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Venice News Updates

News of Venice, CA and Marina del Rey CA

NASA’s First Deep-Space CubeSats Say: “Polo!”

Note:  Based on press release from NASA/JPL

Bob Eklund Looking Up Column

Bob Eklund
Looking Up Column

NASA has received radio signals indicating that the first-ever CubeSats headed to deep space are alive and well. Engineers will now be performing a series of checks before both CubeSats enter their cruise to deep space.

Mars Cube One, or MarCO, is a pair of briefcase-sized spacecraft that launched May 5 along with NASA’s InSight Mars lander from Vandenberg Air Force Base in Central California. InSight is a scientific mission that will probe the Red Planet’s deep interior for the first time. The name stands for Interior Exploration using Seismic Investigations, Geodesy and Heat Transport.

The twin MarCO CubeSats are on their own separate mission: rather than collecting science, they will follow the InSight lander on its cruise to Mars, testing out miniature spacecraft technology along the way.

Both were programmed to unfold their solar panels soon after launch, followed by several opportunities to radio back their health.

“Both MarCO-A and B say ‘Polo!’ It’s a sign that the little sats are alive and well,” said Andy Klesh, chief engineer for the MarCO mission at NASA’s Jet Propulsion Laboratory in Pasadena, California, which built the twin spacecraft.

A couple of weeks will be spent assessing how the MarCO CubeSats are performing. If they survive the radiation of space and function as planned, they’ll fly over the Red Planet during InSight’s entry, descent and landing in November.

Seven Habitable-Zone Planets Found around Single Star

 

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This artist’s concept shows what the TRAPPIST-1 planetary system may look like, based on available data about the planets’ diameters, masses and distances from the host star. Credit: NASA-JPL/Caltech

 

Bob Eklund Looking Up Column

Bob Eklund
Looking Up Column

Note:  This is from a NASA press release.

 

NASA’s Spitzer Space Telescope has revealed the first known system of seven Earth-size planets around a single star. Three of these planets are located in the habitable zone, the area around the parent star where a rocky planet is most likely to have liquid water.

The discovery sets a new record for greatest number of habitable-zone planets found around a single star outside our solar system. All of these seven planets could have liquid water — key to life as we know it — under the right atmospheric conditions.

“This discovery could be a significant piece in the puzzle of finding habitable environments, places that are conducive to life,” said Thomas Zurbuchen, associate administrator of the agency’s Science Mission Directorate in Washington. “Answering the question ‘are we alone’ is a top science priority and finding so many planets like these for the first time in the habitable zone is a remarkable step forward toward that goal.”

At about 40 light-years (235 trillion miles) from Earth, the system of planets is relatively close to us, in the constellation Aquarius.

Using Spitzer data, the team precisely measured the sizes of the seven planets and developed first estimates of the masses of six of them, allowing their density to be estimated.

In contrast to our sun, the TRAPPIST-1 star-classified as an ultra-cool dwarf-is so cool that liquid water could survive on planets orbiting very close to it, closer than is possible on planets in our solar system.

NASA’s Juno Spacecraft Sends First In-Orbit View

Note: this is a press release from JPL

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This color view from NASA’s Juno spacecraft is made from some of the first images taken by JunoCam after the spacecraft entered orbit around Jupiter on July 5th (UTC). Image credit: NASA/JPL-Caltech/SwRI/MSSS

Bob Eklund Looking Up

Bob Eklund
Looking Up

The JunoCam camera aboard NASA’s Juno mission is operational and sending down data after the spacecraft’s July 4 arrival at Jupiter. Juno’s visible-light camera was turned on six days after Juno fired its main engine and placed itself into orbit around the largest planetary inhabitant of our solar system. The first high-resolution images of the gas giant Jupiter are still a few weeks away.

“This scene from JunoCam indicates it survived its first pass through Jupiter’s extreme radiation environment without any degradation and is ready to take on Jupiter,” said Scott Bolton, Juno principal investigator from the Southwest Research Institute in San Antonio. “We can’t wait to see the first view of Jupiter’s poles.”

The view was obtained on July 9, when the spacecraft was 2.7 million miles from Jupiter on the outbound leg of its initial 53.5-day capture orbit. The color image shows atmospheric features on Jupiter, including the famous Great Red Spot, and three of the massive planet’s four largest moons—Io, Europa, and Ganymede, from left to right in the image.

