NASA gears up for livestreaming mega event of Artemis I launch

As the SLS rocket is scheduled for launch during a two-hour window that opens at 8:33 a.m. EDT Monday, Aug. 29, from Launch Pad 39B at Kennedy Space Center, NASA is planning to provide a wide coverage of prelaunch, launch, and postlaunch activities for Artemis I.

Artemis I will be the first integrated test of NASA’s Orion spacecraft, Space Launch System (SLS) rocket, and the ground systems at the launch center in Florida, heralding future crewed flight test and future human lunar exploration.

The rocket and spacecraft have already reached the launch pad last week after the nearly 10-hour, four-mile trek from the Vehicle Assembly Building and a livestream of the rocket and spacecraft at the launch pad has been made available on the NASA Kennedy YouTube channel.

Live coverage of events will air on NASA Television, the NASA app, and the agency’s website, with prelaunch events starting Monday, Aug. 22. The launch countdown will begin Saturday, Aug. 27, at 10:23 a.m.

 

artemis

Artemis I set for launch / NASA

A live broadcast of the launch includes celebrity appearances by Jack Black, Chris Evans, and Keke Palmer, as well as a special performance of “The Star-Spangled Banner” by Josh Grobin and Herbie Hancock. It also will feature a performance of “America the Beautiful” by The Philadelphia Orchestra and cellist Yo-Yo Ma, conducted by Yannick Nézet-Séguin.

The first in a series of complex missions, Artemis I is an uncrewed flight test that will provide a foundation to extend human presence to the Moon and beyond. The mission will test the performance of the SLS rocket and test Orion’s capabilities over a period of about six weeks while on its travel that covers about 40,000 miles beyond the Moon and back to Earth.

Lightweight Crane Technology to be Tested on the Moon [ARTEMIS PROJECT]

Like a Swiss Army knife, NASA’s Lightweight Surface Manipulation System (LSMS) technology is likely to find many ways of usage on the surface of Moon as part of its Artemis moon program.

This lightweight robotic crane with a structurally efficient truss frame and cable actuation mimics the movement of a human arm, but with a much longer reach as seen in the visual provided by NASA. It is scalable to fit any sized lander, vehicle, or surface application and can use a toolbox of quick-interchange end-effectors, or tools, that allow it to act as a hoist, forklift, regolith scoop, welder, said the US space agency.

“The unique thing about the LSMS is its dexterity and multi-functionality,” said Barmac Taleghani, project manager at NASA’s Langley Research Center in Hampton, Virginia.

The LSMS tested at Langley more than a decade ago to demonstrate the concept for offloading large payloads, such as habitats and rovers, from landers on human exploration missions. Once it is used on the moon’s surface, it’s likely to be sent to Mars too in future NASSA programs.

“We started thinking about additional tools that could be useful so that when you land the LSMS it could be used for multiple tasks,” said Tom Jones.“You’ve already carried that mass there; why not reuse it?”

Meanwhile, LSMS has been upgraded to include a suite of new tools, such as a bucket truck end-effector for digging and maneuvering regolith, a forklift tine tool for lifting cargo pallets, and a welding tool, in addition to greater autonomous functionality. The next design is on a larger for a large cargo to lunar lander under the artemis project.

LSMS in action
Although similar in structural design to a terrestrial crane, the LSMS uses a cable-driven actuation system to articulate its arm links and precisely maneuver payloads.
Credits: NASA

“As we establish a sustainable presence on the Moon under the Artemis missions, we will need to start setting up multiple elements, and there will be a wide range of tasks that could leverage the versatility and functionality of the LSMS,” Jones said.

The new LSMS will be similar in size to the original prototype with about a 25-foot reach and will be able to lift payloads weighing around one metric ton on the Moon, equal to approximately 2,200 pounds, or the size of an elephant.

Jones further said, “LSMS is designed to operate either on the Moon or Mars or really any kind of planetary body. There may be different environmental concerns depending on the destination, but the hardware would be very similar.”

 

Planet Nine or Exoplanet? Scientists find startling resemblance in star 336 light years away

As astronomers are looking for a hypothetical “Planet Nine” in our solar system, an exoplanet 336 light years from Earth is looking more like the Planet Nine of its star system.

Planet Nine, potentially 10 times the size of Earth and orbiting far beyond Neptune in a highly eccentric orbit around the sun, was proposed in 2012 to explain perturbations in the orbits of dwarf planets beyond Neptune’s orbit, so-called detached Kuiper Belt objects. However, it has yet to be found, if ever it exists.

