Strange Skies
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Moon

Moon is drifting away from Earth says NASA

Laser Reflector
© NASAA close-up photograph of the laser reflecting panel deployed by Apollo 14 astronauts on the Moon in 1971.
Dozens of times over the last decade NASA scientists have launched laser beams at a reflector the size of a paperback novel about 240,000 miles (385,000 kilometers) away from Earth. They announced today, in collaboration with their French colleagues, that they received signal back for the first time, an encouraging result that could enhance laser experiments used to study the physics of the universe.

The reflector NASA scientists aimed for is mounted on the Lunar Reconnaissance Orbiter (LRO), a spacecraft that has been studying the Moon from its orbit since 2009. One reason engineers placed the reflector on LRO was so it could serve as a pristine target to help test the reflecting power of panels left on the Moon's surface about 50 years ago. These older reflectors are returning a weak signal, which is making it harder to use them for science.

Scientists have been using reflectors on the Moon since the Apollo era to learn more about our nearest neighbor. It's a fairly straightforward experiment: Aim a beam of light at the reflector and clock the amount of time it takes for the light to come back. Decades of making this one measurement has led to major discoveries.

One of the biggest revelations is that the Earth and Moon are slowly drifting apart at the rate that fingernails grow, or 1.5 inches (3.8 centimeters) per year. This widening gap is the result of gravitational interactions between the two bodies.

"Now that we've been collecting data for 50 years, we can see trends that we wouldn't have been able to see otherwise," said Erwan Mazarico, a planetary scientist from NASA's Goddard Space Flight Center in Greenbelt, Maryland who coordinated the LRO experiment that was described on August 7 in the journal Earth, Planets and Space.

"Laser-ranging science is a long game," Mazarico said.

But if scientists are to continue using the surface panels far into the future, they need figure out why some of them are returning only a 10th of the expected signal.

Attention

Binary companion of our Sun postulated by Harvard

Nemesis
© M. WeissArtist's conception of a potential solar companion, which theorists believe was developed in the Sun's birth cluster and later lost. If proven, the solar companion theory would provide additional credence to theories that the Oort cloud formed as we see it today, and that Planet Nine was captured rather than formed in place.
Cambridge, MA - A new theory published today in The Astrophysical Journal Letters by scientists from Harvard University suggests that the Sun may once have had a binary companion of similar mass. If confirmed, the presence of an early stellar companion increases the likelihood that the Oort cloud was formed as observed and that Planet Nine was captured rather than formed within the solar system.

Dr. Avi Loeb, Frank B. Baird Jr. Professor of Science at Harvard, and Amir Siraj, a Harvard undergraduate student, have postulated that the existence of a long-lost stellar binary companion in the Sun's birth cluster — the collection of stars that formed together with the Sun from the same dense cloud of molecular gas — could explain the formation of the Oort cloud as we observe it today.

Popular theory associates the formation of the Oort cloud with debris left over from the formation of the solar system and its neighbors, where objects were scattered by the planets to great distances and some were exchanged amongst stars. But a binary model could be the missing piece in the puzzle, and according to Siraj, shouldn't come as a surprise to scientists. "Previous models have had difficulty producing the expected ratio between scattered disk objects and outer Oort cloud objects. The binary capture model offers significant improvement and refinement, which is seemingly obvious in retrospect: most Sun-like stars are born with binary companions."

If the Oort cloud was indeed captured with the help of an early stellar companion, the implications for our understanding of the solar system's formation would be significant. "Binary systems are far more efficient at capturing objects than are single stars," said Loeb. "If the Oort cloud formed as observed, it would imply that the Sun did in fact have a companion of similar mass that was lost before the Sun left its birth cluster."

Cloud Lightning

Magnificent red jellyfish sprite photographed during a storm in Mount Locke, Texas

Magnificent Red Jellyfish
© S. HummelMagnificent red jellyfish
Storm chasers are people who love to chase storms and witness how they unfold. While most of them want to see tornadoes, many storm chasers would go for thunderstorms and the delight of seeing cumulonimbus clouds and other related hail and lightning phenomena.

