Spirit Mars Rover news

To join today’s post on the next generation of Mars rovers, here is news hot from the inbox on a current Mars rover.

The release (not from the link):

NASA Rover Finds Clue to Mars’ Past and Environment for Life

PASADENA, Calif., June 3 /PRNewswire-USNewswire/ — Rocks examined by NASA’s Spirit Mars Rover hold evidence of a wet, non-acidic ancient environment that may have been favorable for life. Confirming this mineral clue took four years of analysis by several scientists.

(Logo: http://www.newscom.com/cgi-bin/prnh/20081007/38461LOGO)

An outcrop that Spirit examined in late 2005 revealed high concentrations of carbonate, which originates in wet, near-neutral conditions, but dissolves in acid. The ancient water indicated by this find was not acidic.

NASA’s rovers have found other evidence of formerly wet Martian environments. However the data for those environments indicate conditions that may have been acidic. In other cases, the conditions were definitely acidic, and therefore less favorable as habitats for life.

Laboratory tests helped confirm the carbonate identification. The findings were published online Thursday, June 3 by the journal Science.

“This is one of the most significant findings by the rovers,” said Steve Squyres of Cornell University in Ithaca, N.Y. Squyres is principal investigator for the Mars twin rovers, Spirit and Opportunity, and a co-author of the new report. “A substantial carbonate deposit in a Mars outcrop tells us that conditions that could have been quite favorable for life were present at one time in that place.”

Spirit inspected rock outcrops, including one scientists called Comanche, along the rover’s route from the top of Husband Hill to the vicinity of the Home Plate plateau which Spirit has studied since 2006. Magnesium iron carbonate makes up about one-fourth of the measured volume in Comanche. That is a tenfold higher concentration than any previously identified for carbonate in a Martian rock.

“We used detective work combining results from three spectrometers to lock this down,” said Dick Morris, lead author of the report and a member of a rover science team at NASA’s Johnson Space Center in Houston. “The instruments gave us multiple, interlocking ways of confirming the magnesium iron carbonate, with a good handle on how much there is.”

Massive carbonate deposits on Mars have been sought for years without much success. Numerous channels apparently carved by flows of liquid water on ancient Mars suggest the planet was formerly warmer, thanks to greenhouse warming from a thicker atmosphere than exists now. The ancient, dense Martian atmosphere was probably rich in carbon dioxide, because that gas makes up nearly all the modern, very thin atmosphere.

It is important to determine where most of the carbon dioxide went. Some theorize it departed to space. Others hypothesize that it left the atmosphere by the mixing of carbon dioxide with water under conditions that led to forming carbonate minerals. That possibility, plus finding small amounts of carbonate in meteorites that originated from Mars, led to expectations in the 1990s that carbonate would be abundant on Mars. However, mineral-mapping spectrometers on orbiters since then have found evidence of localized carbonate deposits in only one area, plus small amounts distributed globally in Martian dust.

Morris suspected iron-bearing carbonate at Comanche years ago from inspection of the rock with Spirit’s Moessbauer Spectrometer, which provides information about iron-containing minerals. Confirming evidence from other instruments emerged slowly. The instrument with the best capability for detecting carbonates, the Miniature Thermal Emission Spectrometer, had its mirror contaminated with dust earlier in 2005, during a wind event that also cleaned Spirit’s solar panels.

“It was like looking through dirty glasses,” said Steve Ruff of Arizona State University in Tempe, Ariz., another co-author of the report. “We could tell there was something very different about Comanche compared with other outcrops we had seen, but we couldn’t tell what it was until we developed a correction method to account for the dust on the mirror.”

Spirit’s Alpha Particle X-ray Spectrometer instrument detected a high concentration of light elements, a group including carbon and oxygen, that helped quantify the carbonate content.

The rovers landed on Mars in January 2004 for missions originally planned to last three months. Spirit has been out of communication since March 22 and is in a low-power hibernation status during Martian winter. Opportunity is making steady progress toward a large crater, Endeavour, which is about seven miles away.

NASA’s Jet Propulsion Laboratory, Pasadena, manages the Mars Exploration Rovers for the agency’s Science Mission Directorate in Washington. For more information about the rovers, visit:

http://www.nasa.gov/rovers

Photo:  http://www.newscom.com/cgi-bin/prnh/20081007/38461LOGO
PRN Photo Desk photodesk@prnewswire.com
Source: NASA

Web Site:  http://www.nasa.gov/

Kepler launched

News from NASA.

The release:

NASA’s Kepler Mission Rockets to Space in Search of Other Earths

CAPE CANAVERAL, Fla., March 7 /PRNewswire-USNewswire/ — NASA’s Kepler mission successfully launched into space from Cape Canaveral Air Force Station, Fla., aboard a United Launch Alliance Delta II at 10:49 p.m. EST, Friday. Kepler is designed to find the first Earth-size planets orbiting stars at distances where water could pool on the planet’s surface. Liquid water is believed to be essential for the formation of life.

