The Red Paper: Canids Was NOT Meant To Earn ME Money.

Someone, who really has no idea and knows NOTHING about me, said that maybe my book Red Paper: Canids was a disappointment to me because it never made me any money?

Firstly, there is over 40 years of research in the book so it does NOT disappoint me.

Make ME money? That was never the intention. Any profits were to go to the UK Wolf Conservation Trust which does a LOT of educational work including with schools and The National Fox Welfare Society who do things like give advice on sick or injured foxes and FREE mange treatment.

 I am only disappointed (almost ashamed really) in that I have been unable to contribute to these two organisations.

 Terry Hooper

The Red Paper: Canids

Paperback, 

A4 (21 x 30cms)

202 Pages 

Photographs, illustrations and maps

Price: £10.29

Ships in 3–5 business days

 

 

 

By the 1700s the British fox was on the verge of extinction and about to follow the bear and wolf having been hunted for sport for centuries. 

 

The answer was to import thousands of foxes per year for sport. But foxes kept dying out so jackals were tried. Some were caught, some escaped. Even wolves and coyote were released for hunting and "country folk" were very far from "happy" -some even threatening local hunts -one intending to release a wolf for a hunt- with legal and other consequences.

 

The summation of over 40 years research by the noted naturalist and former UK police forces exotic wildlife consultant reveals the damnable lie of "pest control" hunting but also reveals the cruelty the animals were subject to and how private menageries as well as travelling shows.

 

Private menageries, or single exotic "pets" as well as travelling shows helped provide the British and Irish countryside with some incredible events such as the 1905 "vampiric" sheep killer of Badminton, the mystery hounds of Cavan and Coyotes of Epping Forest. 

 

The Girt Dog of Ennerdale is also dealt with in detail -was it a tiger? A Tasmania Thylacine? This book gives the exact facts and details for the first time.

Up-dated 2013 edition includes a section on sarcoptic mange in foxes and treatment plus a list of wildlife sanctuaries and rescue centres in the UK.

http://www.lulu.com/shop/terry-hooper/the-red-papercanines-vol1/paperback/product-20492038.html

"Wow!" Signal -Just Hydrogen?

I have to say that if -IF- a natural cause for the Wow! Signal was found it might seem sad but, again, you have to dismiss the false data to get to the True data.

A lot of Signals from Space that the AOP Bureau under Franklyn Angus Davin-Wilson looked into did have natural causes because planetary noise, pulsars and so on were not known at the time.  However, I have to agree that I am doubtful because of the hydrogen factor.  I can't see this being correct but....


https://www.newscientist.com/article/dn28747-famous-wow-signal-might-have-been-from-comets-not-aliens/?utm_source=NSNS&utm_medium=SOC&utm_campaign=hoot&cmpid=SOC|NSNS|2016-GLOBAL-twitter

Famous Wow! signal might have been from comets, not aliens

On 15 August 1977, radio astronomers using the Big Ear radio telescope at Ohio State University picked up a powerful signal from space. Some believe it was our first interception of an alien broadcast. Now it seems something closer to home may have been the source: a pair of passing comets.

The signal – known as the “Wow! signal” after a note scribbled by astronomer Jerry Ehman, who detected it – came through at 1420 megahertz, corresponding to a wavelength of 21 centimetres.

Searchers for extraterrestrial transmissions have long considered it an auspicious place to look, as it is one of the main frequencies at which atoms of hydrogen, the most common element in the universe, absorb and emit energy. What’s more, this frequency easily penetrates the atmosphere.

But in the 40 years since, we’ve never heard anything like it again. Analysis of the signal ruled out a satellite, and a reflected signal from the Earth’s surface is unlikely because regulations forbid transmission in that frequency range.

The signal’s intensity rose and fell over the course of 72 seconds, which is the length of time that the Big Ear could keep an object in its field of view due to the rotation of the Earth. That meant it was clearly coming from space. So what was it?

Antonio Paris, a professor of astronomy at St Petersburg College in Florida, thinks the signal might have come from one or more passing comets. He points the finger at two suspects, called 266P/Christensen and P/2008 Y2 (Gibbs). “I came across the idea when I was in my car driving and wondered if a planetary body, moving fast enough, could be the source,” he says.

Hydrogen clouds

Comets release a lot of hydrogen as they swing around the sun. This happens because ultraviolet light breaks up their frozen water, creating a cloud of the gas extending millions of kilometres out from the comet itself.


If the comets were passing in front of the Big Ear in 1977, they would have generated an apparently short-lived signal, as the telescope (now dismantled) had a fixed field of view. Searching that same area – as subsequent radio telescopes did – wouldn’t show anything. Tracing the comets’ positions back in time, Paris says that the possible origin for the Wow! signal falls right between where they would have been.

Neither comet was known in 1977; they were both discovered in the last decade, which would mean nobody would have thought to search for them. The odds of any telescope catching them in the region of the Wow! signal by chance were vanishingly small.

