China starts 'combat ready' patrols in disputed South China Sea

The move comes amid rising tensions between China and its neighbors over disputed islands in the resource rich area.

By Ben Blanchard, Judy Hua, and David Stanway,?Reuters / June 28, 2012

A handout photo shows two Chinese surveillance ships which sailed between a Philippines warship and eight Chinese fishing boats to prevent the arrest of any fishermen in the Scarborough Shoal, in this April 10 photo.

Philippine Army/Reuters/File

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China has begun combat-ready patrols in the waters around a disputed group of islands in the South China Sea, the Defence Ministry said on Thursday, the latest escalation in tension over the potentially resource-rich area.

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Asked about what China would do in response to Vietnamese air patrols over the Spratly Islands, the ministry's spokesman, Geng Yansheng, said China would "resolutely oppose any militarily provocative behavior."

"In order to protect national sovereignty and our security and development interests, the Chinese military has already set up a normal, combat-ready patrol system in seas under our control," he said.

"The Chinese military's resolve and will to defend territorial sovereignty and protect our maritime rights and interests is firm and unshakeable," Mr. Geng added, according to a transcript on the ministry's website of comments at a briefing.

He did not elaborate. The ministry does not allow foreign reporters to attend its monthly briefings.

China is involved in long-running disputes with Vietnam and the Philippines about ownership of the South China Sea and its myriad, mostly uninhabited, islands and atolls. Taiwan, Malaysia and Brunei also have claims.

Last week, China said it "vehemently opposed" a Vietnamese law asserting sovereignty over the Paracel and Spratly Islands, which straddle key shipping lanes and are thought to contain rich energy reserves.

That row came days after an easing in a months-long standoff between China and the Philippines, but shows the persistent cycle of territorial frictions triggered by what some see as China's growing assertiveness in the area.

The South China Sea is potentially the biggest flashpoint for confrontation in Asia, and tensions have risen since the United States adopted a policy last year to reinforce its influence in the region.

At stake is control over what are believed to be significant reserves of oil and gas.

CNOOC, China's offshore oil specialist, said on its website last weekend that it would invite foreign partners to explore jointly and develop nine blocks in the western part of the South China Sea this year.

On Tuesday, Vietnam said CNOOC's plan was "illegal" and the blocks encroached on Vietnamese territorial waters.

At a regular briefing on Wednesday, China's Foreign Ministry spokesman, Hong Lei, insisted that the tenders were in accord with Chinese and international law and urged Vietnam not to escalate the dispute.

(Editing by Jeremy Laurence and Robert Birsel)

Source: http://rss.csmonitor.com/~r/feeds/csm/~3/-0QmZuTrbwg/China-starts-combat-ready-patrols-in-disputed-South-China-Sea

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Maintain Hygiene For Home Improvements | Home Improvement On ...

Home improvement seems to be a very important thing for you. Remodeling a house can leave you the room dirt. Maybe you will think how to keep your home in a clean condition when the work is being done. Do you have to remove all the items in your home?. Of course not. Suppose you?re fixing the bathroom, you do not have to remove the carpet.

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Original Post In >> HomeImprovementBiz.com >> Maintain Hygiene For Home Improvements

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Ugliest Dog contest: 'Mugly' had the name, now he gets the prize

Ugliest Dog contest:?Eight-year-old rescue dog 'Mugly' was declared the World?s Ugliest Dog at an annual competition in Petaluma, Calif., making him the latest Chinese crested to get the top prize.?

By Mounira Al Hmoud,?Christian Science Monitor / June 25, 2012

Mugly, a Chinese crested dog owned by Bev Nicholson of Peterborough, England, won the title of 'World's Ugliest Dog' at the Sonoma-Marin Fair in Petaluma, Calif., Friday.

The Press Democrat, Beth Schlanker/AP

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Mugly, a Chinese crested dog, bested 28 other contestants at the annual competition for the World?s Ugliest Dog in Petaluma, Calif., making him the latest Chinese crested to win the top prize. ?

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Judged for their ?natural ugliness in both pedigree and mutt classes,? Princess Abby, Handsome Hector, and Creature were not able to top the sheer unattractiveness of Mugly, with his short snout, beady eyes, and white whiskers.

Bev Nicholson, Mugly's owner who rescued him in the streets in the United Kingdom after the dog was abandoned by his family, told the Associated Press, "I couldn't speak when they announced Mugly's name."?

"I didn't know which way to look," she said. "I was shaking as much as the dog."

Mugly?s ugliness has long been recognized. In 2005, he was awarded the title of Britain?s ugliest dog. His looks do not, however, prevent him from holding down a job as a therapy dog for children.?

