Showing posts with label NASA. Show all posts
Showing posts with label NASA. Show all posts

NASA Asteroid Missions


Asteroid day is celebrated every day at NASA. We are constantly gazing to the sky, from expeditions to asteroids in our solar system – some of which even return samples to Earth – to attempts to locate, track, and monitor near-Earth objects and safeguard our planet from possible impact dangers.


Several ambitious missions to investigate unusual asteroids will be launched in the coming years. 


In October and November 2021 NASA will be launching, 




    • Lucy is the Trojan Asteroids' First Mission
    • These primordial entities may contain crucial insights about the solar system's past, as well as the beginnings of biological stuff on Earth.



    • NASA has entrusted the Double Asteroid Redirection Test (DART) mission to the Johns Hopkins Applied Physics Laboratory (APL), with assistance from several NASA centers including the Jet Propulsion Laboratory (JPL), Goddard Space Flight Center (GSFC), Johnson Space Center (JSC), Glenn Research Center (GRC), and Langley Research Center (LaRC).
    • DART is a planetary defense-driven test of technology aimed at preventing an asteroid from colliding with Earth. DART will be the first time a kinetic impactor will be used to alter an asteroid's velocity in space. 
    • The DART project is now in Phase C, directed by APL and administered by Marshall Space Flight Center for NASA's Planetary Defense Coordination Office and the Science Mission Directorate's Planetary Science Division at NASA Headquarters in Washington, DC, under NASA's Solar System Exploration Program.


Followed by,



    • The Psyche mission will go to a rare metal asteroid that orbits the Sun between Mars and Jupiter. 
    • The asteroid Psyche is unusual in that it seems to be the exposed nickel-iron core of an early planet, one of our solar system's building components.


    • OSIRIS-REx has arrived at the near-Earth asteroid Bennu and is bringing back a tiny sample for examination. 
    • The mission took off from Cape Canaveral Air Force Station on September 8, 2016. 
    • In 2018, the spacecraft arrived on Bennu, and in 2023, it will return a sample to Earth.




    • It has verified infrared sightings of over 39,100 objects in our solar system to far.
    • From December 2009 to February 2011, NASA's Wide-field Infrared Survey Explorer (WISE) was a NASA infrared-wavelength astronomical space telescope. 
    • The spacecraft was revived in September 2013, renamed NEOWISE, and given a new mission: to help NASA in identifying and characterizing the population of near-Earth objects (NEO).


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International Space Station Sun Transit



The International Space Station, which has a crew of seven onboard, is silhouetted in this composite picture created from seven frames as it transits the Sun at approximately five miles per second on Friday, June 25.


Image Credit & Courtesy of: NASA.gov / Joel Kowsky


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Mars Robotics - Robotic Exploration of Mars



NASA's Mars Exploration Program (MEP) is managed by JPL. For many years, this program has been conducting a series of robotic missions to investigate Mars. 


  • The success of the Mars Pathfinder, Mars Exploration Rover, and Mars Science Laboratory missions has shown that autonomous rovers can effectively and efficiently explore the surface of Mars and collect scientific data in small regions. 
  • As a consequence, the MEP has created an ambitious long-term strategy for in situ exploration based on a consensus among top Mars scientists. 
  • The hunt for past or current life on Mars is the highest priority objective. 


For instance, a JPL website addresses the question, “Why Explore Mars?” 


  • Mars has the most pleasant environment in the solar system after Earth. 
  • It was once so welcoming that it might have supported primitive, bacteria-like life. =
  • Outflow channels and other geologic structures on Mars' surface offer sufficient evidence that liquid water flowed billions of years ago. 
  • Although liquid water may exist deep under Mars' surface, the temperature is presently too low and the atmosphere is too thin for liquid water to exist at the surface. 

What caused the climate on Mars to change? 

Were the prerequisites for the emergence of life ever exist on Mars? 

Is it possible that microorganisms in the subsurface are still living today? 

 

These are the kinds of questions that motivate us to go to Mars. 

Mars' environment has clearly cooled significantly.... 



We must initially ask the following questions when we begin to explore the cosmos and seek for planets in other solar systems: 


Is there evidence of life on another planet in our solar system? 

What are the bare minimum requirements for the emergence of life? 


Four topics were prioritized by the Mars Exploration Program 


  1. Look for traces of a previous existence. 
  2. Investigate hydrothermal environments. (The chances of finding evidence of past and current life have considerably increased.) 
  3. Look for the current moment. 
  4. Investigate the development of Mars. 


The hunt for proof of previous life was the main short-term aim. If hydrothermal vents were identified (which they haven't yet), the search would be narrowed down to those areas. 

The hunt for current life would “follow on from previous orbiting or landing missions discovering that current Mars conditions have the capacity to sustain life.” 

Only if the... presently accepted theories for Mars' climatic history are wrong will the subject of Martian evolution be highlighted. 


If future missions show that there is no convincing evidence of wet conditions on ancient Mars involving standing bodies of water, as has been interpreted from orbital remote sensing to date, the program's current focus on the search for surface habitats will be lowered significantly — unless, of course, liquid water is discovered on or near the surface of Mars today. 

With this unexpected finding would arise the conundrum of how the terrestrial planets developed so differently, despite their striking resemblance. 

Liquid water, on the other hand, is unstable at Mars' surface temperatures and pressures. 

As a result, standing pools of liquid water cannot exist on or near Mars' surface. 

Liquid water might theoretically exist far under the surface, where temperatures are greater, and liquid water under pressure could sometimes rush up to the top owing to a subterranean event, where it would rapidly freeze. 

                                                                

The loss mechanisms and sinks for water and CO2 on Mars would be studied throughout time, as well as comparisons of the parallels and differences between the three terrestrial planets: 


Venus, Earth, and Mars. More than 130 terrestrial and planetary scientists gathered at Jackson Hole, Wyoming, to study early Mars. 

