Thursday, May 9, 2019

For a Split Second, a (Simulated) Particle Went Backward in Time

  In photography and film, a broken egg can be         perfectly unscrambled to its original state. But in   real life, quantum mechanics prevent even a     single particle from reversing its own course   through time.

This is not typically seen in regular life — with the possible exception of middle-agers who develop a sudden taste for sports cars and young trophy spouses. The question is, why not?
In what amounts to a technological triumph for the aspiring Benjamin Buttons of the virtual world, a team of quantum physicists reported earlier this year that they had succeeded in creating a computer algorithm that acts like the Fountain of Youth.
Using an IBM quantum computer, they managed to undo the aging of a single, simulated elementary particle by one millionth of a second. But it was a Pyrrhic victory at best, requiring manipulations so unlikely to occur naturally that it only reinforced the notion that we are helplessly trapped in the flow of time.

Most of us already sense that the atoms of a scrambled egg can’t be unscrambled back inside a pristine shell. Now it seems that, under general conditions, even a single particle probably can’t go backward without help and careful tinkering.
“We demonstrate that time-reversing even ONE quantum particle is an unsurmountable task for nature alone,” Valerii M. Vinokur, of Argonne National Laboratory, said in an email message; he is one of the five aspiring time lords led by Gordey B. Lesovik of the Moscow Institute of Physics and Technology.

On paper, the basic laws of physics are reversible; they work mathematically whether time is running forward or backward. But if time is just another dimension of space-time, as Einstein said, it’s a strange one-way dimension. In the real world we can climb out of the subway and turn left or right, but we don’t have the choice of going forward or back in time. We are always headed toward the future.

Left, IBM’s Q dilution refrigerator, which houses a quantum computer. Right, scientists Hanhee Paik and Sarah Sheldon examine hardware inside an open dilution fridge at IBM’s Thomas J. Watson Research Center in Yorktown Heights, N.Y.
CrediWe seem to be at the mercy of the second law of thermodynamics, which states that disorder and complexity only increase in a closed system such as, say, the universe. Thus, the atoms in an egg never unscramble themselves, in part because there are countless more ways for them to be thoroughly scrambled than successfully reassembled.We seem to be at the mercy of the second law of thermodynamics, which states that disorder and complexity only increase in a closed system such as, say, the universe. Thus, the atoms in an egg never unscramble themselves, in part because there are countless more ways for them to be thoroughly scrambled than successfully reassembled.
We seem to be at the mercy of the second law of thermodynamics, which states that disorder and complexity only increase in a closed system such as, say, the universe. Thus, the atoms in an egg never unscramble themselves, in part because there are countless more ways for them to be thoroughly scrambled than successfully reassembled.
But the arrow of time takes its direction not only from big numbers. According to quantum theory, that paradoxical body of rules governing the subatomic universe, not even a single particle can reverse its own course through time.
The uncertainty principle, which lies at the heart of quantum mechanics, states that, at any given moment, either the location or the velocity of a subatomic particle can be specified, but not both. As a result, a particle such as an electron, or a system of them, is represented by a mathematical entity called a wave function, whose magnitude is a measure of the probability of finding a particle in a particular place or condition.
The wave function extends throughout space and time. The law describing its evolution, known as the Schrödinger equation, after Austrian physicist Erwin Schrödinger​, is equally valid running forward or backward. But getting a wave function to go in reverse is no small trick.
Dr. Vinokur likened the challenge to sending a speeding billiard ball back to where it started. Seems easy: Just hit it with a cue stick. But if it’s a quantum ball, the uncertainty principle kicks in: You can know how hard to hit the ball, or in which direction to hit it, but not both.
“Because of the uncertainty principle, the quantum ball will never return back to the point of the origin,” Dr. Vinokur said.
Moreover, in quantum mechanics, the ball is actually a wave: Once its location is known, it spreads like ripples on a pond and evolves. Making it go backward takes more than a nudge with a cue stick. It requires reversing the phases of the waves, turning crests into troughs, and so forth, an operation too complex for nature to accomplish on its own.