Some of them chase red sprites or the tentacle-like spurts of red lightning in the sky during a storm. They happen so fast that sometimes people would think they are only hallucinating. The European Space Agency said that these sprites are ultrafast electricity traveling through the atmosphere at 37 and 50 miles up and move toward space.


Cloud Grey

Strange cloud phenomenon captured over Ashville, Alabama

Strange cloud phenomenon over Ashville, Alabama
Strange cloud phenomenon over Ashville, Alabama
Thousands of people have shared a photo of clouds in the Ashville, Alabama sky yesterday and no one has been able to identify a reason for the strange phenomenon. Townsquare Media Tuscaloosa and ABC 33/40 Chief Meteorologist James Spann shared the photo set on Sunday evening, submitted by Facebook user Joshua Smith. Smith said he took the pictures on Interstate 59 near Ashville.


Cloud Precipitation

Adapt 2030 Ice Age Report: Why is so much rain happening globally?

The Kwanyin temple built on a rocky island in the middle of the Yangtze River is seen flooded as the water level surge along Ezhou in central China's Hubei province
© Chinatopix Via APThe Kwanyin temple built on a rocky island in the middle of the Yangtze River is seen flooded as the water level surge along Ezhou in central China's Hubei province on Sunday, July 19, 2020.
Summer snow in Beijing China, Red Noctilucent Clouds first time ever seen as a disturbance in the ozone layer commences, hundreds of record rain and 500 year+ floods events through July 2020. Cosmic Ray increases seem to play a large part, and the increases are just beginning as the Eddy Grand Solar Minimum intensifies.


Comment: See also:


Sun

Breakthrough method for predicting solar storms says study

Sun's Corona
© NASAImage of corona from NASA's Solar Dynamics Observatory showing features created by magnetic fields.
Extensive power outages and satellite blackouts that affect air travel and the internet are some of the potential consequences of massive solar storms. These storms are believed to be caused by the release of enormous amounts of stored magnetic energy due to changes in the magnetic field of the sun's outer atmosphere - something that until now has eluded scientists' direct measurement. Researchers believe this recent discovery could lead to better "space weather" forecasts in the future.

"We are becoming increasingly dependent on space-based systems that are sensitive to space weather. Earth-based networks and the electrical grid can be severely damaged if there is a large eruption", says Tomas Brage, Professor of Mathematical Physics at Lund University in Sweden.

Solar flares are bursts of radiation and charged particles, and can cause geomagnetic storms on Earth if they are large enough. Currently, researchers focus on sunspots on the surface of the sun to predict possible eruptions. Another and more direct indication of increased solar activity would be changes in the much weaker magnetic field of the outer solar atmosphere - the so-called Corona.

However, no direct measurement of the actual magnetic fields of the Corona has been possible so far.

Mars

Elongated long cloud has reappeared over Martian volcano

Long Cloud Over Mars
© ESA/GCP/UPV/EHU Bilbao
A mysteriously long, thin cloud has again appeared over the 20-km high Arsia Mons volcano on Mars.

A recurrent feature, the cloud is made up of water ice, but despite appearances it is not a plume linked to volcanic activity. Instead, the curious stream forms as airflow is influenced by the volcano's 'leeward' slope − the side that does not face the wind.

These images of the cloud, which can reach up to 1800-km in length, were taken on 17 and 19 July by the Visual Monitoring Camera (VMC) on Mars Express, which has been studying the Red Planet from orbit for the past 16 years.

"We have been investigating this intriguing phenomenon and were expecting to see such a cloud form around now," explains Jorge Hernandez-Bernal, PhD candidate at the University of the Basque Country (Spain) and lead author of the ongoing study.

"This elongated cloud forms every martian year during this season around the southern solstice, and repeats for 80 days or even more, following a rapid daily cycle. However, we don't know yet if the clouds are always quite this impressive".