A similarly weird extrasolar planet was discovered far from the star HD 106906 in 2013 was much heavier than the predicted mass of Planet Nine at probably 11 times the mass of Jupiter, or 3,500 times the mass of Earth. And it was located in an unexpected location, far above the dust plane of the planetary system and tilted at an angle of about 21 degrees.

It is not known whether the planet, HD 106906 b, is in an orbit perpetually bound to the binary star — which is 15 million years old compared to the 4.5 billion-year age of our sun or on its way out of the planetary system, never to return.

In a paper published on Dec. 10, 2020, in the Astronomical Journal, astronomers answer that question. By precisely tracking the planet’s position over 14 years, they determined that it is likely bound to the star in a 15,000-year, highly eccentric orbit, making it a distant cousin of Planet Nine.

If it is in a highly eccentric orbit around the binary, “This raises the question of how did these planets get out there to such large separations,” said Meiji Nguyen, a recent UC Berkeley graduate and first author of the paper. “Were they scattered from the inner solar system? Or, did they form out there?”

According to senior author Paul Kalas, University of California, Berkeley, the resemblance to the orbit of the proposed Planet Nine shows that such distant planets can really exist and that they may form within the first tens of millions of years of a star’s life. “Something happens very early that starts kicking planets and comets outward, and then you have passing stars that stabilize their orbits,” he said.

What makes HD 106906 unique is that it is the only exoplanet that we know that is directly imaged, surrounded by a debris disk, misaligned, and widely separated, Nguyen said. “This is what makes it the sole candidate we have found thus far whose orbit is analogous to the hypothetical Planet Nine.”

Internet for All? SpaceX just launched 60 satellites into space orbit, as part of its Starlink fleet

On Wednesday, June 3 at 9:25 p.m. EDT, SpaceX launched its eighth Starlink mission aboard Falcon 9, which lifted off from Space Launch Complex 40 (SLC-40) at Cape Canaveral Air Force Station, just days after SpaceX and NASA made history amid coronavirus pandemic last weekend, launching two astronauts into space on board a Falcon 9 rocket to join the International Space Station (ISS).

Astronauts Robert Behnken and Douglas Hurley were launched into space on board a SpaceX Falcon 9 rocket, marking the first time humans have been launched from the US since 2011.

Falcon 9’s first stage previously supported the Telstar 18 VANTAGE mission in September 2018, the Iridium-8 mission in January 2019, and two separate Starlink missions in May 2019 and in January 2020. Following stage separation, SpaceX landed Falcon 9’s first stage on the “Just Read the Instructions” droneship, which was stationed in the Atlantic Ocean.

On this mission, SpaceX launched the first Starlink satellite with a deployable visor to block sunlight from hitting the brightest spots of the spacecraft. NASA’s Kennedy Space Centre said: “The goal of Starlink is to create a network that will help provide internet services to those who are not yet connected, and to provide reliable and affordable internet across the globe.”

Starlink Satellite

Explaining the Starlink satellite design, SpaceX said on its website that it was driven by the fact that they fly at a very low altitude compared to other commmunication satellites. “We do this to prioritize space traffic safety and to minimize the latency of the signal between the satellite and the users who are getting internet service from it. Because of the low altitude, drag is a major factor in the design.”

During orbit raise, the satellites must minimize their cross-sectional area relative to the wind, otherwise drag will cause them to fall out of orbit. High drag is a double-edged sword—it means that flying the satellites is tricky, but it also means that any satellites that are experiencing problems will de-orbit quickly and safely burn up in the atmosphere. This reduces the amount of orbital debris or “space junk” in orbit.

This low-drag and thrusting flight configuration resembles an open book, where the solar array is laid out flat in front of the vehicle. When Starlink satellites are orbit raising, they roll to a limited extent about the velocity vector for power generation, always keeping the cross sectional area minimized while keeping the antennas facing Earth enough to stay in contact with the ground stations, said SpaceX.

Shark-Fin orientation

When the satellites reach their operational orbit of 550 km, drag is still a factor—so any inoperable satellite will quickly decay—but the altitude control system is able to overcome this drag with the solar array raised above the satellite in a vertical orientation that we call “shark-fin.” This is the orientation in which the satellite spends the majority of its operational life.