(Logo: /Photo: http://www.newscom.com/cgi-bin/prnh/20081007/38461LOGO )

“It was a stunning launch,” said Kepler Project Manager James Fanson of NASA’s Jet Propulsion Laboratory in Pasadena, Calif. “Our team is thrilled to be a part of something so meaningful to the human race — Kepler will help us understand if our Earth is unique or if others like it are out there.”

Engineers acquired a signal from Kepler at 12:11 a.m. Saturday, after it separated from its spent third-stage rocket and entered its final sun-centered orbit, trailing 950 miles behind Earth. The spacecraft is generating its own power from its solar panels.

“Kepler now has the perfect place to watch more than 100,000 stars for signs of planets,” said William Borucki, the mission’s science principal investigator at NASA’s Ames Research Center at Moffett Field, Calif. Borucki has worked on the mission for 17 years. “Everyone is very excited as our dream becomes a reality. We are on the verge of learning if other Earths are ubiquitous in the galaxy.”

Engineers have begun to check Kepler to ensure it is working properly, a process called “commissioning” that will take about 60 days. In about a month or less, NASA will send up commands for Kepler to eject its dust cover and make its first measurements. After another month of calibrating Kepler’s single instrument, a wide-field charge-couple device camera, the telescope will begin to search for planets.

The first planets to roll out on the Kepler “assembly line” are expected to be the portly “hot Jupiters” — gas giants that circle close and fast around their stars. NASA’s Hubble and Spitzer space telescopes will be able to follow up with these planets and learn more about their atmospheres. Neptune-size planets will most likely be found next, followed by rocky ones as small as Earth. The true Earth analogs — Earth-sized planets orbiting stars like our sun at distances where surface water, and possibly life, could exist — would take at least three years to discover and confirm. Ground-based telescopes also will contribute to the mission by verifying some of the finds.

In the end, Kepler will give us our first look at the frequency of Earth-size planets in our Milky Way galaxy, as well as the frequency of Earth-size planets that could theoretically be habitable.

“Even if we find no planets like Earth, that by itself would be profound. It would indicate that we are probably alone in the galaxy,” said Borucki.

As the mission progresses, Kepler will drift farther and farther behind Earth in its orbit around the sun. NASA’s Spitzer Space Telescope, which was launched into the same orbit more than five years ago, is now more than 62 million miles behind Earth.

Kepler is a NASA Discovery mission. Ames is the home organization of the science principal investigator and is responsible for the ground system development, mission operations and science data analysis. JPL manages the Kepler mission development. Ball Aerospace & Technologies Corp. of Boulder, Colo., is responsible for developing the Kepler flight system and supporting mission operations. NASA’s Launch Services Program at NASA’s Kennedy Space Center, Fla., managed the launch service including payload integration and certifying the Delta II launch vehicle for NASA’s use.

For more information about the Kepler mission, visit:

http://www.nasa.gov/kepler

Photo:  http://www.newscom.com/cgi-bin/prnh/20081007/38461LOGO
AP Archive:  http://photoarchive.ap.org/
PRN Photo Desk photodesk@prnewswire.com
Source: NASA
   

Web Site:  http://www.nasa.gov/

NASA announces new Jupiter mission

Sounds cool.

The release:

NASA Prepares for New Juno Mission to Jupiter

WASHINGTON, Nov. 24 /PRNewswire-USNewswire/ — NASA is officially moving forward on a mission to conduct an unprecedented, in-depth study of Jupiter.

(Logo:  http://www.newscom.com/cgi-bin/prnh/20081007/38461LOGO )

Called Juno, the mission will be the first in which a spacecraft is placed in a highly elliptical polar orbit around the giant planet to understand its formation, evolution and structure. Underneath its dense cloud cover, Jupiter safeguards secrets to the fundamental processes and conditions that governed our early solar system.

“Jupiter is the archetype of giant planets in our solar system and formed very early, capturing most of the material left after the sun formed,” said Scott Bolton, Juno principal investigator from the Southwest Research Institute in San Antonio. “Unlike Earth, Jupiter’s giant mass allowed it to hold onto its original composition, providing us with a way of tracing our solar system’s history.”

The spacecraft is scheduled to launch aboard an Atlas rocket from Cape Canaveral, Fla., in August 2011, reaching Jupiter in 2016. The spacecraft will orbit Jupiter 32 times, skimming about 3,000 miles over the planet’s cloud tops for approximately one year. The mission will be the first solar powered spacecraft designed to operate despite the great distance from the sun.