The report's primary topic was the hunt for life on Mars. In their 26-page study, the term "life" appears 119 times, or almost five times each page. 

According to the report's introduction, "perhaps the single most compelling reason scientists find this early period of Martian geologic history so compelling is that its dynamic character may have given rise to conditions suitable for the development of life, the creation of habitable environments for that life to colonize, and the subsequent preservation of evidence of those early environments in the geologic record." 



“Did life emerge on early Mars?” was listed as one of the three “top scientific questions linked to early Mars.” 

“The issue of Martian life contains basically three fundamental aspects,” the study continues. 



  • The first was the idea that Mars might have had its own separate genesis of life. 
  • The second was the possibility of life developing on one planet and then being transported to another via impact ejection and gravitational capture (i.e., panspermia). 
  • The third looked at the possibility of life on Mars having survived and developed after its first appearance. The study goes on to say that “how life starts anyplace remains a basic unsolved mystery,” and that “the closeness of Earth and Mars raises uncertainty as to whether Earth and Mars had genuinely separate beginnings of life.” 


Microorganisms may have been transferred between the two worlds as a result of meteoritic collisions, such as those that brought Martian meteorites to Earth. 

In the distant geologic past, impact events were much more common and significant, including at the time when life started on Earth. 

As a result, it's impossible to say if the finding of life on Mars entails the discovery of a genuinely separate genesis of life. 

Because liquid water is thought to be a required (but not sufficient) prerequisite for life to develop from inanimate materials, the Mars scientific community puts a high priority on finding evidence of liquid water's previous effect on the surface (it cannot exist there under present conditions). 

The hunt for evidence of previous circumstances that might have supported life on Mars is still a major focus of the mission. 


The key issue for Mars exploration, according to the MEP, is: Is there life on Mars? 


Among the many discoveries we've made about Mars, one stands out above the rest: 

the possibility of liquid water on Mars, either in the distant past or now in the subsurface. 

Water is essential because life exists nearly everywhere on Earth where there is water. 

If Mars previously had liquid water, and if it still does now, it's intriguing to speculate about whether microscopic life might have evolved on its surface. 



Is there any proof of life on the earth in the past? 

Is it possible that any of these small live organisms survive today? 


Consider how thrilling it would be to say, "Yes!" 


  • The first science goal is to find out whether life has ever existed on Mars. 
  • NASA will need to undertake multiple missions over the next several decades to determine if life ever existed on Mars. 
  • Similarly, the hunt for life lies at the heart of NASA's exploration of other planets in the solar system and beyond. 
  • A hunt for life on Titan, Saturn's moon, and the Search for Extraterrestrial Intelligence (SETI) using radio telescopes are among them. 

The focus on life in the NASA community has swayed a number of otherwise competent and even prominent scientists to develop programs, papers, and reports to analyze, hypothesize, and imagine the possibility of liquid water and life on other planetary bodies, with a particular focus on Mars—and the press has exaggerated these occasional musings. 

Mars scientists are under a lot of pressure to discover implications for water and life in their research. 


An interesting article reports on an interview with Steve Squyres, the project scientist for the Mars Exploration Rovers mission. 


The following are two extracts from the article: 

According to reports, Squyers believes the rovers would provide answers to two questions: 

"Are we alone in the universe?" and "How did life come to be?" 


Most significantly, they've discovered signs of water on Mars. There is life where there is water. It's hard to believe Squyres really stated this. 


How can the media say such ludicrous things? 

What proof is there that a planet with liquid water had life at some point? 

Isn't it possible to tell the difference between essential and sufficient? 

Although water is essential for life, is it sufficient? 

There is no proof that it is. And who in their right mind thinks the MER rovers will provide a solution to the issue of how life forms? 


This isn't science at all. It's the worst kind of pseudoscience. 

In regular news releases ascribed to renowned and competent space experts, the Internet is full with crazy erroneous claims. 


P.S ~ When did science go from proving hypotheses with measurements, cautious understated conclusions, and carefully verifying ideas before going public—to wild untested statements, baseless claims, and repeated press releases reporting nonsense?


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Mars Exploration And The Search For Life



The Apollo human trips to the Moon must be considered one of mankind's greatest technical accomplishments, especially given the rudimentary electronics available at the time. 


  • That was undoubtedly the pinnacle of NASA's accomplishments. 
  • Since then, NASA has been debating what should happen next in terms of people in space.
  • There seems to have been a strong desire to get humans into space, which led to the creation of the Space Shuttle. 



While it is true that any human mission in space requires access, the problems with the Shuttle were that, 

(i) the development and operation of the Shuttle required so much funding that there wasn't much left over to support what humans would do once they did get access to space, and 

(ii) the Shuttle's reliability deteriorated over time, until the main goal seemed to be merely to land sat. 



Following the Shuttle, NASA began on the Space Station, which, like the Shuttle, proved to be a money drain while delivering even less value. 

Michael Griffin was the NASA Administrator at the time, and his perspective aligned with Robert Zubrin's: 


  • The NASA budget allocates funding to its constituencies for technology development in the belief that if enough technical work is done, the building blocks for missions will be available (Zubrin 2014). 
  • As Zubrin put it, "technology and hardware components are created in accordance with the desires of different technical groups" under this manner. 


These initiatives are therefore justified by the premise that they may be helpful in the future when large-scale flying programs are restarted. 


  • In theory, if executed intelligently and successfully, this method has considerable value. 
  • However, we know from experience that establishing and maintaining a link between technology development and mission requirements is difficult. 



Furthermore, the requirement to connect technology to particular objectives may suffocate innovation and hinder development on higher-paying technologies. 