A recent study, published in arXiv, researchers led by Stefano Gallozzi, wrote: “Depending on their altitude and surface reflectivity, their contribution to the sky brightness is not negligible for professional ground based observations. With the huge amount of about 50,000 new artificial satellites for telecommunications planned to be launched in Medium and Low Earth Orbit, the mean density of artificial objects will be of >1 satellite for square sky degree; this will inevitably harm professional astronomical images.”

NASA’s Aqua satellite catches Tropical Cyclone Gaja’s landfall

Caught in the act of landfall, Tropical Cyclone Gaja was seen by NASA’s Aqua satellite as it passed overhead and collected temperature information.

The Atmospheric Infrared Sounder or AIRS instrument aboard NASA’s Aqua satellite passed over Tropical Cyclone Gaja on Nov. 15 at 3:29 p.m. EDT (2029 UTC) and analyzed the storm in infrared light. Infrared light provides temperature data and that’s important when trying to understand how strong storms can be. The higher the cloud tops, the colder and the stronger they are.

When Aqua passed over the Indian Ocean, Gaja’s center was making landfall along the coast of southeastern India. The AIRS instrument found coldest cloud top temperatures in thunderstorms around the center, where temperatures were as cold as minus 63 degrees Fahrenheit (minus 53 degrees Celsius). Storms with cloud top temperatures that cold have the capability to produce heavy rainfall.

At 10 a.m. EST (1500 UTC), the center of Tropical Cyclone Gaja was located near latitude 9.7 degrees north and longitude 75.9 degrees west. Gaja was moving toward west-southwest. Maximum sustained winds are near 46 mph (40 knots/74 kph) with higher gusts.

Gaja was exiting the southwestern coast of India on Nov. 16 at 7 a.m. EST (1200 UTC) and was moving into the Arabian Sea where it is expected to maintain strength and travel in a westerly direction over the next several days.

Sunday May 6: Solar Storm to cause Mobile, TV, Tech Blackout on Earth?

US space agency NASA has informed that a solar storm brewing on Sun is flaring up splitting huge sun storms which may reach earth on Sunday, May 6. It said a coronal hole or sun spot has opened up releasing huge swarm of cosmic rays which may take 8 minutes to reach earth.

The space weather watching unit of National Oceanic and Atmospheric Administration (NOAA) said the solar tsunami can create an aurora or polar lights when it hits earth. Astronomers have estimated that three such solar storms are likely to reach earth on May 6, to be precise, the Indian Ocean and India is very much within the target area.

The storm classified as G-1 or ‘minor’ is the biggest since 2004 and it could trigger sparks and melt soil on Moon, while its impact on Earth is still not comprehended by astronomers but similar storms had apparently given birth to origin of life on earth.

A section of scientists warned that the solar storms on Sunday could be severe enough to disrupt communications, satellite-based GPS, flaring up magnetic field around electricity power stations or transmitters. A partial tech blackout is likely to disrupt the Internet-based communications, they added.

Effects on Earth?

Since the severity has been classified as low by NOAA, it may cause voltage fluctuations in electricity supply or even cause power failures for now. However, the US Space Weather Prediction Center (SWPC) has issued a storm alert on Sunday and Monday stating that the solar storm could cause a “high stream of activity” that is characteristic to any G1-class storm. The gigantic coronal hole in the sun’s surface was captured today by NASA’s Solar Dynamics Observatory (SDO), said SWPC.

G1 (Minor) geomagnetic storm watches have been issued for 06 and 07 May 2018 due to the anticipated effects of a negative polarity coronal hole high speed stream… Aurora may be visible at high latitudes, that is, northern tier of the US such as northern Michigan and Maine,” said SWPC in a statement.

Meanwhile, conspiracy theorists woke up to the situation to claim that these disruptions are due to the effect of an approaching Nibiru planet which is lurking in the vicinity of our solar system. David Meade, its proponent, has repeated that the next seven years will witness tribulation with many more calamities. NASA has denied these claims as Internet Hoax, though.

50-Year-Cycle?

 

Researchers have long announced that a storm is likely to come and the most intense solar flare may reach earth in maximum fifty years. It is not sure whether the Sunday storm was the one or not.

Mausumi Dikpati of the National Center for Atmospheric Research (NCAR), who’s been working on these storms for decades, predicted that the next solar storm will be a stronger one. “The next sunspot cycle will be 30% to 50% stronger than the previous one,” she said a few years ago. It can produce a burst of solar activity second only to the historic Solar Max of 1958.

Earlier, such intense solar storms had been observed in 1805 and 1958 but with no mobiles and magnetic power lines, the disruption was not detectable as clearly as it would today when auroras and cell technology will showcase the real impact.

