Category Archives: Space Systems

Mars Reconnaissance Orbiter reaches 10 year milestone

This video shows a small sample of the many magnificent images of the Martian surface taken by the Mars Reconnaissance Orbiter MRO during its first 10 years of operation:

NASA’s Mars Reconnaissance Orbiter has clocked more than a decade of service at the Red Planet and has yielded scientific discoveries and magnificent views of a distant world. These images taken by MRO’s HiRISE camera are not in true color because they are optimized for geological science.

Here is a release from NASA noting the 10 year milestone:

Ten Years of Discovery by Mars Reconnaissance Orbiter

True to its purpose, the big NASA spacecraft that began orbiting Mars a decade ago this week has delivered huge advances in knowledge about the Red Planet.

NASA’s Mars Reconnaissance Orbiter (MRO) has revealed in unprecedented detail a planet that held diverse wet environments billions of years ago and remains dynamic today.

One example of MRO’s major discoveries was published last year, about the possibility of liquid water being present seasonally on present-day Mars.  It drew on three key capabilities researchers gained from this mission: telescopic camera resolution to find features narrower than a driveway; spacecraft longevity to track seasonal changes over several Martian years; and imaging spectroscopy to map surface composition.

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NASA’s Mars Reconnaissance Orbiter, nearing the 10th anniversary of its arrival at Mars, used its High Resolution Imaging Science Experiment (HiRISE) camera to obtain this view of an area with unusual texture on the southern floor of Gale Crater. Credits: NASA/JPL-Caltech/Univ. of Arizona
Other discoveries have resulted from additional capabilities of the orbiter. These include identifying underground geologic structures, scanning atmospheric layers and observing the entire planet’s weather daily. All six of the orbiter’s science instruments remain productive in an extended mission more than seven years after completion of the mission’s originally planned primary science phase.

“This mission has helped us appreciate how much Mars — a planet that has changed greatly over time — continues to change today,” said MRO Project Scientist Rich Zurek of NASA’s Jet Propulsion Laboratory, Pasadena, California. JPL manages the mission.

Data from MRO have improved knowledge about three distinct periods on Mars. Observations of the oldest surfaces on the planet show that diverse types of watery environments existed — some more favorable for life than others. More recently, water cycled as a gas between polar ice deposits and lower-latitude deposits of ice and snow, generating patterns of layering linked to cyclical changes similar to ice ages on Earth.

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Dynamic activity on today’s Mars includes fresh craters, avalanches, dust storms, seasonal freezing and thawing of carbon dioxide sheets, and summertime seeps of brine.

The mission provides three types of crucial support for rover and stationary lander missions to Mars. Its observations enable careful evaluation of potential landing sites. They also help rover teams choose routes and destinations. Together with NASA’s Mars Odyssey, which has been orbiting Mars since 2001, MRO relays data from robots on Mars’ surface to NASA Deep Space Network antennas on Earth, multiplying the productivity of the surface missions.

The mission has been investigating areas proposed as landing sites for future human missions in NASA’s Journey to Mars.

“The Mars Reconnaissance Orbiter remains a powerful asset for studying the Red Planet, with its six instruments all continuing capably a decade after orbit insertion. All this and the valuable infrastructure support that it provides for other Mars missions, present and future, make MRO a keystone of the current Mars Exploration Program,” said Zurek.

Arrival at Mars

On March 10, 2006, the spacecraft fired its six largest rocket engines for about 27 minutes, slowing it down enough for the gravity of Mars to catch it into orbit. Those engines had been used only once before, for 15 seconds during the first trajectory adjustment during the seven-month flight from Earth to Mars. They have been silent since arrival day. Smaller engines provide thrust for orbit adjustment maneuvers.

For its first three weeks at Mars, the spacecraft flew elongated, 35-hour orbits ranging as far as 27,000 miles (43,000 kilometers) from the Red Planet. During the next six months, a process called aerobraking used hundreds of carefully calculated dips into the top of the Martian atmosphere to gradually adjust the size of the orbit. Since September 2006, the craft has been flying nearly circular orbits lasting about two hours, at altitudes from 155 to 196 miles (250 to 316 kilometers).