Enter the quantum computer.
Unlike regular computers, which process a series of zeros and ones, or bits, quantum computers are made of so-called qubits, each of which can be zero and one at the same time. A quantum computer can perform thousands or millions of calculations simultaneously, so long as nobody looks to see what the answer is until the end.
Many of the largest tech companies, including Google, Microsoft and IBM, are racing to build such machines, which eventually could solve problems that regular computers can’t, such as breaking currently unbreakable cryptographic codes. Some scientists argue that nature itself is a quantum computer, and that the greatest utility of such a computer will be in simulating and exploring the paradoxes of quantum weirdness.
Dr. Lesovik and his colleagues set out to do just that. They wanted to try to make a wave function go backward, using an IBM quantum computer that is available online to the public.
A four-qubit superconducting square circuit in an IBM quantum computer.
CreditIBM Research

“It remains to be seen,” the team wrote in their paper posted online in February, “whether the irreversibility of time is a fundamental law of nature or whether, on the contrary, it might be circumvented.”
The IBM computer they used represents a baby step in the direction of what theorists call “quantum supremacy.” It had only 5 qubits (IBM devices with 16 and 20 qubits are also available), compared to Google’s top-of-the-line 72-qubit “Bristlecone” computer. To keep things even simpler, the group only used two or, sometimes, three of the qubits.
The time-reversal experiment was a four-step process. First the qubits were teed up in a simple initial state that mimicked “an artificial atom,” Dr. Vinokur said. Moreover, the qubits were entangled, by what Einstein called “spooky action at a distance” — whatever happened to one qubit affected measurements of the other one (or two, depending on how many were deployed).
Then the team tapped the qubits with a series of microwave radio pulses, which nudged the qubits from a simple state into more complexity. After a millionth of a second, the scientists then halted this phase — “the evolution program” — and treated the qubits with another microwave pulse, to reverse their phase and ready them to devolve to their youthful selves.
“In graphic language, we convert spreading rings in the pond into the rings that are ready to go back to their origin,” Dr. Vinokur said. That took another millionth of a second.
Finally, the team turned the “evolution” program back on. And the qubits went back to their original alignment — back to their own past. In effect, they got a millionth of a second younger.
The algorithm almost always worked. It succeeded in returning the qubits to their youthful states 85 percent of the time when the calculation involved two qubits, but only half the time when three qubits were used. The authors attributed the reduced reliability to imperfections in the quantum computer, and to the tendency of qubits to fall out of sync when their numbers increase.
Ultimately, it will take machines with hundreds of qubits to achieve the ambitions of quantum mathematicians. When such computers become available, the team’s time-reversal algorithm could be used to test them, Andrey V. Lebedev, a physicist at ETH Zurich in Switzerland and an author on the paper, said in a news release from the Moscow Institute of Physics and Technology.
In the meantime, anyone with a quantum computer can play Benjamin Button, using their algorithm. “Now everybody can make qubits younger,” Dr. Vinokur said.




Tuesday, May 7, 2019

Quantum computing with graphene plasmons

A novel material that consists of a single sheet of carbon atoms could lead to new designs for optical quantum computers. Physicists from the University of Vienna and the Institute of Photonic Sciences in Barcelona have shown that tailored graphene structures enable single photons to interact with each other. The proposed new architecture for quantum computer is published in the recent issue of npj Quantum Information.

Photons barely interact with the environment, making them a leading candidate for storing and transmitting  information. This same feature makes it especially difficult to manipulate information that is encoded in photons. In order to build a photonic quantum computer, one  must change the state of a second. Such a device is called a quantum logic gate, and millions of  will be needed to build a quantum computer. One way to achieve this is to use a so-called '' wherein two photons interact within the material. Unfortunately, standard nonlinear materials are far too inefficient to build a quantum logic gate.
It was recently realized that nonlinear interactions can be greatly enhanced by using plasmons. In a , light is bound to electrons on the surface of the material. These electrons can then help the photons to interact much more strongly. However, plasmons in standard materials decay before the needed quantum effects can take place.
In their new work, the team of scientists led by Prof. Philip Walther at the University of Vienna propose to create plasmons in graphene. This 2-D material discovered barely a decade ago consists of a single layer of carbon atoms arranged in a honeycomb structure, and, since its discovery, it has not stopped surprising us. For this particular purpose, the peculiar configuration of the electrons in graphene leads to both an extremely strong nonlinear interaction and plasmons that live for an exceptionally long time.