“Jupiter is more than 400 million miles from the sun or five times further than Earth,” Bolton said. “Juno is engineered to be extremely energy efficient.”

The spacecraft will use a camera and nine science instruments to study the hidden world beneath Jupiter’s colorful clouds. The suite of science instruments will investigate the existence of an ice-rock core, Jupiter’s intense magnetic field, water and ammonia clouds in the deep atmosphere, and explore the planet’s aurora borealis.

“In Greek and Roman mythology, Jupiter’s wife Juno peered through Jupiter’s veil of clouds to watch over her husband’s mischief,” said Professor Toby Owen, co-investigator at the University of Hawaii in Honolulu. “Our Juno looks through Jupiter’s clouds to see what the planet is up to, not seeking signs of misbehavior, but searching for whispers of water, the ultimate essence of life.”

Understanding the formation of Jupiter is essential to understanding the processes that led to the development of the rest of our solar system and what the conditions were that led to Earth and humankind. Similar to the sun, Jupiter is composed mostly of hydrogen and helium. A small percentage of the planet is composed of heavier elements. However, Jupiter has a larger percentage of these heavier elements than the sun.

“Juno’s extraordinarily accurate determination of the gravity and magnetic fields of Jupiter will enable us to understand what is going on deep down in the planet,” said Professor Dave Stevenson, co-investigator at the California Institute of Technology in Pasadena. “These and other measurements will inform us about how Jupiter’s constituents are distributed, how Jupiter formed and how it evolved, which is a central part of our growing understanding of the nature of our solar system.”

Deep in Jupiter’s atmosphere, under great pressure, hydrogen gas is squeezed into a fluid known as metallic hydrogen. At these great depths, the hydrogen acts like an electrically conducting metal which is believed to be the source of the planet’s intense magnetic field. Jupiter also may have a rocky solid core at the center.

“Juno gives us a fantastic opportunity to get a picture of the structure of Jupiter in a way never before possible,” said James Green, director of NASA’s Planetary Division at NASA Headquarters in Washington. “It will allow us to take a giant step forward in our understanding on how giant planets form and the role that plays in putting the rest of the solar system together.”

The Juno mission is the second spacecraft designed under NASA’s New Frontiers Program. The first was the Pluto New Horizons mission, launched in January 2006 and scheduled to reach Pluto’s moon Charon in 2015. The program provides opportunities to carry out several medium-class missions identified as top priority objectives in the Decadal Solar System Exploration Survey, conducted by the Space Studies Board of the National Research Council in Washington.

NASA’s Jet Propulsion Laboratory in Pasadena, Calif., manages the Juno mission. Lockheed Martin of Denver is building the spacecraft. The Italian Space Agency is contributing an infrared spectrometer instrument and a portion of the radio science experiment.

For more information about the Juno mission, visit:

http://juno.nasa.gov/

Photo:  http://www.newscom.com/cgi-bin/prnh/20081007/38461LOGO
AP Archive:  http://photoarchive.ap.org/
PRN Photo Desk photodesk@prnewswire.com
Source: NASA
   

Web Site:  http://www.nasa.gov/

NASA tests new deep space communication

Successfully and based on the structure of the internet. Pretty cool stuff.

The release from about ten minutes ago:

NASA Successfully Tests First Deep Space Internet

PASADENA, Calif., Nov. 18 /PRNewswire-USNewswire/ — NASA has successfully tested the first deep space communications network modeled on the Internet.

(Logo:  http://www.newscom.com/cgi-bin/prnh/20081007/38461LOGO )

Working as part of a NASA-wide team, engineers from NASA’s Jet Propulsion Laboratory in Pasadena, Calif., used software called Disruption-Tolerant Networking, or DTN, to transmit dozens of space images to and from a NASA science spacecraft located about 20 million miles from Earth.

“This is the first step in creating a totally new space communications capability, an interplanetary Internet,” said Adrian Hooke, team lead and manager of space-networking architecture, technology and standards at NASA Headquarters in Washington.

NASA and Vint Cerf, a vice president at Google Inc., in Mountain View, Calif., partnered 10 years ago to develop this software protocol. The DTN sends information using a method that differs from the normal Internet’s Transmission-Control Protocol/Internet Protocol, or TCP/IP, communication suite, which Cerf co-designed.

The Interplanetary Internet must be robust to withstand delays, disruptions and disconnections in space. Glitches can happen when a spacecraft moves behind a planet, or when solar storms and long communication delays occur. The delay in sending or receiving data from Mars takes between three-and-a-half to 20 minutes at the speed of light.