The spacecraft’s two large solar panels give MRO a wingspan the length of a school bus. That surface area helped with atmospheric drag during aerobraking and still cranks out about 2,000 watts of electricity when the panels face the sun. Generous power enables the spacecraft to transmit a torrent of data through its main antenna, a dish 10 feet (3 meters) in diameter. The total science data sent to Earth from MRO — 264 terabits — is more than all other interplanetary missions combined, past and present.

Lockheed Martin Space Systems, Denver, built the spacecraft with the capability to transmit copious data to suit the science goals of revealing Mars in great detail, which requires plenty of data.

For example, the mission’s High Resolution Imaging Science Experiment (HiRISE) camera, managed by the University of Arizona, Tucson, has returned images that show features as small as a desk anywhere in observations that now have covered about 2.4 percent of the Martian surface, an area equivalent to two Alaskas, with many locations imaged repeatedly. The Context Camera (CTX), managed by Malin Space Systems, San Diego, has imaged more than 95 percent of Mars, with resolution showing features smaller than a tennis court. The Compact Reconnaissance Imaging Spectrometer (CRISM), managed by Johns Hopkins University Applied Physics Laboratory, Laurel, Maryland, also has imaged nearly 98 percent of the planet in multiple visual-light and infrared wavelengths, providing composition information at scales of 100 to 200 yards or meters per pixel.

For more information about MRO, visit:

For more information about NASA’s journey to Mars, visit: www.nasa.gov/topics/journeytomars

Videos: “From Here to the Stars” interview series by the Tennessee Valley Interstellar Workshop

The Tennessee Valley Interstellar Workshop  (TVIW) recently initiated a Youtube video series titled, From Here to the Stars, that consists of interviews with scientists and leading thinkers in the area of interstellar travel. Here are the first four entries in the series:

In Episode 1, Stephen Euin Cobb, Host of “Future and You” podcast, interviews Marc G. Millis, Founder and Director of Tau Zero Foundation, in association with Tennessee Valley Interstellar Workshop (Les Johnson, Executive Producer).

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In Episode 2, Stephen Euin Cobb, Host of “Future and You” podcast, interviews Dr. Louis D. Friedman, Co-Founder of The Planetary Society with Carl Sagan and Bruce C. Murray and Planetary Society Executive Director Emeritus, in association with Tennessee Valley Interstellar Workshop (Les Johnson, Executive Producer).

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In Episode 3, Stephen Euin Cobb, Host of “Future and You” podcast, interviews Dr. Philip Lubin, a professor of Physics at the University of California, Santa Barbara and a co-recipient of the 2006 Gruber Prize in Cosmology along with the COBE science team for their groundbreaking work in cosmology. This series is produced in association with Tennessee Valley Interstellar Workshop (Les Johnson, Executive Producer).

See the see DEEP-IN webpage for more about the work of Lubin’s group at UCSB on “Directed Energy Interstellar Precursors”.

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In Episode 4, Stephen Euin Cobb, Host of “Future and You” podcast, interviews Dr. Gregory L. Matloff, Emeritus Associate and Adjunct Associate Professor of Physics at New York City College of Technology (NYCCT), Fellow of the British interplanetary Society, and Hayden Associate at the American Museum of Natural History. This series is produced in association with Tennessee Valley Interstellar Workshop (Les Johnson, Executive Producer).

Dawn: A mountain on Ceres comes into focus + A mission review

Marc Rayman, the Dawn mission Chief Engineer and Mission Director, writes an interesting review of the project: Dear Indawnbitably Successful Readers – Dawn Blog

And here is a new science report today:

Dawn’s First Year at Ceres: A Mountain Emerges 

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The mysterious mountain Ahuna Mons is seen in this mosaic of images from NASA’s Dawn spacecraft. Dawn took these images from its lowest-altitude orbit. Image Credit: NASA/JPL-Caltech/UCLA/MPS/DLR/IDA
One year ago, on March 6, 2015, NASA’s Dawn spacecraft slid gently into orbit around Ceres, the largest body in the asteroid belt between Mars and Jupiter.  Since then, the spacecraft has delivered a wealth of images and other data that open an exciting new window to the previously unexplored dwarf planet.