In their proposed graphene quantum logic gate, the scientists show that if single plasmons are created in nanoribbons made out of graphene, two plasmons in different nanoribbons can interact through their electric fields. Provided that each plasmon stays in its ribbon multiple  can be applied to the plasmons which is required for quantum computation. "We have shown that the strong nonlinear interaction in graphene makes it impossible for two plasmons to hop into the same ribbon," says Irati Alonso Calafell, first author of the study.
Their proposed scheme makes use of several unique properties of graphene, each of which has been observed individually. The team in Vienna is currently performing experimental measurements on a similar -based system to confirm the feasibility of their gate with current technology. Since the gate is naturally small, and operates at room temperature it should readily lend itself to being scaled up, as is required for many quantum technologies.

Hubble Sees Extremely Distant Lensing Galaxy Cluster

A spectacular new image from the NASA/ESA Hubble Space Telescope shows SPT-CL J0615-5746, a very massive group of galaxies located approximately 7.7 billion light-yearsaway in the constellation Pictor. First discovered by the South Pole Telescope less than a decade ago, SPT-CL J0615-5746 is so massive that its gravity bends light like a lens, making it very useful for peering deep into the early Universe.
This Hubble image shows the massive galaxy cluster SPT-CL J0615-5746. Image credit: NASA / ESA / Hubble 



Galaxy clusters contain thousands of galaxies of all ages, shapes and sizes.
Typically, they have a mass of about one million billion times the mass of the Sun and form over billions of years as smaller groups of galaxies slowly come together.
Albert Einstein predicted in his theory of general relativity that massive objects will deform the fabric of space itself.
When light passes one of these objects, such as a huge galaxy cluster, its path is changed slightly.
This effect, called gravitational lensing, is only visible in rare cases and only the best telescopes can observe the related phenomena.
A galaxy cluster called SPT-CL J0615-5746 is one of the farthest observed to cause gravitational lensing.
Among the identified background objects, there is SPT0615-JD, a galaxy that is thought to have emerged just 500 million years after the Big Bang. It is the farthest galaxy ever imaged by means of gravitational lensing.
SPT0615-JD has a mass of approximately 3 billion solar masses and is less than 2,500 light-years across, half the size of the nearby Small Magellanic Cloud.
The object is considered prototypical of young galaxies that emerged during the epoch shortly after the Big Bang.
“Just as ancient paintings can tell us about the period of history in which they were painted, so too can ancient galaxies tell us about the era of the Universe in which they existed,” Hubble astronomers said.
“To learn about cosmological history, we explore the most distant reaches of the Universe, probing ever further out into the cosmos.”
“The light from distant objects travels to us from so far away that it takes an immensely long time to reach us, meaning that it carries information from the past — information about the time at which it was emitted.”

“By studying such distant objects, we are continuing to fill the gaps in our picture of what the very early Universe looked like, and uncover more about how it evolved into its current state.”

High-Velocity Charged Particles Emit Cherenkov Radiation in Quantum Vacuum.

According to new research published in the journal Physical Review Letters, charged particles traveling through empty space can emit Cherenkov radiation by interacting with quantum vacuum.
 the properties of vacuum Cherenkov radiation in strong laser pulses and the magnetic field around a pulsar.