NASA Targets May 2018 Launch for Mars InSight Mission

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Note: This is a press release from JPL/NASA.

NASA has set a new launch opportunity, beginning May 5, 2018, for the InSight mission to Mars. InSight is the first mission dedicated to investigating the deep interior of Mars. Image credit: NASA/JPL-Caltech

NASA has set a new launch opportunity, beginning May 5, 2018, for the InSight mission to Mars. InSight is the first mission dedicated to investigating the deep interior of Mars. Image credit: NASA/JPL-Caltech

NASA’s Interior Exploration using Seismic Investigations, Geodesy and Heat Transport (InSight) mission to study the deep interior of Mars is targeting a new launch window that begins May 5, 2018, with a Mars landing scheduled for Nov. 26, 2018.

InSight’s primary goal is to help us understand how rocky planets—including Earth—formed and evolved. The spacecraft had been on track to launch this month until a vacuum leak in its prime science instrument prompted NASA in December to suspend preparations for launch.

InSight project managers recently briefed officials at NASA and France’s space agency, Centre National d’Études Spatiales (CNES), on a path forward; the proposed plan to redesign the science instrument was accepted in support of a 2018 launch.

“The science goals of InSight are compelling, and the NASA and CNES plans to overcome the technical challenges are sound,” said John Grunsfeld, associate administrator for NASA’s Science Mission Directorate in Washington. “The quest to understand the interior of Mars has been a longstanding goal of planetary scientists for decades. We’re excited to be back on the path for a launch, now in 2018.”

NASA’s Jet Propulsion Laboratory in Pasadena, California, will redesign, build and conduct qualifications of the new vacuum enclosure for the Seismic Experiment for Interior Structure (SEIS), the component that failed in December. CNES will lead instrument level integration and test activities, allowing the InSight Project to take advantage of each organization’s proven strengths. The two agencies have worked closely together to establish a project schedule that accommodates these plans, and scheduled interim reviews over the next six months to assess technical progress and continued feasibility.

The cost of the two-year delay is being assessed. An estimate is expected in August, once arrangements with the launch vehicle provider have been made.

The seismometer instrument’s main sensors need to operate within a vacuum chamber to provide the exquisite sensitivity needed for measuring ground movements as small as half the radius of a hydrogen atom. The rework of the seismometer’s vacuum container will result in a finished, thoroughly tested instrument in 2017 that will maintain a high degree of vacuum around the sensors through rigors of launch, landing, deployment and a two-year prime mission on the surface of Mars.

“The shared and renewed commitment to this mission continues our collaboration to find clues in the heart of Mars about the early evolution of our solar system,” said Marc Pircher, director of CNES’s Toulouse Space Centre.

The mission’s international science team includes researchers from Austria, Belgium, Canada, France, Germany, Japan, Poland, Spain, Switzerland, the United Kingdom and the United States.

Ceres: Celebrating 215 Years of Planetary Discovery

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Note: This is a press release from JPL.

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New Year’s Day, 1801, the dawn of the 19th century, was a historic moment for astronomy, and for a space mission called Dawn more than 200 years later. That night, Giuseppe Piazzi pointed his telescope at the sky and observed a distant object that we now know as dwarf planet Ceres.

Today, NASA’s Dawn mission allows us to see Ceres in exquisite detail. From the images Dawn has taken over the past year, we know Ceres is a heavily cratered body with diverse features on its surface that include a tall, cone-shaped mountain and more than 130 reflective patches of material that is likely salt. But on that fateful evening in 1801, Piazzi wasn’t sure what he was seeing when he noticed a small, faint light through his telescope.

“When Piazzi discovered Ceres, exploring it was beyond imagination. More than two centuries later, NASA dispatched a machine on a cosmic journey of more than 3 billion miles to reach the distant, mysterious world he glimpsed,” said Marc Rayman, mission director and chief engineer for Dawn at NASA’s Jet Propulsion Laboratory, Pasadena, California.

Piazzi was the director of the Palermo Observatory in Sicily, Italy, which has collected documents and instruments from the astronomer’s time, and published a booklet on the discovery of Ceres. According to the observatory, Piazzi had been working on a catalog of star positions on January 1, 1801, when he noticed something whose “light was a little faint and colored as Jupiter.” He looked for it again on subsequent nights and saw that its position changed slightly.

What was this object? Piazzi wrote to fellow astronomers Johann Elert Bode and Barnaba Oriani to tell them he had discovered a comet.

“I have presented this star as a comet, but owing to its lack of nebulosity, and to its motion being so slow and rather uniform, I feel in the heart that it could be something better than a comet, perhaps. However, I should be very careful in passing this conjecture to the public,” Piazzi wrote to Oriani.

By July 1801, Piazzi had calculating the object’s orbit and made public his observations, announcing it as a planet, and naming it “Ceres”—after the Roman goddess of agriculture, was also the patron deity of Sicily, where Piazzi then lived and worked.

The news was especially interesting to Bode because he had championed the Titius-Bode hypothesis: that the positions of planets in our solar system follow a specific pattern, which predicts each planet’s distance from the Sun. The pattern demanded that there be a planet, yet undiscovered, between Mars and Jupiter—and this is exactly where Ceres orbited.

In March 1802, Heinrich Wilhelm Matthias Olbers discovered a second, similar object: Pallas. William Herschel, discoverer of Uranus, then wrote an essay proposing that both Ceres and Pallas represented an entirely new class of objects, which he named “asteroids.”

The door had opened for many more asteroids to be observed. The discoveries of Juno in 1804 and Vesta in 1807 reinforced Herschel’s notion that asteroids are a class of their own. Today, we know there are hundreds of thousands of asteroids in the main asteroid belt between Mars and Jupiter.

Now, as we commemorate the 215th anniversary of Ceres’ discovery, Dawn is observing the dwarf planet from its lowest orbit ever: 240 miles from the surface. The many craters and other features that Piazzi could not see with his telescope are being named after agricultural deities or festivals, extending the theme that Piazzi began with the name “Ceres.”

NASA’s Curiosity Mars Rover Heads Toward Active Dunes

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Note: This is based on press release from NASA/JPL.

This Sept. 25, 2015, view from the Mast Camera on NASA's Curiosity Mars rover shows a dark sand dune in the middle distance. Credit: NASA/JPL-Caltech/MSSS

This Sept. 25, 2015, view from the Mast Camera on NASA’s Curiosity Mars rover shows a dark sand dune in the middle distance. Credit: NASA/JPL-Caltech/MSSS

On its way to higher layers of the mountain where it is investigating how Mars’ environment changed billions of years ago, NASA’s Curiosity Mars rover will take advantage of a chance to study some modern Martian activity at mobile sand dunes.

In the next few days, the rover will get its first close-up look at these dark dunes, called the “Bagnold Dunes,” which skirt the northwestern flank of Mount Sharp. No Mars rover has previously visited a sand dune, as opposed to smaller sand ripples or drifts. One dune Curiosity will investigate is as tall as a two-story building and as broad as a football field. The Bagnold Dunes are active: Images from orbit indicate some of them are migrating as much as about 3 feet per Earth year. No active dunes have been visited anywhere in the solar system besides Earth.

“We’ve planned investigations that will not only tell us about modern dune activity on Mars but will also help us interpret the composition of sandstone layers made from dunes that turned into rock long ago,” said Bethany Ehlmann ofCaltech and JPL..

As of Nov. 16, Curiosity has about 200 yards remaining to drive before reaching “Dune 1.” The rover is already monitoring the area’s wind direction and speed each day and taking progressively closer images, as part of the dune research campaign. At the dune, it will use its scoop to collect samples for the rover’s internal laboratory instruments, and it will use a wheel to scuff into the dune for comparison of the surface to the interior.

What distinguishes actual dunes from windblown ripples of sand or dust, like those found at several sites visited previously by Mars rovers, is that dunes form a downwind face steep enough for sand to slide down. The effect of wind on motion of individual particles in dunes has been studied extensively on Earth, a field pioneered by British military engineer Ralph Bagnold (1896-1990). Curiosity’s campaign at the Martian dune field informally named for him will be the first in-place study of dune activity on a planet with lower gravity and less atmosphere.