  • Griffin, unlike his predecessors, was committed to what Zubrin referred to as the Apollo Mode: first, a destination for human space travel is selected. 
  • After that, a strategy for achieving the goal is devised. Following that, technologies and designs are created to put the strategy into action. 
  • The mission is then flown once these designs have been constructed. 


Griffin's strategy was to choose a particular destination and devote a significant portion of NASA's budget to developing technologies to get there. 


  • By rapidly phasing out the Shuttle and the Space Station and diverting NASA Center technology money to shorter-term initiatives directly meeting the requirements of his destination-driven mission idea, his goal was to establish a pool of resources inside NASA for executing his vision. Griffin made the decision to return to the Moon. 
  • He most likely postponed a trip to Mars because the finances were just not available. 


An interview with Griffin may provide some insight into Griffin's thoughts (2010). 


  • He said in the interview that the Obama administration's strategy "does not bring us out beyond low Earth orbit in a timely and efficient manner." 
  • Transporting people to the Moon, he said, was an essential step toward ultimately sending humans to Mars. 
  • He also said that "the Moon is fascinating in and of itself." “I believe the experience of learning how to live on another planet just three days from home is extremely valuable...” he said. 
  • Griffin's objective, however, was not able to be realized due to a lack of funding in the NASA budget. 
  • Griffin's Constellation project was hampered by continued funding for the Space Shuttle and the International Space Station. 



Furthermore, after further consideration, the benefit of returning to the Moon seemed to be extremely speculative. 

President Barack Obama canceled the Constellation program in 2010, and NASA seems to have returned to a constituency-driven model since then. 

 

While NASA has made some crazy promises about sending people to Mars in the 2030s, beautiful PowerPoint slides do not seem to be enabling for this trip. 


  • How, where, and when life emerged from inorganic materials is an unanswered question. 
  • One fundamental piece of information we have is that life lived on Earth in a rudimentary form over 3 billion years ago (BYA). 
  • This was discovered in dated strata using fossil remnants of early forms of life. 


What was the method through which lifeless matter gave birth to life in its earliest stages? 

Is there life beyond the solar system or somewhere in the solar system? 



All of these issues are subordinate to the main question: 


  • Is the emergence of life from inanimate matter a probable (or perhaps predictable) process given enough time, a warm environment, liquid water, and a scattering of chemical elements from the lower periodic table? 
  • Some scientists have used logic and creativity to concoct a broad range of possible scenarios for the emergence of life, many of which are based on little evidence. 


To this writer, they seem to be extremely questionable. 


  • Science despises the lack of solutions to critical problems, just as nature despises a vacuum. 
  • As a consequence, scientists have come up with a variety of "explanations" for how life started.
  • There are many articles on livable worlds. Surely, there must be a large number in the different galaxies. But the issue isn't whether there are livable planets; there are. 



What is the likelihood that life would emerge spontaneously on such a planet? 


  • The commonly held idea seems to be that any planetary body with enough heat, water, and a few components would spontaneously develop life. 
  • Given this viewpoint, Mars seems like an obvious location to look for alien life. 



As a result, NASA's exploration missions are primarily focused on looking for life on Mars. 

But how likely is it that life will develop on such a planet?

Is NASA looking for an ephemeral fantasy with a very little chance of occurring?


~ Jai Krishna Ponnappan


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Is NASA On The Lookout For Aliens?





    The hunt for extraterrestrial life is one of NASA's main objectives. 


    NASA has yet to discover any convincing evidence of alien life, but it has long been investigating the solar system and beyond to help us answer basic issues such as whether we are alone in the cosmos. 

    The astrobiology program of the agency studies the origins, development, and dispersion of life beyond Earth. 

    NASA's scientific missions are working together to discover unambiguous evidence of life beyond Earth, from investigating water on Mars to exploring potential "oceans worlds" like Titan and Europa, to searching for biosignatures in the atmospheres of our cosmic neighborhood and planets beyond our solar system. 



    Is there a chance that life exists anywhere else than Earth? 



    There is a chance, if not a certainty, that life exists somewhere other than Earth. Science is motivated by a desire to learn more about the unknown - yet science is ultimately based on evidence, and alien life has yet to be discovered. We will, however, continue our search. 



    Do intelligent extraterrestrials exist? 


    There is no known evidence for sentient life elsewhere, intelligent or otherwise, based on study at the SETI Institute, examination of Martian meteorites, new discoveries of methane inside the Mars atmosphere, and other similar investigations. 

    The hunt for life in the cosmos, on the other hand, is one of NASA's main objectives. 

    NASA is in charge of the US government's hunt for alien life, whether it's here on Earth, on the planets and moons of our solar system, or farther out in space. 



    How does NASA go about looking for life? 


    The hunt for life at NASA is complex. The research approach for NASA's astrobiology program focuses on three fundamental questions: 


      • What is the origin of life and how does it progress? 
      • Is there life somewhere else in the universe? 
      • What methods do we use to look for life in the universe? 

    • Astrobiologists have discovered a plethora of hints to these major issues during the last 50 years. In addition to utilizing missions like the Transiting Exoplanet Survey Satellite (TESS) and the Hubble Space Telescope to look for habitable exoplanets, NASA's hunt for life involves using the Transiting Exoplanet Survey Satellite (TESS) and the Hubble Space Telescope. 
    • Missions such as the forthcoming James Webb Space Telescope will look for biosignatures in the atmospheres of other planets - finding oxygen and carbon dioxide in other planets' atmospheres, for example, may indicate that an exoplanet supports plants and animals in the same way as ours does. 



    Is NASA on the lookout for technosignatures? 


    Technosignatures are a kind of biosignature that is defined as any observable indication of living or dead organisms. 

    • Technosignatures are technological indicators that may be used to infer the presence of intelligent life elsewhere in the cosmos, such as narrow-band radio transmissions or pulsed laser searches for alien intelligence. 


    The terms SETI (Search for Extraterrestrial Intelligence) and technosignatures are often used interchangeably. 


    • NASA funds technosignatures research, but not ground-based radio-telescope searches, owing to NASA's policy of supporting astrophysical research using space-based assets. 
    • NASA also sponsored a Topical Workshops, Symposia, and Conference to create a research agenda to prioritize and direct future theoretical and observational investigations of non-radio technosignatures, as well as to produce a publishable report that can be used to start creating a technosignatures library. 

    Given that a planet may support life for billions of years before intelligent life evolves to create technology that can be detected from other solar systems – our own planet, for example, has only been creating detectable technosignatures for a little over a century – we have a much better chance of finding life if we look for other biosignatures instead of just technosignatures. 



    Is NASA looking for or studying UAPs (Unidentified Aerial Phenomena)?


    NASA does not go out of its way to look for UAPs. NASA, on the other hand, gathers significant data about Earth's atmosphere via our Earth-observing satellites, frequently in cooperation with other international space organizations. 


    • While these data are not intentionally gathered to detect UAPs or extraterrestrial technosignatures, they are publicly accessible and anybody may scan the atmosphere with them. 
    • While NASA does not actively look for UAPs, if they are discovered, it will offer up new scientific topics to investigate. 
    • Scientists from the atmosphere, aerospace, and other fields may all contribute to a better understanding of the phenomena. 


    Exploring the unknown in space is fundamental to our identity.


    Courtesy: NASA.gov


    ~ Jai Krishna Ponnappan

    You may also want to read more about Space Missions and Systems here.


    How Does NASA's Perseverance Rover Take Selfies On Mars?



      The historic photo of the rover next to the Mars Helicopter turned out to be one of the most difficult rover selfies ever shot. 




      The procedure is explained in detail in this video, which also includes additional audio. 





      Have you ever wondered how rovers on Mars snap selfies? 


      NASA's Perseverance rover took the historic April 6, 2021, picture of itself alongside the Ingenuity Mars Helicopter in color video. 

      The sound of the arm's motors spinning was recorded by the rover's entry, descend, and landing microphone as an added bonus. 


      Engineers may use selfies to evaluate the rover's wear and tear. They do, however, inspire a new generation of space aficionados: 


      • Many members of the rover crew may recall a favorite picture that first piqued their interest in NASA. 
      • Vandi Verma, Perseverance's lead engineer for robotic operations at NASA's Jet Propulsion Laboratory in Southern California, stated, "I got into this when I saw a photo from Sojourner, NASA's first Mars rover." 
      • Verma served as a driver for the agency's Opportunity and Curiosity rovers, and she was involved in the first selfie taken by Curiosity on Oct. 31, 2012. 
      • “We had no idea when we snapped that first selfie that these would become so iconic and routine,” she added. 
      • The rover's robotic arm twists and maneuvers to capture the 62 pictures that make up the image, as shown on video from one of Perseverance's navigation cameras. 
      • What it doesn't show is how much effort went into creating the first selfie. Let's take a deeper look. 






      Teamwork. 


      Perseverance's selfie was made possible by a core group of approximately a dozen individuals, including rover drivers, JPL engineers who conducted tests, and camera operations engineers who created the camera sequence, analyzed the pictures, and stitched them together. 


      It took approximately a week to plan out all of the necessary individual instructions. 

      • Everyone was working on “Mars time,” which meant being up in the middle of the night and catching up on sleep throughout the day (a day on Mars is 37 minutes longer than on Earth). 
      • These members of the crew would occasionally forego sleep in order to complete the selfie. JPL collaborated with Malin Space Science Systems (MSSS) in San Diego, which designed and operated the selfie camera. 




      The camera, dubbed WATSON (Wide Angle Topographic Sensor for Operations and eNgineering), is intended for close-up detail pictures of rock textures rather than wide-angle images. 


      • Engineers had to order the rover to snap hundreds of separate pictures to create the selfie since each WATSON image only captures a tiny part of a scene. 
      • Mike Ravine, MSSS's Advanced Projects Manager, stated, "The thing that required the greatest care was putting Ingenuity into the proper position in the selfie." 

      “Considering how tiny it is, I think we did fairly well.” The MSSS image processing experts got to work as soon as the pictures from Mars arrived. 


      • They begin by removing any imperfections produced by dust that has collected on the light sensors of the camera. 
      • They next use software to combine the individual picture frames into a mosaic and smooth out the seams. 
      • Finally, an engineer warps and crops the mosaic to make it seem more like a standard camera picture that the general public is familiar with. 






      Simulations on a computer. 



      Perseverance, like the Curiosity rover (seen taking a selfie in this black-and-white video from March 2020), has a spinning turret at the end of its robotic arm. 


      • The WATSON camera, which remains focused on the rover during selfies while being tilted to record a portion of the landscape, is housed in the turret among other scientific equipment. 
      • The arm serves as a selfie stick in the final result, staying just out of frame. 
      • Perseverance is considerably more difficult to get to video its selfie stick in action than Curiosity. 
      • Perseverance's turret is 30 inches (75 centimeters) wide, compared to Curiosity's 22 inches (55 centimeters). 
      • That's the equivalent of waving a road bike wheel a few millimeters in front of Perseverance's mast, the rover's "head." 
      • JPL developed software to prevent the arm from colliding with the rover. 
      • The engineering team changes the arm trajectory every time a collision is detected in simulations on Earth; the procedure is repeated hundreds of times to ensure the arm motion is safe. 
      • The last instruction sequence brings the robotic arm as near to the rover's body as possible without touching it. 

      Other simulations are performed to verify that the Ingenuity helicopter is properly positioned in the final photo, or that the microphone can catch sound from the robotic arm's motors, for example. 





      Microphone Onboard




      Perseverance has a microphone in its SuperCam instrument in addition to its entrance, descent, and landing microphones. 


      • The microphones are a first for NASA's Mars mission, and audio will be a valuable new tool for rover engineers in the coming years. 
      • It may be used to give crucial information about whether something is functioning properly, among other things. 
      • Engineers used to have to make do with listening to a test rover on Earth. 


      “It's like your car: even if you're not a technician, you may hear an issue before you know there's a problem,” Verma said. 


      The humming engines sound strangely melodic when echoing through the rover's chassis, despite the fact that they haven't heard anything alarming thus yet. 





      More Information about the Mission. 



      • Astrobiology, particularly the hunt for evidence of ancient microbial life, is a major goal for Perseverance's mission on Mars. 
      • The rover will study the planet's geology and climatic history, lay the path for human exploration of Mars, and be the first mission to gather and store Martian rock and regolith (broken rock and dust). 
      • Following NASA missions, in collaboration with the European Space Agency (ESA), spacecraft would be sent to Mars to collect these sealed samples from the surface and return them to Earth for further study. 


      The Mars 2020 Perseverance mission is part of NASA's Moon to Mars exploration strategy, which includes Artemis lunar missions to assist prepare for human exploration of Mars. 


      The Perseverance rover was constructed and is operated by JPL, which is administered for NASA by Caltech in Pasadena, California. 



      For additional information about Perseverance, go to: 

      mars.nasa.gov/mars2020/ 

      nasa.gov/perseverance


      Courtesy: NASA.gov


      ~ Jai Krishna Ponnappan

      You may also want to read more about Space Missions and Systems here.



      Juno, NASA's Spacecraft, Takes A Close Look At Jupiter's Moon Ganymede

       


      From the left to the right: The mosaic and geologic maps of Ganymede, Jupiter's moon, were created using the finest available photos from NASA's Voyager 1 and 2 spacecraft, as well as NASA's Galileo spacecraft. 

      Credit: USGS Astrogeology Science Center/Wheaton/NASA/JPL-Caltech/USGS Astrogeology Science Center/Wheaton/NASA/JPL-Caltech 


      After more than 20 years, the first of the gas-giant orbiter's back-to-back flybys will deliver a close encounter with the gigantic moon. 

      NASA's Juno spacecraft will pass within 645 miles (1,038 kilometers) of Jupiter's biggest moon, Ganymede, on Monday, June 7 at 1:35 p.m. EDT (10:35 a.m. PDT). Since NASA's Galileo spacecraft made its last near approach to the solar system's largest natural satellite on May 20, 2000, the flyby will be the closest a spacecraft has gotten near the solar system's greatest natural satellite. 


      The solar-powered spacecraft's flyby will provide insights about the moon's composition, ionosphere, magnetosphere, and ice shell, in addition to stunning photographs. Future missions to the Jovian system will benefit from Juno's studies of the radiation environment around the moon. 

      Ganymede is the only moon in the solar system with its own magnetosphere, a bubble-shaped area of charged particles around the celestial body that is larger than Mercury. “Juno contains a suite of sensitive equipment capable of observing Ganymede in ways never previously possible,” stated Southwest Research Institute in San Antonio Principal Investigator Scott Bolton. 

      “By flying so close, we will bring Ganymede exploration into the twenty-first century, complementing future missions with our unique sensors and assisting in the preparation of the next generation of missions to the Jovian system, including NASA's Europa Clipper and ESA's Jupiter ICy moons Explorer [JUICE] mission.” 


      About three hours before the spacecraft's closest approach, Juno's science equipment will begin gathering data. Juno's Microwave Radiometer (MWR) will gaze through Ganymede's water-ice crust, gathering data on its composition and temperature, alongside the Ultraviolet Spectrograph (UVS) and Jovian Infrared Auroral Mapper (JIRAM) sensors. 




      A spinning Ganymede globe with a geologic chart placed over a global color mosaic is animated. Credit: USGS Astrogeology Science Center/Wheaton/ASU/NASA/JPL-Caltech/USGS Astrogeology Science Center/Wheaton/ASU/NASA/JPL-Caltech 


      “The ice shell of Ganymede contains some light and dark parts, implying that certain parts may be pure ice while others include filthy ice,” Bolton explained. 


      “MWR will conduct the first comprehensive study of how ice composition and structure change with depth, leading to a deeper understanding of how the ice shell originates and the mechanisms that resurface the ice over time.” 

      The findings will be used to supplement those from ESA's upcoming JUICE mission, which will study ice using radar at various wavelengths when it launches in 2032 to become the first spacecraft to circle a moon other than Earth's Moon. 


      Juno's X-band and Ka-band radio frequencies will be utilized in a radio occultation experiment to study the moon's fragile ionosphere (the outer layer of an atmosphere where gases are excited by solar radiation to form ions, which have an electrical charge). 

      “As Juno travels behind Ganymede, radio signals will travel over Ganymede's ionosphere, generating modest variations in frequency that should be picked up by two antennas at the Deep Space Network's Canberra complex in Australia,” said Dustin Buccino, a Juno mission signal analysis engineer at JPL. “We might be able to grasp the relationship between Ganymede's ionosphere, its intrinsic magnetic field, and Jupiter's magnetosphere if we can monitor this change.” 


      With NASA's interactive Eyes on the Solar System, you can see where Juno is right now. 

      The Juno spacecraft is a dynamic technical wonder, with three huge blades reaching out 66 feet (20 meters) from its cylindrical, six-sided body, spinning to keep itself steady as it executes oval-shaped orbits around Jupiter. 