 It has long been known that charged particles, such as electrons and protons, produce the electromagnetic equivalent of a sonic boom when their speeds exceed that of photons in the surrounding medium.
This effect, known as Cherenkov radiation, is responsible for the characteristic blue glow from water in a nuclear reactor.
According to Albert Einstein, nothing can travel faster than light in vacuum. Because of this, it is usually assumed that the Cherenkov emission cannot occur in vacuum.
But according to quantum theory, the vacuum itself is packed full of ‘virtual particles,’ which move momentarily in and out of existence.
These particles are usually not observable but, in the presence of extremely strong electric and magnetic fields, they can turn the vacuum into an optical medium where the speed of light is slowed down so that high velocity charged particles can emit Cherenkov radiation. This is totally unexpected in a vacuum.
“This is a very exciting new prediction because it could provide answers to basic questions such as what is the origin of the gamma ray glow at the center of galaxies?” said University of Strathclyde’s Professor Dino Jaroszynski.
“Also, it provides a new way of testing some of the most fundamental theories of science by pushing them to their limits.”
Professor Jaroszynski and colelagues found that in extreme conditions, such as found at the focus of the world’s most powerful lasers, and the huge magnetic fields around neutron stars, this ‘polarized’ vacuum can slow down gamma rays just enough for Cherenkov emission to occur.
This means that the highest energy cosmic rays passing through the magnetic fields surrounding pulsars should predominantly emit Cherenkov radiation, vastly in excess of other types such as synchrotron radiation.
“Quantum electrodynamics is one of the best tested theories in physics, with extraordinary agreement between theoretical predictions and experimental data,” said Alexander Macleod, a researcher at the University of Plymouth.
“But this agreement has only been verified in the weak-field regime. Vacuum Cherenkov radiation offers a new way to test whether it survives in the strong-field limit.”

Friday, May 3, 2019

Hubble Assemble Wide View of the Evolving Universe

Astronomers have put together the largest and most comprehensive "history book" of galaxies into one single image, using 16 years' worth of observations from NASA's Hubble Space Telescope.
The deep-sky mosaic, created from nearly 7,500 individual exposures, provides a wide portrait of the distant universe, containing 265,000 galaxies that stretch back through 13.3 billion years of time to just 500 million years after the big bang. The faintest and farthest galaxies are just one ten-billionth the brightness of what the human eye can see. The universe's evolutionary history is also chronicled in this one sweeping view. The portrait shows how galaxies change over time, building themselves up to become the giant galaxies seen in the nearby universe.
This ambitious endeavor, called the Hubble Legacy Field, also combines observations taken by several Hubble deep-field surveys, including the eXtreme Deep Field (XDF), the deepest view of the universe. The wavelength range stretches from ultraviolet to near-infrared light, capturing the key features of galaxy assembly over time.
This Hubble Space Telescope image represents a portion of the Hubble Legacy Field, one of the widest views of the universe ever made. The image, a combination of thousands of snapshots, represents 16 years' worth of observations. The Hubble Legacy Field includes observations taken by several Hubble deep-field surveys, including the eXtreme Deep Field (XDF), the deepest view of the universe. The wavelength range stretches from ultraviolet to near-infrared light, capturing all the features of galaxy assembly over time. This cropped image mosaic presents a wide portrait of the distant universe and contains roughly 200,000 galaxies. They stretch back through 13.3 billion years of time to just 500 million years after the universe's birth in the big bang.
Credits: NASA, ESA, G. Illingworth and D. Magee (University of California, Santa Cruz), K. Whitaker (University of Connecticut), R. Bouwens (Leiden University), P. Oesch (University of Geneva) and the Hubble Legacy Field team

Thursday, May 2, 2019

Dark Web Users Aren’t Completely Safe On Tor Network

Over the span of last few years, the popularity of Dark Web has increased significantly and it continues to entice users every day with the privacy and anonymity it offers in the shadowy part of the world wide web.
The content on Dark Web can be accessed by The Onion Routing (TOR) which is an anonymous network. However, a recently published paper has found that you cannot be completely anonymous on the Tor network while accessing the dark web.

It is to be noted that the results in this paper are based on results obtained via two dark web search engines: Onion City and Ahimia. Furthermore, the study used the number of Tor users as a representative of the total number of dark web users and neglected other anonymous networks such as Freenet and I2P.

Can anonymity be verified on the Dark Web?