Observations of the Bagnold Dunes with the Compact Reconnaissance Imaging Spectrometer on NASA’s Mars Reconnaissance Orbiter indicate that mineral composition is not evenly distributed in the dunes. The same orbiter’s High Resolution Imaging Science Experiment has documented movement of Bagnold Dunes.

“We will use Curiosity to learn whether the wind is actually sorting the minerals in the dunes by how the wind transports particles of different grain size,” Ehlmann said.

Ehlmann and Nathan Bridges of the Johns Hopkins University’s Applied Physics Laboratory, Laurel, Maryland, lead the Curiosity team’s planning for the dune campaign.

“These dunes have a different texture from dunes on Earth,” Bridges said. “The ripples on them are much larger than ripples on top of dunes on Earth, and we don’t know why. We have models based on the lower air pressure. It takes a higher wind speed to get a particle moving. But now we’ll have the first opportunity to make detailed observations.”

THE KELSO DUNES in California’s Mojave Desert are a good example of somewhat similar dunes on Earth. These dunes, covering 45 square miles near the town of Baker, are called “booming” or “singing” dunes because of the low-pitched resonant noise they produce—especially when someone slides down their steep face. Do the Bagnold Dunes on Mars also boom, when slid down? That’s something for an expedition of human “Martians” to check out, some day.

New Names and Insights at Dwarf Planet Ceres

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Eklund scours the astronomy press releases and chooses the one or ones most interesting for his readers. This is a press release from Jet Propulsion Laboratory

Colorful new maps of Ceres, based on data from NASA’s Dawn spacecraft, showcase a diverse topography, with height differences between crater bottoms and mountain peaks as great as 9 miles.

Scientists continue to analyze the latest data from Dawn as the spacecraft makes its way to its third mapping orbit.

“The craters we find on Ceres, in terms of their depth and diameter, are very similar to what we see on Dione and Tethys, two icy satellites of Saturn that are about the same size and density as Ceres. The features are pretty consistent with an ice-rich crust,” said Dawn science team member Paul Schenk, a geologist at the Lunar and Planetary Institute, Houston.

Some of these craters and other features now have official names, inspired by spirits and deities relating to agriculture from a variety of cultures (since Ceres takes its name from the Roman goddess of agriculture). The International Astronomical Union recently approved a batch of names for features on Ceres.

The newly labeled features include Occator, the mysterious crater containing Ceres’ brightest spots, which has a diameter of about 60 miles and a depth of about 2 miles. Occator is the name of the Roman agriculture deity of harrowing, a method of leveling soil.

A smaller crater with bright material, previously labeled “Spot 1,” is now identified as Haulani, after the Hawaiian plant goddess. Haulani has a diameter of about 20 miles. Temperature data from Dawn’s visible and infrared mapping spectrometer show that this crater seems to be colder than most of the territory around it.

Dantu crater, named after the Ghanaian god associated with the planting of corn, is about 75 miles across and 3 miles deep. A crater called Ezinu, after the Sumerian goddess of grain, is about the same size. Both are less than half the size of Kerwan, named after the Hopi spirit of sprouting maize, and Yalode, a crater named after the African Dahomey goddess worshipped by women at harvest rites.

“The impact craters Dantu and Ezinu are extremely deep, while the much larger impact basins Kerwan and Yalode exhibit much shallower depth, indicating increasing ice mobility with crater size and age,” said Ralf Jaumann, a Dawn science team member at the German Aerospace Center (DLR) in Berlin.

Almost directly south of Occator is Urvara, a crater named for the Indian and Iranian deity of plants and fields. Urvara, about 100 miles wide and 3 miles deep, has a prominent central pointy peak that is 2 miles high.

Dawn is currently spiraling toward its third science orbit, 900 miles above the surface, or three times closer to Ceres than its previous orbit. The spacecraft will reach this orbit in mid-August and begin taking images and other data again.

Ceres, with a diameter of 584 miles, is the largest object in the main asteroid belt, located between Mars and Jupiter. This makes Ceres about 40 percent the size of Pluto, another dwarf planet, which NASA’s New Horizons mission flew by earlier this month.

On March 6, 2015, Dawn made history as the first mission to reach a dwarf planet, and the first to orbit two distinct extraterrestrial targets. It conducted extensive observations of asteroid Vesta in 2011-2012.