To test his idea, Paris proposes looking at the same region of space when the comets are back. Comet 266P/Christensen will transit the region first, on 25 January 2017, then P/2008 Y2 (Gibbs), on 7 January 2018. An analysis of the hydrogen signal of the comets should reveal if he is correct.

Doubts signalled

Some researchers are sceptical, saying it isn’t clear the comets would release enough hydrogen to generate something like the Wow! signal. James Bauer of the Jet Propulsion Laboratory in Pasadena, California, agrees that the hydrogen from comets can extend quite far, but still thinks the signal won’t be strong enough. “If comets were radio-bright at 21 centimetres, I would be puzzled as to why they aren’t observed more often at those wavelengths,” he says.

Paris says future observations will determine whether he is right. One crucial piece of evidence will be how fast the comets move across the sky. Too slow, and the Big Ear would have seen another signal 24 hours later as they rolled back into view, unlike the solo blast of the Wow! signal. “The hypothesis must be tested before it is ruled out,” he says. “Science 101.”

Journal reference: To appear in the Journal of the Washington Academy of Sciences, preprint

(Image credit: The Ohio State University Radio Observatory and the North American Astrophysical Observatory (NAAPO)

New Details on Ceres

Some great photos from NASA JPL. I'll say the bright spots are Cereseans with laser pointers!

New Details on Ceres Seen in Dawn Images

This image from NASA's Dawn spacecraft shows Kupalo Crater, one of the youngest craters on Ceres. Image Credit: NASA/JPL-Caltech/UCLA/MPS/DLR/IDA

Features on dwarf planet Ceres that piqued the interest of scientists throughout 2015 stand out in exquisite detail in the latest images from NASA's Dawn spacecraft, which recently reached its lowest-ever altitude at Ceres.

Dawn took these images near its current altitude of 240 miles (385 kilometers) from Ceres, between Dec. 19 and 23, 2015.

Kupalo Crater, one of the youngest craters on Ceres, shows off many fascinating attributes at the high image resolution of 120 feet (35 meters) per pixel. The crater has bright material exposed on its rim, which could be salts, and its flat floor likely formed from impact melt and debris. Researchers will be looking closely at whether this material is related to the "bright spots" of Occator Crater. Kupalo, which measures 16 miles (26 kilometers) across and is located at southern mid-latitudes, is named for the Slavic god of vegetation and harvest.

"This crater and its recently-formed deposits will be a prime target of study for the team as Dawn continues to explore Ceres in its final mapping phase," said Paul Schenk, a Dawn science team member at the Lunar and Planetary Institute, Houston.

Dawn's low vantage point also captured the dense network of fractures on the floor of 78-mile-wide (126-kilometer-wide) Dantu Crater. One of the youngest large craters on Earth's moon, called Tycho, has similar fractures. This cracking may have resulted from the cooling of impact melt, or when the crater floor was uplifted after the crater formed.


A 20-mile (32-kilometer) crater west of Dantu is covered in steep slopes, called scarps, and ridges. These features likely formed when the crater partly collapsed during the formation process. The curvilinear nature of the scarps resembles those on the floor of Rheasilvia, the giant impact crater on protoplanet Vesta, which Dawn orbited from 2011 to 2012.

Dawn's other instruments also began studying Ceres intensively in mid-December. The visible and infrared mapping spectrometer is examining how various wavelengths of light are reflected by Ceres, which will help identify minerals present on its surface.

Dawn's gamma ray and neutron detector (GRaND) is also keeping scientists busy. Data from GRaND help researchers understand the abundances of elements in Ceres' surface, along with details of the dwarf planet's composition that hold important clues about how it evolved.

The spacecraft will remain at its current altitude for the rest of its mission, and indefinitely afterward. The end of the prime mission will be June 30, 2016.

"When we set sail for Ceres upon completing our Vesta exploration, we expected to be surprised by what we found on our next stop. Ceres did not disappoint," said Chris Russell, principal investigator for the Dawn mission, based at the University of California, Los Angeles. "Everywhere we look in these new low- altitude observations, we see amazing landforms that speak to the unique character of this most amazing world."

Dawn is the first mission to visit a dwarf planet, and the first mission outside the Earth-moon system to orbit two distinct solar system targets. After orbiting Vesta for 14 months in 2011 and 2012, it arrived at Ceres on March 6, 2015.

Dawn's mission is managed by the Jet Propulsion Laboratory for NASA's Science Mission Directorate in Washington. Dawn is a project of the directorate's Discovery Program, managed by NASA's Marshall Space Flight Center in Huntsville, Alabama. UCLA is responsible for overall Dawn mission science. Orbital ATK Inc., in Dulles, Virginia, designed and built the spacecraft. The German Aerospace Center, Max Planck Institute for Solar System Research, Italian Space Agency and Italian National Astrophysical Institute are international partners on the mission team. For a complete list of mission participants, visit:


http://dawn.jpl.nasa.gov/mission
More information about Dawn is available at the following sites:
http://dawn.jpl.nasa.gov
http://www.nasa.gov/dawn