Cassiopaea

Rare red noctilucent clouds photographed over Sweden

red noctilucent cloud sweden
© P-M HedénScreenshot: Red NLCs over Vallentuna, Sweden. July 25, 2020.
Noctilucent clouds (NLCs) are supposed to be electric blue. This past weekend in Sweden, photographer P-M Hedén saw a different color: Dark Red. "My 17 year-old son was out with friends and he texted me the message 'Noctilucent!' I looked out and didn't really understand what I saw. The tops of the clouds were red."

Hedén hopped in his car and drove to a clear site for a better look. The movie he made, above, shows the dynamics of the clouds and the development of their amber crown. "This all happened around local midnight," he says.

NLCs are Earth's highest clouds. Seeded by meteoroids, they float at the edge of space 83 km above the ground. Hedén's video shows ordinary clouds scudding dark and low across the Swedish landscape. NLCs float high overhead, catching the rays of the sun, which is still "up" at their extremely high altitude.

Comment: It's notable that the most recent sighting of rare red NLC's was just last year, because rare phenomena of all kinds appear to be on the increase in recent years: And check out SOTT radio's:


Info

Rare supernova in Draco may explain how white dwarfs explode

Rare Supernova
© Northwestern UniversityThe blue dot marks the approximate location of the supernova event.
Astrophysicists have spotted a spectacular flash of ultraviolet light accompanying a white dwarf explosion.

It's only the second time such a rare type of supernova has been seen, they say, and may help explain how white dwarfs explode.

The flash "is telling us something very specific", says Adam Miller from Northwestern University, US, the lead author of a paper in in the Astrophysical Journal.

"As time passes, the exploded material moves farther away from the source. As that material thins, we can see deeper and deeper.

"After a year, the material will be so thin that we will see all the way into the centre of the explosion."

Using the Zwicky Transient Facility in California, the researchers spotted the event, named SN2019yvq, just a day after it occurred last December in a galaxy about 140 million light-years from Earth and very close to the tail of the dragon-shaped Draco constellation.

They quickly studied it in ultraviolet and X-ray wavelengths using NASA's Neil Gehrels Swift Observatory and classified it as a type Ia supernova.

Cassiopaea

Bright Nova Reticuli 2020 discovered by astronomer

Nova Reticuli 2020
© Remanzacco Blogspot
Following the posting on the CBET 4811 & 4812 about the NOVA RETICULI 2020 we performed some follow-up of this object through a TEL 0.1-m f/3.6 astrograph + CCD located in the Heaven's Mirror Observatory, Australia (MPC code Q56) and operated by Telescope Live network.
On images taken on July 16.82, 2020 we can confirm the presence of an optical counterpart (with R-filtered magnitude about +4.5; B-filtered magn. +5.6; V-filtered magn. +5.6) at coordinates:

R.A. = 03 58 29.61, Decl.= -54 46 39.8

(equinox 2000.0; Gaia DR2 catalogue reference stars for the astrometry).

This transient was discovered by Robert H. McNaught (Coonabarabran, NSW, Australia) as an apparent 5th-magnitude nova on CCD images obtained on July 15.590 UT with a Canon 6D camera and an 8-mm-f.l. f/2.8 lens (at ISO 800). The position is very close to an object listed as "MGAB-V207" in the AAVSO's VSX online database (which gives position R.A. = 3h58m29s.55, Decl. = -54d46'41".2, equinox J2000.0, which calls it a novalike "VY Scl"-type variable with V magnitude range 15.8-18.0).

Spectroscopy by E. Aydi et al. (ATel #13867) using the High Resolution Spectrograph (HRS) mounted on the 11m Southern African Large Telescope as part of the SALT Large Science Program on Transients shows a spectrum that resembles that of a classical nova, likely after optical peak. Also, R. Kaufman (Bright, VIC, Australia) reports a low-resolution spectrum obtained by him on 2020 Jul. 16.62 UT (with a Canon 800D camera + 200-mm-f.l. f/3.5 lens) indicates the object to be a "Fe II-type" classical nova.