Even though TOR has several features which attempt to anonymize your activities online, researchers and security experts are continuously working to develop tools through which they can identify individuals or hidden services and de-anonymize them.
For instance, when the FBI took control of the Freedom Hosting (a defunct Tor specialist web hosting service) in 2013, it infected the web hosting service with a malware designed to identify visitors.
The FBI used malware which served as “a computer and internet protocol address verifier” in Freedom Hosting to identify and verify suspects as well as their location using a proxy server or anonymous services such as TOR.

How are Tor users identified?

In this study, the number of Tor users was estimated on the basis of the directory requests made by the Tor client. The directory requests then disassemble IP addresses according to country codes.
These IP addresses were found through ISPs that recognize Tor network connections via a continuously updated Tor relay list. The requests of directories are also numbered frequently for the clients. These numbers, together, represent the number of Dark Web users indirectly.
The study also analyzed the influence of the dark web on various parts of society. It represents a new evaluation of the current state of the dark web by estimating the number of Tor users. For further insights, you can refer to the complete report HerHere.


Chandrayaan -2 full details here .

Updates-

• The orbiter and lander modules will be stacked as an integrated module and accommodated inside an advanced GSLV MK-III launch vehicle
  • The journey from the earth to the moon will take around 45-50 days.

NEW DELHI: India’s highly ambitious Rs 800-crore Chandrayaan-2 mission will be launched between July 9 and July 16. The spacecraft, involving an orbiter, a lander called Vikram and a rover named Pragyan, is expected to land on the moon on September 6.

The orbiter and lander modules will be stacked as an integrated module and accommodated inside an advanced GSLV MK-III launch vehicle. The rover will be housed inside the lander. After the launch from Sriharikota into the earth-bound orbit by GSLV MK-III between July 9 and 16, the integrated module will reach the moon orbit using an orbiter propulsion module, a statement from Indian Space Research Organisation (Isrosaid. The journey from the earth to the moon will take around 45-50 days.

CHANDRAYAAN-2 LAUNCH, LUNAR TRANSFER, AND LANDING TRAJECTORY
Modified from a presentation given by ISRO director M. Annadurai to the United Nations Committee on the Peaceful Uses of Outer Space in June 2017.

Once Chandrayaan-2 spacecraft reaches the lunar orbit, Vikram will separate from the orbiter and soft-land at the predetermined site close to the south pole, which had not been explored by other countries.

Talking to TOI, Isro chairman K Sivan said, “Once Vikram lands on the lunar surface on September 6, rover Prayan will come out of it and roll out on the lunar surface for 300-400 metre. It will spend 14 earth days on the moon for carrying out different scientific experiments.”

Sivan said, “Altogether, there will be 13 payloads in the spacecraft. Three payloads in rover Pragyan and rest 10 payloads in lander Vikram and orbiter." The rover will analyse the content of the lunar surface and send data and images back to the Earth through the orbiter within 15 minutes, he said.

The launch of India’s second lunar mission was initially planned in April last year but Isro kept deferring it because of the complexities involved in the mission. In fact, the four-legged Vikram lander suffered a fracture in one of its legs during a test earlier this year. India had also almost lost the race to 
Israel
 to become the fourth country in the world after 
, US and China to land the spacecraft on the moon. However, with Israel’s Beresheet failing to land on the moon on April 12 this year, Chandrayaan-2’s moon-landing on September 6, if successful, will make India the fourth country in the world to land on the moon.

The landing of 3,290-kg Chandrayaan-2 craft will be much more difficult than Israel’s Beresheet. While Beresheet tried to touch down on a plain of solidified lava, known as the Sea of Serenity, which has a flattened surface and more exposure to the sun, Chandrayaan-2 will explore the south pole, an uncharted territory. Only China’s Chang’e 4 spacecraft had recently in January landed on the moon’s far side, also known as the dark side because it faces away from the Earth and remains comparatively unknown.

India had first launched its moon mission Chandrayaan-1, which involved only an orbiter, on October 22, 2008. The spacecraft made more than 3,400 orbits around the moon during which it took hundreds of images of the moon. The Rs 386-crore mission concluded when the communication with the spacecraft was lost on August 29, 2009. Chandrayaan operated for 312 days as opposed to the intended two years but the mission achieved 95% of its planned objectives.


CHANDRAYAAN-2 LANDING TRAJECTORY
From M. Annadurai et al. presentation to the 10th IAA Symposium on the Future of Space Exploration, Torino, Italy, 27-29 June, 2017.


Orbiter

The orbiter is physically similar to Chandrayaan-1. It is three-axis stabilized with reaction wheels. The orbiter carries five science instruments and two supporting instruments.


  • Terrain Mapping Camera 2 (TMC-2) is based upon TMC (a predecessor on Chandrayaan-1) and will perform 3D mapping of the lunar surface using two cameras.
  • Collimated Large Array Soft X-ray Spectrometer (CLASS) is based upon C1XS (a predecessor on Chandrayaan-1) and will map abundance of major rock-forming elements on the Moon including Mg, Al, Si, Ca, Ti, and Fe. Assisting it is the Solar X-ray Monitor (XSM), which measures solar x-ray emission.
  • Chandra's Atmospheric Composition Explorer(ChACE-2) is a neutral mass spectrometer that is based upon CHACE (a predecessor on Chandrayaan-1's Moon Impact Probe).
  • Synthetic Aperture Radar (SAR) will perform radar mapping of the surface in both L and S bands of the radio spectrum. It has heritage from MiniSAR on Chandrayaan-1 but will be the first L-band radar mapper to orbit the Moon.
  • Imaging Infra-Red Spectrometer (IIRS) is sensitive to light with wavelengths between 0.8 and 5 microns and has the specific goal of mapping the abundance of hydroxl ions and molecular water.
  • Finally, the Orbiter High Resolution Camera (OHRC) will perform high-resolution imaging of the landing site prior to the lander mission.
CAD MODEL OF CHANDRAYAAN-2, LAUNCH CONFIGURATION
Chandrayaan-2 consists of an orbiter, lander, and small rover. Here, the spacecraft is shown in its launch configuration.



Lander

Physically, the lander is shaped like a truncated square-based pyramid, built around a cylinder that houses the substantial propellant tank. It will perform inertial navigation throughout the descent using its Laser-gyro-based inertial reference unit and accelerometer package, LIRAP. The propulsion system includes four throttleable engines that can each provide 800 newtons of thrust, and 8 attitude rockets of 50 newtons each. The lander will communicate direct to Earth using a steerable, dual-gimbal, S-band radio antenna.
The lander has multiple cameras in its Hazard Detection and Avoidance (HDA) system, which it will use to determine horizontal velocity from feature tracking and identify the landing site using pattern matching. HDA also contains microwave and laser altimeters and a laser Doppler velocimiter. The HDA system collects data and instructs the rockets to fire to steer the lander to the landing site. I didn't find any reference that indicated whether the lander has the ability to photograph the landscape it's sitting on. Surely it must, but I don't know.
Once on the ground, the lander will deploy its science payload:
  • Instrument for Lunar Seismic Activity (ILSA) will study moonquakes. Large enough quakes could allow it to study the Moon's deep interior, potentially from a polar position not accessible to the Apollo seismometers, which would be cool. This experiment will be a lot cooler if the lander is capable of surviving multiple lunar days.
  • Chandra’s Surface Thermophysical Experiment (ChaSTE) will measure thermal properties of the lunar surface.
  • Radio Anatomy of Moon Bound Hypersensitive ionosphere and Atmosphere (RAMBHA-Langmuir Probe) will measure near surface plasma density and how it changes over the course of the lunar daytime. According to a recent Nature article, lunar plasma is thought to participate in the levitation of lunar dust, a problem for future human exploration.
And, of course, the lander will carry a rover. The rover is very small, roughly Sojourner-sized, at 20 kilograms. Like NASA's Mars rovers, the Chandrayaan-2 rover uses a rocker-bogie suspension system supporting six independently motorized wheels, but unlike NASA's rovers its corner wheels do not steer. Therefore, it steers by rotating the wheels at different rates, like a tank. This is a perfectly fine method for a lightweight rover as long as the net effect of steering isn't to sink the rover into the soil.
To make sure the rover could move and steer on the Moon without embedding, ISRO developed a big sandbox filled with crushed anorthosite to test rover mobility in. When NASA does this with Mars rovers, they build full-size mobility system mockups with tiny bodies so the whole vehicle weighs on Earth what the real rover weighs on Mars, where gravity is a third of Earth's. But that wouldn't work for the already-small Chandrayaan-2 rover trying to simulate lunar gravity at a sixth of Earth's. So ISRO developed a different solution that I just love: attaching a giant helium-filled balloon to a duplicate test rover to counterbalance 5/6 of its weight. These tests succeeded, evidently.