According to solar physicist David Hathaway of the National Space Science and Technology Center (NSSTC), a typical sunspot exists for just a few weeks. When it decays, it leaves behind a ‘corpse’ of weak magnetic fields.

Whether the big Doomsday is Sunday or not will be known sooner. For now, a storm is coming and how big will it be remains a major question.

Sperm being sent to ISS to see whether they squirm the same way in Space

Remember when you first learned about reproduction process in health class at school? Well, NASA biologists are wondering how some of those basics of how fertilization would work if sperm and egg were to unite in space. In other words, having sex aboard on ISS and examine how the sperm squirm in weightlessness — is their plan.

A cargo mission is launching to the International Space Station in April 2018 to study how weightlessness affects sperm. NASA’s Ames Research Center in California’s Silicon Valley manages the investigation, called Micro-11, aboard SpaceX’s 14th cargo resupply services mission to the International Space Station for NASA.

Little is currently known about the biology of reproduction in space, and this experiment will begin to address that gap by measuring, for the first time, how well bull and human sperm functions in space, said NASA in a statement. Studying reproductive biology in space is useful because the unique environment of microgravity can reveal processes and connections not visible in gravity on Earth, it explained the rationale behind such step.

In mammals, including humans, fertilization occurs when a sperm cell swims toward an egg and fuses with it. Before this can happen, the sperm cell must be activated to start moving. Next, to prepare it for fusing with the egg, the sperm needs to move faster, and its cell membrane must become more fluid.

Previous experiments with sea urchin and bull sperm suggest that activating movement happens more quickly in microgravity, while the steps leading up to fusion happen more slowly, or not at all. Delays or problems at this stage could prevent fertilization from happening in space.

For this experiment, two types of mammalian sperm, human and bull, will be sent to the space station as frozen samples. Bull sperm show similar changes in movement and other markers of fertility as human sperm. However, human sperm are inherently more varied in motion and appearance. So, the measurements of bull sperm will provide quality control to ensure the researchers can detect subtle differences in sperm from both species.

The astronaut crew will thaw the samples and add chemical mixtures that trigger activation of sperm movement and preparation for fusing with an egg. Researchers will use video to assess how well the space sperm move. Finally, the samples will be mixed with preservatives and returned to Earth, where they’ll be analyzed to see whether the steps necessary for fusion occurred and whether the samples from space differ from sperm samples activated on the ground.

We don’t know yet how long-duration spaceflight affects human reproductive health, and this investigation would be the first step in understanding the potential viability of reproduction in reduced-gravity conditions.

Managed by NASA’s Ames Research Center in California’s Silicon Valley, the Micro-11’s principal investigator for the fertilization in space experiment is Joseph S. Tash of the University of Kansas Medical Center in Kansas City. The experimental hardware for Micro-11 was developed by BioServe Space Technologies at the University of Colorado Boulder, and will launch aboard SpaceX’s 14th cargo resupply services mission to the International Space Station for NASA.

Hubble finds first galaxy without dark matter; Stunned scientists in dark for scientific explanation

How can a galaxy be there without dark matter? The galaxy NGC 1052-DF2 challenges currently-known theories of galaxy formation as it negates everything we know about nature of dark matter.

First identified with the Dragonfly Telephoto Array (DFA) and later observed by the Sloan Digital Sky Survey (SDSS), the NASA/ESA Hubble Space Telescope, the Gemini Observatory and the Keck Observatory, the galaxy without dark matter stunned scientists.

Since 1884 astronomers have invoked dark matter to explain why galaxies do not fly apart, given the speed at which they move within galaxies. From Kepler’s Second Law it is expected that the rotation velocities of stars will decrease with distance from the centre of a galaxy. This is not observed in NGC 1052-DF2, which resides about 65 million light-years away in the NGC 1052 Group, which is dominated by a massive elliptical galaxy called NGC 1052.

This large, fuzzy-looking galaxy is so diffuse that astronomers can clearly see distant galaxies behind it. This ghostly galaxy is not well-formed. It does not look like a typical spiral galaxy, but it does not look like an elliptical galaxy either. Based on the colours of its globular clusters, the galaxy is about 10 billion years old. However, even the globular clusters are strange: they are twice as large as typical groups of stars.

All of these oddities pale in comparison to the weirdest aspect of this galaxy: NGC 1052-DF2 is missing most, if not all, of its dark matter. The galaxy contains only a tiny fraction of dark matter that astronomers would expect for a galaxy this size. But how it formed is a complete mystery.