      Juno's Stellar Reference Unit (SRU) navigation camera is normally responsible for keeping the Jupiter spacecraft on track, but it will perform double duty during the flyby. 


      Along with its navigational functions, the camera will collect information on the high-energy radiation environment in the region surrounding Ganymede by capturing a particular collection of photos. 

      The camera is adequately insulated against radiation that may otherwise harm it. “In Jupiter's harsh radiation environment, the traces from penetrating high-energy particles appear in the photos as dots, squiggles, and streaks — like static on a television screen. 

      According to Heidi Becker, Juno's radiation monitoring lead at JPL, "we extract these radiation-induced noise patterns from SRU photos to obtain diagnostic pictures of the radiation levels encountered by Juno." 


      Meanwhile, the Advanced Stellar Compass camera, developed by the Technical University of Denmark, will count very intense electrons that pass through its shielding at a quarter-second interval. The JunoCam imager has also been enlisted. 


      The camera was designed to transmit the thrill and beauty of Jupiter exploration to the public, but it has also given a wealth of essential research throughout the mission's almost five-year stay there. JunoCam will capture photographs at a resolution comparable to the best from Voyager and Galileo for the Ganymede flyby. 

      The Juno research team will examine the photographs and compare them to those taken by earlier missions, seeking for changes in surface characteristics that may have happened over four decades or more. 

      Any changes in the pattern of craters on the surface might aid astronomers in better understanding the present population of objects that collide with moons in the outer solar system. 


      Due to the speed of the flyby, the frozen moon will change from a point of light to a visible disk and back to a point of light in roughly 25 minutes from JunoCam's perspective. 


      There's just enough time for five photographs in that amount of time. “Things move quickly in the area of flybys, and we have two back-to-back flybys coming up next week. As a result, every second counts,” stated Juno Mission Manager Matt Johnson of the Jet Propulsion Laboratory. 

      “On Monday, we'll fly through Ganymede at about 12 miles per second (19 kilometers per second). We're making our 33rd scientific flyby of Jupiter in less than 24 hours, swooping low over the cloud tops at around 36 miles per second (58 kilometers per second). It's going to be a roller coaster.” even more Concerning the Mission. 

      The Juno mission is managed by JPL, a subsidiary of Caltech in Pasadena, California, for the principle investigator, Scott J. Bolton of the Southwest Research Institute in San Antonio. Juno is part of NASA's New Frontiers Program, which is administered for the agency's Science Mission Directorate in Washington by NASA's Marshall Space Flight Center in Huntsville, Alabama. 


      The spacecraft was manufactured and is operated by Lockheed Martin Space in Denver. 


      courtesy www.nasa.com

      Posted by Jai Krishna Ponnappan


      More data on Juno may be found at,


      https://www.nasa.gov/juno for further details.

      https://www.missionjuno.swri.edu


      Follow the mission on social media at 

      https://www.facebook.com/NASASolarSystem 

      and on Twitter at https://twitter.com/NASASolarSystem 






      Quantum Computing Threat to Information Security



      Current RSA public-key (asymmetric) encryption systems and other versions rely on trapdoor mathematical functions, which make it simple to compute a public key from a private key but computationally impossible to compute the converse, a private key from a public key.

      The difficulties of integer factorization and elliptic curve variations of the discrete logarithm issue, both of which have no known solution for computing an inverse in polynomial time, are exploited to create frequently used trapdoor functions (that is, on a finite timescale). 


      In a nutshell, this so-called "computational hardness" provides safety. 


      In 1994, however, Peter Shor proposed a quantum method that may be employed on a sufficiently large-scale quantum computer to perform integer factorization in polynomial time. 

      The now-famous quantum technique has now been proved to solve the discrete logarithm and elliptic-curve logarithm problems in polynomial time as well. 


      As a result of the creation of an FTQC in conjunction with this quantum algorithm, the security of present asymmetric public-key cryptography is jeopardized. 

      Furthermore, Shor's method exemplifies how advances in the mathematics and physical sciences have the potential to jeopardize secure communications in general. 


      In addition to Defense Department and critical cyber infrastructure systems, the world's digital revolution, which includes 4 billion internet users, 2 billion websites, and over $3 trillion in retail transactions, is backed at multiple tiers by existing public-key cryptography. 


      While the creation of an FTQC is estimated to be at least a decade or two away, there is still a pressing need to solve this issue because of the ‘record now, exploit later' danger, in which encrypted data is collected and kept for subsequent decryption by an FTQC when one becomes available. 

      As a result, the US National Institute of Standards and Technology's Post Quantum Cryptography Project, which includes worldwide partners—a security "patch" for the internet—is prioritizing the development of new "quantum hard" public-key algorithms.




      Post Quantum Computing Encryption - Future-Proofing Encryption



      Encryption in the post-quantum era. 


      Many popular media depictions of quantum computing claim that the creation of dependable large-scale quantum computers will bring cryptography to an end and that quantum computers are just around the corner. 

      The latter point of view may turn out to be overly optimistic or pessimistic, if you happen to rely on quantum-computing-proof security. 

      While quantum computers have made significant progress in recent years, there's no certainty that they'll ever advance beyond laboratory proof-of-concept devices to become a realistic daily technology. (For a more thorough explanation, see a recent ASPI study.) 


      Nonetheless, if quantum computing becomes a viable technology, several of the most extensively used encryption systems would be vulnerable to quantum computer cryptography assaults because quantum algorithms may drastically shorten the time it takes to crack them. 


      For example, the RSA encryption scheme for the secure exchange of encryption keys, which underlies most web-based commerce, is based on the practical difficulty of finding prime factors of very big integers using classical (non-quantum) computers.