MOBILITY TESTING OF THE CHANDRAYAAN-2 ROVER
ISRO employs a balloon to counteract 5/6 of the weight of a duplicate of the Chandrayaan-2 rover in order to test its mobility on simulated lunar soil at lunar gravity. From M. Annadurai et al. presentation to the 10th IAA Symposium on the Future of Space Exploration, Torino, Italy, 27-29 June, 2017.


Because of its small size, the rover instrumentation is fairly limited, much like Sojourner's was. It has two navigation cameras for stereo path planning and an inclinometer for safety (drives will stop if the rover's inclination or motor current gets too high). It has no rear-facing cameras. It will use a small radio antenna for communication with the lander, which will relay rover data to Earth. The radio antenna is atop its vertically-mounted solar panel. Its solar panel is mounted vertically because of the near-polar landing site. That suggests the rover will need to turn in place after traverses to align the panel for good power production.
The rover is equipped with two science instruments for elemental composition, both of which point downward, beneath the rover: a Laser-Induced Breakdown Spectroscope (LIBS) and an Alpha Particle X-Ray Spectrometer. In general, LIBS will get you lower-mass elements and APXS will get you higher-mass elements, with substantial overlap between them. LIBS is faster, APXS more sensitive to trace elements if you can give it long enough integration time. Perhaps they will be using LIBS along traverses, and APXS at stops.
Interestingly, a paper I read about the LIBS instrument suggested it was designed for a one-year primary mission. Officially, the lander mission has an expected lifetime of 14 days, but maybe there is hope that it will survive a lunar night to do science on a second lunar day. That would be awesome. But any successful landing at all would be an enormous accomplishment for India; I don't want to get greedy.
CHANDRAYAAN-2 LANDER DEPLOYING ROVER

CAD MODEL OF CHANDRAYAAN-2 ROVER FROM BELOW


Looking Ahead

Originally, Chandrayaan-2 was supposed to be a collaboration with the Russian space agency, but budget problems made Russia drop out, and India decided to go it alone. If Chandrayaan-2 succeeds, India's next step will be lunar sample return. They'd be following exactly the same path China has at the Moon, going quickly from a successful orbiter, to a lander/rover, to autonomous sample return. Unlike China, however, India is using international collaboration to increase its chances for success; Indian prime minister Narendra Modi and his Japanese counterpart Shinzo Abe signed an agreement a couple of weeks ago to collaborate on a future joint lunar sample return mission.
A lot of people are trying to make the separate Chinese and Japanese/Indian lunar efforts into a race. To be sure, there is some national pride riding on successes in space, and reaching milestones first. But races have only one winner. We all win when more organizations launch scientific missions into space. All of these countries have shared the data they gathered during past missions with scientists and the public. India's mission landing near the south pole, and China's landing on farside, will only enhance global understanding of the Moon, regardless of who gets there first. India or China may yet be defeated by physics -- deep-space exploration is challenging -- but they won't be defeated by each other's success.
Good luck, saubhaagy to ISRO and India on the upcoming launch of Chandrayaan-2!


Scientist discovered a Cold Quasar , A new stage of Galaxy Death.

LAWRENCE — At the 234th meeting of the American Astronomical Society in St. Louis, Allison Kirkpatrick, assistant professor of physics ...