“Ceres has defied our expectations and surprised us in many ways, thanks to a year’s worth of data from Dawn. We are hard at work on the mysteries the spacecraft has presented to us,” said Carol Raymond, deputy principal investigator for the mission, based at NASA’s Jet Propulsion Laboratory, Pasadena, California.

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This side-perspective view of Ceres’ mysterious mountain Ahuna Mons was made with images from NASA’s Dawn spacecraft. Dawn took these images from its low-altitude mapping orbit, 240 miles (385 kilometers) above the surface, in December 2015. The resolution of the component images is 120 feet (35 meters) per pixel. A 3-D (anaglyph) view is also available
Among Ceres’ most enigmatic features is a tall mountain the Dawn team named Ahuna Mons. This mountain appeared as a small, bright-sided bump on the surface as early as February 2015 from a distance of 29,000 miles (46,000 kilometers), before Dawn was captured into orbit. As Dawn circled Ceres at increasingly lower altitudes, the shape of this mysterious feature began to come into focus. From afar, Ahuna Mons looked to be pyramid-shaped, but upon closer inspection, it is best described as a dome with smooth, steep walls.

Dawn’s latest images of Ahuna Mons, taken 120 times closer than in February 2015, reveal that this mountain has a lot of bright material on some of its slopes, and less on others. On its steepest side, it is about 3 miles (5 kilometers) high. The mountain has an average overall height of 2.5 miles (4 kilometers). It rises higher than Washington’s Mount Rainier and California’s Mount Whitney.

Scientists are beginning to identify other features on Ceres that could be similar in nature to Ahuna Mons, but none is as tall and well-defined as this mountain.

“No one expected a mountain on Ceres, especially one like Ahuna Mons,” said Chris Russell, Dawn’s principal investigator at the University of California, Los Angeles. “We still do not have a satisfactory model to explain how it formed.”

About 420 miles (670 kilometers) northwest of Ahuna Mons lies the now-famous Occator Crater. Before Dawn arrived at Ceres, images of the dwarf planet from NASA’s Hubble Space Telescope showed a prominent bright patch on the surface. As Dawn approached Ceres, it became clear that there were at least two spots with high reflectivity. As the resolution of images improved, Dawn revealed to its earthly followers that there are at least 10 bright spots in this crater alone, with the brightest area on the entire body located in the center of the crater. It is not yet clear whether this bright material is the same as the material found on Ahuna Mons.

“Dawn began mapping Ceres at its lowest altitude in December, but it wasn’t until very recently that its orbital path allowed it to view Occator’s brightest area. This dwarf planet is very large and it takes a great many orbital revolutions before all of it comes into view of Dawn’s camera and other sensors,” said Marc Rayman, Dawn’s chief engineer and mission director at JPL.

Researchers will present new images and other insights about Ceres at the 47th Lunar and Planetary Science Conference, during a press briefing on March 22 in The Woodlands, Texas.

When it arrived at Ceres 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. The mission conducted extensive observations of Vesta in 2011-2012.

Dawn’s mission is managed by JPL for NASA’s Science Mission Directorate in Washington. Dawn is a project of the directorate’s Discovery Program, managed by NASA’s Marshall Space Flight Center in Huntsville, Alabama. UCLA is responsible for overall Dawn mission science. Orbital ATK Inc., in Dulles, Virginia, designed and built the spacecraft. The German Aerospace Center, Max Planck Institute for Solar System Research, Italian Space Agency and Italian National Astrophysical Institute are international partners on the mission team. For a complete list of mission participants, visit: http://dawn.jpl.nasa.gov/mission

More information about Dawn is available at the following sites:

 

Video: ‘Space to Ground’ report on the ISS – March.4.16

Here is the latest of NASA’s weekly Space to Ground reports on recent activities related to the Int. Space Station:

Video: Planetary Society’s LightSail 2 tests its sail

Here is an update on the Planetary Society’s LightSail 2 project: Meet LightSail 2, The Planetary Society’s new solar sailing CubeSat – The Planetary Society.

Last June, LightSail 1 successfully tested the deployment of its sail in orbit. The goal of LightSail 2 is to achieve propulsion from the pressure of sunlight. It is scheduled to go to space in early 2017 on a SpaceX Falcon Heavy.

Here is a video of a LightSail 2 deployment test: