universe and what it is that we wish to share about the nature of being alive on Earth. Even if we don’t send a single message, the act of conceptualizing one can be transformative. In creating the Voyager Interstellar Message, we strived to attain a cosmic perspective on our planet, our species and our time. It was intended for two distinct kinds of recipients – the putative extraterrestrials of distant worlds in the remote future and our human contemporaries. As we approach the Message’s fortieth anniversary, I am deeply grateful for the chance to collaborate on the Breakthrough Message, for what we might discover together and in the hope that it might inform our outlook and even our conduct on this world.”

Additional information www.breakthroughinitiatives.org.

The Space Show this week – July.20.15

The guests and topics of discussion on The Space Show this week:

1. Monday, July 20, 2015: 2-3:30 PM PDT (5-6:30 PM EDT; 4-5:30 PM CDT): We welcome back RAND SIMBERG & BILL SIMON for the annual EVOLOTERRA ceremony commemorating this important date. Visit www.evoloterra.com. .

2. Tuesday, July 21, 2015:,7-8:30 PM PDT (10-11:30 PM EST, 9-10:30 PM CDT): We welcome DR. JIM WOODWARD back to the show to update us on his work with .a Mach effect drive impulse engine- and gravitational physics. Check his website, http://physics.fullerton.edu/~jimw/.

3. Friday, July 24, 2015; 9:30 -11 AM PDT (12:30-2 PM EDT; 11:30-1 PM CDT): We welcome back Jon Goff for updates with his company Altius Space Machines.

4. Sunday, July 26, 2015: 12-1:30 PM PDT (3-4:30 PM EDT, 2-3:30 PM CDT): We welcome back REX RIDENOURE of Ecliptic Enterprises for updates, LightSail information and much more.

See also:
/– The Space Show on Vimeo – webinar videos
/– The Space Show’s Blog – summaries of interviews.
/– The Space Show Classroom Blog – tutorial programs

The Space Show is a project of the One Giant Leap Foundation.

Everyone can participate in space