"I spent an hour just staring at this image," said lead researcher Pieter van Dokkum of Yale University. "This thing is astonishing: a gigantic blob so sparse that you see the galaxies behind it. It is literally a see-through galaxy."

This discovery makes all the current theories on the distribution of dark matter and its influence on galaxy formation redundant or partly false. "There is no theory that predicts these types of galaxies — how you actually go about forming one of these things is completely unknown," says co-author Allison Merritt from Yale University.

The MOND theory — Modified Newtonian Dynamics — suggests that the phenomena usually attributed to dark matter can be explained by modifying the laws of gravity. The result of this would be that a signature usually attributed to dark matter should always be detected, and is an unavoidable consequence of the presence of ordinary matter.

However, the discovery of NGC 1052-DF2 demonstrates that dark matter is somehow separable from galaxies. This is only expected if dark matter is bound to ordinary matter through nothing but gravity. Now researchers are pondering possible explanations for this missing dark matter in NGC 1052-DF2.

Did a cataclysmic event such as the birth of a multitude of massive stars sweep out all the gas and dark matter? Or did the growth of the nearby massive elliptical galaxy NGC 1052 billions of years ago play a role in NGC 1052-DF2’s dark matter deficiency? These ideas, however, still do not explain how this galaxy formed.


NGC 1052-DF2 is missing its dark matter. The galaxy contains only a tiny fraction of dark matter that astronomers would expect for a galaxy this size. But how it formed is a complete mystery.
Credit: NASA, ESA, and P. van Dokkum (Yale University)

NASA sees wide-eyed Typhoon Noru headed for landfall in Kyushu, Japan

Typhoon Noru was churning just south of the southwestern-most island of Japan when NASA’s Terra satellite captured an image of the storm with an eye over 35 miles wide. The Joint Typhoon Warning Center expects Noru to make landfall in Kyushu by August 6.

On August 4, 2017 at 0220 UTC (Aug. 3 at 10:20 p.m. EDT), NASA’s Terra satellite passed over the Northwestern Pacific Ocean and the Moderate Resolution Imaging Spectroradiometer or MODIS instrument captured a visible-light image of the storm. The image revealed that Noru’s eye had become more apparent since the previous day. The western quadrant of the storm was affecting Japan’s Tokara Islands, which lie to the south of Japan’s large island of Kyushu. The Tokara Islands is an archipelago in the Nansei Islands, part of the Ryukyu Archipelago. The chain of islands consists of twelve small islands between Yakushima and Amami-Oshima.

Animated enhanced infrared satellite imagery and radar imagery indicate that Noru was re-intensifying with improved deep convective thunderstorm banding and a 37-nautical-mile-wide eye.

On August 4, 2017 at 11 a.m. EDT (1500 UTC), Noru’s maximum sustained winds were near 86 mph (75 knots/139 kph). Noru’s eye was centered near 29.3 degrees north latitude and 130.3 degrees east longitude, about 218 nautical miles northeast of Kadena Air Base, Okinawa, Japan. Noru has tracked to the west-northwestward at 5.7 mph (5 knots/9.2 kph).

Warnings are already in effect for the sub-prefecture regions of Kyushu including: Satsuma Chiho, Osumi Chiho, Tanegashima-Yakushima Chiho, Amami Chiho, Nambu Heiyabu, Hokubu Heiyabu, Nambu Yamazoi and Hokubu Yamazoi.

For watches and warnings from the Japan Meteorological Agency on Noru, visit: http://www.jma.go.jp/jma/indexe.html

Noru is forecast to turn north-northeast and make landfall in Kyushu on August 6. The Joint Typhoon Warning Center forecasts the storm will then move in a northeasterly direction and move west of Kyoto on the big island of Japan before moving into the Sea of Japan.

NASA’s Juno to Fly Directly Over Jupiter’s Mysterious Red Spot Now

NASA’s Juno spacecraft is all set for another manoeuvre on July 10, flying directly over Jupiter’s Great Red Spot, the gas giant’s iconic, 10,000-mile-wide (16,000-kilometer-wide) storm.

This meanoeuvre will be humanity’s first close-up view of the gigantic storm being monitored since 1830 and possibly existing for more than 350 years on Jupiter, making it mysterious and puzzling.