Unlike TCP/IP on Earth, the DTN does not assume a continuous end-to-end connection. In its design, if a destination path cannot be found, the data packets are not discarded. Instead, each network node keeps the information as long as necessary until it can communicate safely with another node. This store-and-forward method, similar to basketball players safely passing the ball to the player nearest the basket means information does not get lost when no immediate path to the destination exists. Eventually, the information is delivered to the end user.

“In space today, an operations team must manually schedule each link and generate all the commands to specify which data to send, when to send it, and where to send it,” said Leigh Torgerson, manager of the DTN Experiment Operations Center at JPL. “With standardized DTN, this can all be done automatically.”

Engineers began a month-long series of DTN demonstrations in October. Data were transmitted using NASA’s Deep Space Network in demonstrations occurring twice a week. Engineers use NASA’s Epoxi spacecraft as a Mars data-relay orbiter. Epoxi is on a mission to encounter Comet Hartley 2 in two years. There are 10 nodes on this early interplanetary network. One is the Epoxi spacecraft itself and the other nine, which are on the ground at JPL, simulate Mars landers, orbiters and ground mission-operations centers.

This month-long experiment is the first in a series of planned demonstrations to qualify the technology for use on a variety of upcoming space missions. In the next round of testing, a NASA-wide demonstration using new DTN software loaded on board the International Space Station is scheduled to begin next summer.

In the next few years, the Interplanetary Internet could enable many new types of space missions. Complex missions involving multiple landed, mobile and orbiting spacecraft will be far easier to support through the use of the Interplanetary Internet. It also could ensure reliable communications for astronauts on the surface of the moon.

The Deep Impact Networking Experiment is sponsored by the Space Communications and Navigation Office in NASA’s Space Operations Mission Directorate in Washington. NASA’s Science Mission Directorate and Discovery Program in Washington provided experimental access to the Epoxi spacecraft. The Epoxi mission team provided critical support throughout development and operations.

Photo:  http://www.newscom.com/cgi-bin/prnh/20081007/38461LOGO
AP Archive:  http://photoarchive.ap.org/
PRN Photo Desk photodesk@prnewswire.com
Source: NASA
 

Web Site:  http://www.nasa.gov/

NASA’s Kepler Spacecraft closer to launch

The spaceship just passed an extreme temperature test.

The release:

NASA’s Kepler Spacecraft Baked and Ready for More Tests

PASADENA, Calif., Sept. 23 /PRNewswire-FirstCall/ — NASA’s planet-hunting Kepler mission, scheduled to launch in 2009, has survived an extreme temperature test.

(Photo: http://www.newscom.com/cgi-bin/prnh/20080923/LATU531)

The thermal vacuum test is part of a series of environmental tests the spacecraft will undergo before it blasts into space aboard a Delta II rocket from the Cape Canaveral Air Force Station, Fla.

“Kepler functioned extremely well at the intense temperatures it will encounter in space,” said James Fanson, Kepler project manager at NASA’s Jet Propulsion Laboratory, Pasadena, Calif.

The test, which was performed at Ball Aerospace & Technologies Corp. in Boulder, Colo., simulates the vacuum of space, and the extreme temperatures Kepler will face once launched. The spacecraft is tucked into a vacuum chamber and surrounded by a cold shroud to mimic the deep chill of space. One side of the spacecraft — the side with solar panels — is then baked as if it were being heated by the sun.

The goal is to make sure that the spacecraft and its detectors operate properly in the space-like environment. An electromagnetic compatibility test, to ensure Kepler’s electronics are sound, will begin soon.

Kepler will monitor 100,000 stars, searching for signs of planets — including ones as small as or smaller than Earth. To date, no Earth-sized planet has been discovered.

“The results of these tests are now being used to prepare for the science operations that will start after the spacecraft launches and undergoes in-orbit checkout,” said Bill Borucki of NASA Ames Research Center, Moffett Field, Calif., the science principal investigator for the Kepler Mission.

Kepler is a NASA Discovery mission. In addition to being the home organization of the science principal investigator, NASA Ames Research Center is responsible for the ground system development, mission operations and science data analysis. Kepler mission development is managed by JPL. Ball Aerospace & Technologies Corp. is responsible for developing the Kepler flight system and supporting mission operations.

More information about the Kepler mission is at http://kepler.nasa.gov/. More information about extrasolar planets and NASA’s planet-finding program is at http://planetquest.jpl.nasa.gov/.

Photo:  NewsCom:  http://www.newscom.com/cgi-bin/prnh/20080923/LATU531
AP Archive:  http://photoarchive.ap.org/
AP PhotoExpress Network:  PRN11
PRN Photo Desk, photodesk@prnewswire.com
Source: Ball Aerospace & Technologies Corp.
   

Web site:  http://www.ballaerospace.com/
http://kepler.nasa.gov/
http://planetquest.jpl.nasa.gov/