      However, there is an extremely efficient quantum technique for prime factorization (known as ‘Shor's algorithm') that would make RSA encryption vulnerable to attack, jeopardizing the security of the vast quantity of economic activity that relies on the ability to safeguard moving data. 

      Other commonly used encryption protocols, such as the Digital Signature Algorithm (DSA) and Elliptic Curve DSA, rely on mathematical procedures that are difficult to reverse conventionally but may be vulnerable to quantum computing assaults. 


      Moving to secure quantum communication channels is one technique to secure communications. 


      However, while point-to-point quantum channels are conceivable (and immune to quantum computer assaults), they have large administration overheads, and constructing a quantum ‘web' configuration is challenging. 

      A traditional approach is likely to be favored for some time to come for applications such as networking military force units, creating secure communications between intelligence agencies, and putting up a secure wide-area network. 


      Non-quantum (classical) techniques to data security, fortunately, are expected to remain safe even in the face of quantum computer threats. 


      Quantum assaults have been found to be resistant to the 256-bit Advanced Encryption Standard (AES-256), which is routinely employed to safeguard sensitive information at rest. 

      Protecting data at rest addresses only half of the problem; a secure mechanism for transferring encryption keys between the start and end locations for data in motion is still required. 


      As a result, there's a lot of work being done to construct so-called "post-quantum" encryption systems that rely on mathematical processes for which no quantum algorithms exist. 


      IBM has already detailed a quantum-resistant technology for safely transporting data across networks.  If the necessity arises, such a system might possibly replace RSA and other quantum-vulnerable encryption systems.



      If everything else fails, there's always encryption technologies for the twenty-first century. 


      One technique to improve communication security is to be able to ‘narrowcast' in such a way that eavesdropping is physically difficult, if not impossible. 

      However, this is not always practicable, and there will always be messages that must pass over channels that are sensitive to eavesdropping. 


      Even so-called "secure" channels can be breached at any time. 


      The actual tapping of a subsea cable run to a Soviet naval facility on the Kamchatka Peninsula by the US Navy in the 1970s is a good example. The cable was deemed safe since it ran wholly within Russian territorial seas and was covered by underwater listening posts. 

      As a result, it transmitted unencrypted messages. The gathered signals, though not of high intelligence value in and of themselves, gave cleartext ‘cribs' of Soviet naval communications that could be matched with encrypted data obtained elsewhere, substantially simplifying the cryptanalytic work. 

      Even some of the LPI/LPD technology systems discussed in earlier sections may be subject to new techniques. 

      For example, the Pentagon has funded research on devices that gather single photons reflected off air particles to identify laser signals from outside the beam, with the goal of extracting meaningful information about the beam direction, data speeds, and modulation type. The ultimate objective is to be able to intercept laser signals in the future.  


      A prudent communications security approach is to expect that an opponent will find a method to access communications, notwithstanding best attempts to make it as difficult as possible. 


      Highly sensitive information must be safeguarded from interception, and certain data must be kept safe for years, if not decades. Cryptographic procedures that render an intercepted transmission unintelligible are required. 

      As we saw in the section on the PRC's capabilities, a significant amount of processing power is currently available to target Australian and ally military communications, and the situation is only going to become worse. 

      On the horizon are technical dangers, the most well-known of which is the potential for effective quantum computing. Encryption needs to be ‘future proofed.'


      As secure intermediates, space-based interconnections are used. 


      If the connection can be made un-interceptable, space-based communications might provide a secure communication route for terrestrial organizations. Information and control signals between spacecraft and the Earth have been sent by radio waves to and from ground stations until now. 

      Interception is achievable when collection systems are close enough to the uplink transmitter to collect energy from either the unavoidable side lobes of the main beam or when the collection system is able to be positioned inside the same downlink footprint as the receiver. 

      The use of laser signals of various wavelengths to replace such RF lines has the potential to boost data speeds while also securing the communications against eavesdropping. 


      Using laser communication connection between spacecraft has a number of advantages as well. 

      Transmission losses over long distances restrict the efficiency with which spacecraft with low power budgets can exchange vast amounts of data, and RF connections inevitably restrict bandwidth. 


      The imposts on space, weight, and power on spacecraft would be reduced if such linkages were replaced by laser communications. 

      The benefits might include being able to carry larger sensor and processing payloads, spending more time on mission (owing to reduced downtime to recharge batteries), or a combination of the two. 

      In the United States, the Trump administration's Space Force and anticipated NASA operations (including a presence on the moon and deep space missions) have sparked a slew of new space-based communications research initiatives. 


      NASA has a ten-year project road map (dubbed the "decade of light") aiming at creating infrared and optical frequency laser communication systems, combining them with RF systems, and connecting many facilities and spacecraft into a reliable, damage-resistant network. 

      As part of that effort, it is developing various technology demonstrations. 

      Its Laser Communications Relay Demonstration, which is set to be live in June, will utilize lasers to encode and send data at speeds 10 to 100 times faster than radio systems.  

      NASA uses the example of transmitting a map of Mars' surface back to Earth, which may take nine years with present radio technology but just nine weeks using laser communications. T

      he practicality of laser communications has been demonstrated in laboratory prototype systems, and NASA plans to launch space-based versions later this year. The Pentagon's Space Development Agency (SDA) and the Defense Advanced Research Projects Agency (DARPA) are both working on comparable technologies, but with military and intelligence purposes in mind. 


      The SDA envisions hundreds of satellites linked by infrared and optical laser communication connections. 

      Sensor data will be sent between spacecraft until it reaches a satellite in touch with a ground station, according to the plan. Information from an orbiting sensor grid may therefore be sent to Earth in subsecond time frames, rather than the tens of minutes it can take for a low-Earth-orbiting satellite to pass within line of sight of a ground station. 