“Jupiter’s mysterious Great Red Spot is probably the best-known feature of Jupiter,” said Scott Bolton, principal investigator of Juno from the Southwest Research Institute in San Antonio. “This monumental storm has raged on the solar system’s biggest planet for centuries. Now, Juno and her cloud-penetrating science instruments will dive in to see how deep the roots of this storm go, and help us understand how this giant storm works and what makes it so special,” said a NASA report.

The July 10 flyby will Juno’s sixth on to the gas giant’s mysterious cloud tops. Since Juno’s perijove is on Monday, July 10, at 6:55 pm PDT (9:55 pm EDT), Juno will be about 2,200 miles (3,500 kilometers) above the planet’s cloud tops.

In its closest reach lasting for 11 minutes and 33 seconds, Juno will cover another 24,713 miles (39,771 kilometers) and will be directly above the coiling crimson cloud tops of Jupiter’s Great Red Spot, said NASA. The spacecraft will bee about 5,600 miles (9,000 kilometers) above the Giant Red Spot clouds and all its 8 instruments and its camera JunoCam, will be directly on the storm during the flyby.

“The success of science collection at Jupiter is a testament to the dedication, creativity and technical abilities of the NASA-Juno team,” said Rick Nybakken, project manager for Juno from NASA’s Jet Propulsion Laboratory in Pasadena, California. “Each new orbit brings us closer to the heart of Jupiter’s radiation belt, but so far the spacecraft has weathered the storm of electrons surrounding Jupiter better than we could have ever imagined.”

As US is celebrating its Independence Day on July 4, Juno will have logged exactly one year in Jupiter orbit.

 

Cassini Takes Plunge Into Saturn, Scientists Cross-Fingered

In its line up for final plunge into Saturn’s atmosphere, Cassini has once again taken a proximal plunge into the surface of Saturn on June 29, 2017. The final plunge is scheduled for mid-September.

The Cosmic Dust Analyzer’s (CDA) science team, in Germany adjusted the instrument’s settings this week based on experience in recent “proximal” passages between Saturn’s rings and atmosphere. They have created a string of 39 commands that would set the instrument to make the best possible observations during the next proximal plunge. Now the instrument’s data-collection rate has been adjusted to 4 kilobits per second, thus making sure all ring-particle impacts would be sensed.

Here is a week-long update previous to the plunge:

Wednesday, June 21 (DOY 172)

Writers, bloggers, photographers, educators, students, artists and others who use social media to engage specific audiences are encouraged to apply for special access to Cassini’s Grand Finale event in mid-September.

Thursday, June 22 (DOY 173)

The Composite Infrared Spectrometer (CIRS) turned and looked at Saturn’s large icy moon Dione for 3.5 hours today. The Imaging Science Subsystem (ISS), the Visible and Infrared Mapping Spectrometer (VIMS), and the Ultraviolet Imaging Spectrograph (UVIS) – all the other Optical Remote-Sensing (ORS) instruments – rode along to make observations as well. CIRS’s goal was to measure Dione’s surface emissivity at thermal-infrared wavelengths, which hold clues to the composition and structure of that moon’s regolith.

Friday, June 23 (DOY 174)

Beginning late today, the spacecraft trained its High-Gain Antenna dish on the distant Earth. It then accurately tracked our planet for a total of 28 hours. Accordingly, the Radio Science Subsystem (RSS) team had Cassini power on its S-band (2 GHz) and Ka-band (32 GHz) radio transmitters, which directed their beams of energy out the HGA along with the main communications beam at X-band (8 GHz).

The result was a high-precision measurement of Saturn’s gravitation, which will be analyzed to reveal deviations from spherical symmetry.

Saturday, June 24 (DOY 175)

CIRS observed the dark side of Saturn’s A ring at far-infrared wavelengths for five hours today, with the other ORS instruments riding along. In addition to studying ring-particle compositions, the observation was part of a campaign to compare the spectral properties of ices among different regions of Saturn’s rings and icy moons.

Cassini and Titan happened to come close to one another today, to a distance about the same as that from Earth to our own Moon.

Sunday, June 25 (DOY 176)

This week’s Titan observing wrapped up with its final 4.3 hours devoted to observing clouds on the planet-like moon; VIMS rode along.

Monday, June 26 (DOY 177)

ISS turned and spent 7.7 hours observing Saturn’s irregular moon Bebhionn, an object of about six kilometers diameter, which orbits Saturn in an inclined ellipse that reaches as far as 25.1 million km from the planet. It might have a binary or contact-binary nature. Bebhionn was named after the goddess of birth in early Irish mythology.