      Furthermore, because to the narrow beams created by lasers, an eavesdropper has very limited chance of intercepting the message. Because of the increased communication efficiency, ‘traffic jams' in the considerably more extensively utilized radio spectrum are significantly less likely to occur. 

      This year, the SDA plans to conduct a test with a small number of "cubesats." Moving to even higher frequencies, X-ray beams may theoretically transport very high data-rate messages. In terrestrial applications, ionization of air gases would soon attenuate signals, but this isn't an issue in space, and NASA is presently working on gigabit-per-second X-ray communication lines between spacecraft.  

      Although NASA is primarily interested in applications for deep space missions (current methods can take many hours to transmit a single high-resolution photograph of a distant object such as an asteroid after a flyby), the technology has the potential to link future constellations of intelligence-gathering and communications satellites with extremely high data-rate channels. On board the International Space Station, NASA has placed a technology demonstration.



      Communications with a low chance of being detected. 


      One technique to keep communications safe from an enemy is to never send them over routes that can be detected or intercepted. For mobile force units, this isn't always practicable, but when it is, communications security may be quite effective. 

      The German army curtailed its radio transmissions in the run-up to its Ardennes operation in December 1944, depending instead on couriers and landlines operating within the region it held (which was contiguous with Germany, so that command and control traffic could mostly be kept off the airwaves).

       The build-up of considerable German forces was overlooked by Allied intelligence, which had been lulled into complacency by having routinely forewarned of German moves via intercepted radio communications. 

      Even today, when fibre-optic connections can transmit data at far greater rates than copper connections, the option to go "off air" when circumstances allow is still valuable. Of course, mobile troops will not always have the luxury of transferring all traffic onto cables, especially in high-speed scenarios, but there are still techniques to substantially minimize the footprint of communication signals and, in some cases, render them effectively undetectable. 


      Frequency-hopping and spread-spectrum radios were two previous methods for making signals less visible to an eavesdropper. 


      Although these approaches lower the RF footprint of transmissions, they are now vulnerable to detection, interception, and exploitation using wideband receivers and computer spectral analysis tools. Emerging technologies provide a variety of innovative approaches to achieve the same aim while improving security. 

      The first is to use extremely directed ‘line of sight' signals that may be focused directly at the intended receiver, limiting an adversary's ability to even detect the broadcast. This might be accomplished, for example, by using tightly concentrated laser signals of various wavelengths that may be precisely directed at the desired recipient's antenna when geography allow. 


      A space-based relay, in which two or more force components are linked by laser communication channels with a constellation of satellites, which are connected by secure links (see the following section for examples of ongoing work in that field), offers a difficult-to-intercept communications path. 


      As a consequence, data might be sent with far less chance of being intercepted than RF signals. The distances between connecting parties are virtually unlimited for a satellite system with a worldwide footprint for its uplinks and downlinks. Moving radio signals to wavelengths that do not travel over long distances due to atmospheric absorption, but still give effective communications capabilities at small ranges, is a second strategy that is better suited to force elements in close proximity. 


      The US Army, for example, is doing research on deep ultraviolet communications (UVC). 5 UVC has the following benefits over radio frequencies such as UHF and VHF: 


      • the higher frequency enables for faster data transfer

      • very low-powered signals can still be received over short distances

      • signal strength rapidly drops off over a critical distance 


      Communications with a low chance of being detected. One technique to keep communications safe from an enemy is to never send them over routes that can be detected or intercepted. 


      For mobile force units, this isn't always practicable, but when it is, communications security may be quite effective. The German army curtailed its radio transmissions in the run-up to its Ardennes operation in December 1944, depending instead on couriers and landlines operating within the region it held (which was contiguous with Germany, so that command and control traffic could mostly be kept off the airwaves). 

      The build-up of considerable German forces was overlooked by Allied intelligence, which had been lulled into complacency by having routinely forewarned of German moves via intercepted radio communications. 

      Even today, when fiber-optic connections can transmit data at far greater rates than copper connections, the option to go "off air" when circumstances allow is still valuable. Of course, mobile troops will not always have the luxury of transferring all traffic onto cables, especially in high-speed scenarios, but there are still techniques to substantially minimize the footprint of communication signals and, in some cases, render them effectively undetectable. 


      Frequency-hopping and spread-spectrum radios were two previous methods for making signals less visible to an eavesdropper. 


      Although these approaches lower the RF footprint of transmissions, they are now vulnerable to detection, interception, and exploitation using wideband receivers and computer spectral analysis tools. Emerging technologies provide a variety of innovative approaches to achieve the same aim while improving security. 

      The first is to use extremely directed ‘line of sight' signals that may be focused directly at the intended receiver, limiting an adversary's ability to even detect the broadcast. 

      This might be accomplished, for example, by using tightly concentrated laser signals of various wavelengths that may be precisely directed at the desired recipient's antenna when geography allow. 

      A space-based relay, in which two or more force components are linked by laser communication channels with a constellation of satellites, which are connected by secure links (see the following section for examples of ongoing work in that field), offers a difficult-to-intercept communications path. 

      As a consequence, data might be sent with far less chance of being intercepted than RF signals. The distances between connecting parties are virtually unlimited for a satellite system with a worldwide footprint for its uplinks and downlinks. 

      Moving radio signals to wavelengths that do not travel over long distances due to atmospheric absorption, but still give effective communications capabilities at small ranges, is a second strategy that is better suited to force elements in close proximity. 


      The US Army, for example, is doing research on deep ultraviolet communications (UVC). 5 UVC has the following benefits over radio frequencies such as UHF and VHF: 


      • the higher frequency allows for faster data transfer 

      • very low-powered signals can still be heard over short distances 

      • there is a quick drop-off in signal strength at a critical distance







      What Is Artificial General Intelligence?

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