The flight team held a Command Approval Meeting fine-tuning commands with consent from representatives from each of the affected spacecraft subsystems and instruments.

Tuesday, June 27 (DOY 178)

UVIS observed. Ten minutes after the Deep Space Network (DSN) station in Australia acquired Cassini’s downlink, its 18-kilowatt transmitter was turned on, and comands were sent. After a round-trip of 2 hours 31 minutes, telemetry confirmed that the commands had been received and were ready to take effect right before Cassini’s eleventh proximal plunge on June 29.

A total of 58 individual commands were uplinked, and about 1,625 megabytes of science and engineering telemetry data were downlinked and captured at rates as high as 142,201 bits per second.

Wrap up:

Cassini is executing its set of 22 Grand Finale Proximal orbits, which have a period of 6.5 days, in a plane inclined 61.9 degrees from the planet’s equatorial plane. Each orbit stretches out to an apoapsis altitude of about 1,272,000 km from Saturn, where the spacecraft’s planet-relative speed is around 6,000 km/hr. At periapsis, the distance shrinks to about 2,500 km above Saturn’s visible atmosphere on the planet’s total 120,660 km in diameter with a speed of 123,000 km/hr.

Mars Colony with Child Slaves? No Way, Says NASA Denying Ex-CIA Man’s Allegations

NASA has always been accused of wrong doing in space or hiding aliens or UFOs spotted in the sky and the US space agency has kept silent or denied very often any such conspiracy theories and the lastest one was Anonymous video and in less than a week another conspiracy theory has hit the agency.

In a bizarre revelation on Jones’ TV show , Robert David Steele, an erstwhile CIA officer proposed that kids have been secretly shipped to Mars in the last two decades to live and work as slaves. However, his contention had no evidence but enough of an allegation that forced NASA to deny it.

In his allegations, Steele said: “We actually believe that there is a colony on Mars that is populated by children who were kidnapped and sent into space on a 20-year ride. So that once they get to Mars they have no alternative but to be slaves on the Mars colony.”

Jones pointed out that 90 percent of NASA’s missions are secret and hence the allegations get credence. Soon, a NASA official gave a curt statement to the Daily Beast, which had published the allegation:

“There are no humans on Mars. There are active rovers on Mars. There was a rumor going around last week that there weren’t. There are,” said Guy Webster, a spokesperson for Mars exploration at NASA told the site. “But there are no humans,” he added categorically.

 

The “discovery” or allegation was made after showing an image on Mars that showed tracks, which looked like man-made.

NASA Denies Anonymous Video on Alien Life Discovery Announcement

US space agency NASA has denied global hackers group Anonymous claim that it is going make announcement on the discovery of alien life, said a spokesman.

Last week, the hacking group Anonymous posted a video on YouTube that said NASA is about to announce the discovery of life in our galaxy but NASA scientist beyond Earth.

“Contrary to some reports, there’s no pending announcement from NASA regarding extraterrestrial life,” said NASA science chief Thomas Zurbuchen in a tweet.

“Are we alone in the universe? While we do not know yet, we have missions moving forward that may help answer that fundamental question,” Zurbuchen said.

In fact, Anonymous has put out its video based on Zurbuchen’s testimony to the House of Representatives’ Committee on Science and Space in April this year. However, NASA has always maintained that there is no discovery of alien life and Anonymous video (see below) has surprised many.

Anonymous on their website said, “NASA says aliens are coming!” and  uploaded the above video citing alien-friendly comments made by NASA astronauts and space scientists.

Anonymous quoted Zurbuchen’s rendering before a Congressional hearing in April titled “Advances in the Search for Life” that said: “NASA`s recent advances, such as the discovery of hydrogen in Saturn`s moon Enceladus and the Hubble team’s promising results from the oceans of Jupiter`s moon Europa, are promising signs that we’re closer than ever to discovering evidence of alien life.”

“Taking into account all of the different activities and missions that are specifically searching for evidence of alien life, we are on the verge of making one of the most profound, unprecedented, discoveries in history,” Zurbuchen said. Perhaps the second part of the quote has made Anonymous see NASA forthcoming with an announcement.

 

 

 

NASA Successfully Tests Mini Methane Sensor for Future Mars Exploration

NASA researchers have developed a mini drone-like methane sensor that can fly and successfully tested it on a Vertical Take-off and Landing like any small unmanned aerial system (sUAS). The sensor, developed by JPL for use on Mars, will be used to detect methane with much higher sensitivity than previously available, especially in NASA’s next mission to Mars in 2018.

The tests were conducted in central California at the Merced Vernal Pools and Grassland Reserve, in partnership with Pipeline Research Council International (PRCI). The jointly conducted test of NASA’s Open Path Laser Spectrometer (OPLS) sensor also helps to detect methane in parts per billion by volume could help the pipeline industry more accurately pinpoint small methane leaks.

“These tests mark the latest chapter in the development of what we believe will eventually be a universal methane monitoring system for detecting fugitive natural-gas emissions and contributing to studies of climate change,” said Lance Christensen, OPLS principal investigator at JPL.

Researchers from JPL and the Mechatronics, Embedded Systems and Automation (MESA) Lab at the University of California, Merced, conducted the flight tests in late February. They flew a small unmanned aerial system equipped with the OPLS sensor at various distances from methane-emitting gas sources. Tests were done in a controlled setting to test the accuracy and robustness of the system, said NASA.

Next stage of testing later this year will feature a fixed-wing UAS, which can fly longer and farther so as to monitor natural-gas transmission pipeline systems, which are often hundreds of miles long and can be located in rural or remote areas.

A JPL mini methane gas sensor is flight tested on a small unmanned aerial system (sUAS) under a project to improve energy pipeline industry safety. The sensor enables methane detection with higher sensitivity than previously available for the industry in hand-carried or sUAS-deployable instruments.Credit: University of California, Merced.

NASA-Cassini Probe: Image of Titan’s Tallest Mountain Measuring 10948 Ft Mesmerizes

NASA’s Cassini probe mission has sent images of Saturn’s moon Titan showing some tallest mountains on its surface measuring more than 10,000 feet.

The mountainous ridges called the Mithrim Montes showed three series of mountain ridges and the top measured 10,948 feet in height. Most of these mountain ridges are located near the equator. The region is called Xanadu.

“It’s not only the highest point we’ve found so far on Titan, but we think it’s the highest point we’re likely to find,” said Stephen Wall of the Cassini radar team at NASA. Another observer of the Cassini radar team Jani Radebaugh said, “Titan’s extremes also tell us important things about forces affecting its evolution.”

The mountainous cliffs point at the evolution of a planet where forces have shoved the surface upward from underneath. Earth too has similar mountains and cliffs and the tallest mountain Everest is one such star example. The Himalaya and Andes Mountains still manifest such forces of nature underneath.

Cassini has found that Titan also has rain and rivers and some active tectonic forces causing quakes. Titan’s rotation, tidal forces from Saturn or cooling of the crust are some of its natural effects tied to this phenomenon.

Since its arrival in 2004, Cassini’s observations have changed whole dimension of saturn and its largest moon Titan. It has revealed that Titan’s surface is shaped by rivers and lakes of liquid ethane and methane, which forms clouds and causes occasional rains from the sky as water does on Earth. Winds sculpt vast regions of dark, hydrocarbon-rich dunes that girdle the moon’s equator and low latitudes, while volcanoes erupt spewing liquid water as the lava.

On its journey to Saturn, Cassini carried the European-built Huygens probe, which landed on Jan. 14, 2005, becoming humankind’s first landing on a body in the Outer Solar System when it parachuted through Titan’s murky skies. Currently, scientists are eager to get new data that could confirm the presence of a liquid ocean beneath the Titan’s surface.

Radar images do not present scenes as they would appear to human eyes but use radio waves beamed by the spacecraft that are reflected and scattered off of Titan’s surface in order to see through Titan’s opaque atmosphere. Bright regions indicate materials that are rough or that otherwise scatter the beam; dark regions indicate materials that are relatively smooth or that otherwise absorb radar waves. A side effect of this technique is the grainy pattern called “speckle” that typically is present in Cassini radar images.

This view was produced using a technique for handling noise in Cassini radar images, called despeckling, that produces clearer, easier-to-interpret views. Titan’s icy crust sits atop a deep ocean of liquid water that probably acts much like Earth’s upper mantle — the layer of hot, high-pressure rock below the crust that can slowly flow and deform over time.

This radar view was obtained on May 12, 2008 taken from a location at 2 degrees south latitude, 127 degrees west longitude. The incidence angle is about 34 degrees.

The Cassini-Huygens mission is a cooperative project of NASA, the European Space Agency and the Italian Space Agency. NASA’s Jet Propulsion Laboratory, a division of the California Institute of Technology in Pasadena, manages the mission for NASA’s Science Mission Directorate, Washington.