In addition to competing for international recognition, the British dog won a $1,000 prize and a year?s worth of dog cookies. He will also be invited for a photo shoot and a VIP stay at the local Sheraton.?

Last year?s winner at the Sonoma-Marin Fairgrounds, Yoda, was a Chinese crested and Chihuahua mix. Since the contest began in 2000, most of the winning dogs have been Chinese crested or Chinese crested and?Chihuahua mixes.?

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New way of probing exoplanet atmospheres

ScienceDaily (June 27, 2012) ? The planet Tau Bootis b [1] was one of the first exoplanets to be discovered back in 1996, and it is still one of the closest exoplanets known. Although its parent star is easily visible with the naked eye, the planet itself certainly is not, and up to now it could only be detected by its gravitational effects on the star. Tau Bootis b is a large "hot Jupiter" planet orbiting very close to its parent star.

Like most exoplanets, this planet does not transit the disc of its star (like the recent transit of Venus). Up to now such transits were essential to allow the study of hot Jupiter atmospheres: when a planet passes in front of its star it imprints the properties of the atmosphere onto the starlight. As no starlight shines through Tau Bootis b's atmosphere towards us, this means the planet's atmosphere could not be studied before.

But now, after 15 years of attempting to study the faint glow that is emitted from hot Jupiter exoplanets, astronomers have finally succeeded in reliably probing the structure of the atmosphere of Tau Bootis b and deducing its mass accurately for the first time. The team used the CRIRES [2] instrument on the Very Large Telescope (VLT) at ESO's Paranal Observatory in Chile. They combined high quality infrared observations (at wavelengths around 2.3 microns) [3] with a clever new trick to tease out the weak signal of the planet from the much stronger one from the parent star [4].

Lead author of the study Matteo Brogi (Leiden Observatory, the Netherlands) explains: "Thanks to the high quality observations provided by the VLT and CRIRES we were able to study the spectrum of the system in much more detail than has been possible before. Only about 0.01% of the light we see comes from the planet, and the rest from the star, so this was not easy."

The majority of planets around other stars were discovered by their gravitational effects on their parent stars, which limits the information that can be gleaned about their mass: they only allow a lower limit to be calculated for a planet's mass [5]. The new technique pioneered here is much more powerful. Seeing the planet's light directly has allowed the astronomers to measure the angle of the planet's orbit and hence work out its mass precisely. By tracing the changes in the planet's motion as it orbits its star, the team has determined reliably for the first time that Tau Bootis b orbits its host star at an angle of 44 degrees and has a mass six times that of the planet Jupiter in our own Solar System.

"The new VLT observations solve the 15-year old problem of the mass of Tau Bootis b. And the new technique also means that we can now study the atmospheres of exoplanets that don't transit their stars, as well as measuring their masses accurately, which was impossible before," says Ignas Snellen (Leiden Observatory, the Netherlands), co-author of the paper. "This is a big step forward."

As well as detecting the glow of the atmosphere and measuring Tau Bootis b's mass, the team has probed its atmosphere and measured the amount of carbon monoxide present, as well as the temperature at different altitudes by means of a comparison between the observations and theoretical models. A surprising result from this work was that the new observations indicated an atmosphere with a temperature that falls higher up. This result is the exact opposite of the temperature inversion -- an increase in temperature with height -- found for other hot Jupiter exoplanets [6] [7].

The VLT observations show that high resolution spectroscopy from ground-based telescopes is a valuable tool for a detailed analysis of non-transiting exoplanets' atmospheres. The detection of different molecules in future will allow astronomers to learn more about the planet's atmospheric conditions. By making measurements along the planet's orbit, astronomers may even be able to track atmospheric changes between the planet's morning and evening.

"This study shows the enormous potential of current and future ground-based telescopes, such as the E-ELT. Maybe one day we may even find evidence for biological activity on Earth-like planets in this way," concludes Ignas Snellen.

Notes

[1] The name of the planet, Tau Bootis b, combines the name of the star (Tau Bootis, or ? Bootis, ? is the Greek letter "tau," not a letter "t" ) with the letter "b" indicating that this is the first planet found around this star. The designation Tau Bootis a is used for the star itself.

[2] CRyogenic InfraRed Echelle Spectrometer

[3] At infrared wavelengths, the parent star emits less light than in the optical regime, so this is a wavelength regime favorable for separating out the dim planet's signal.

[4] This method uses the velocity of the planet in orbit around its parent star to distinguish its radiation from that of the star and also from features coming from Earth's atmosphere. The same team of astronomers tested this technique before on a transiting planet, measuring its orbital velocity during its crossing of the stellar disc.

[5] This is because the tilt of the orbit is normally unknown. If the planet's orbit is tilted relative to the line of sight between Earth and the star then a more massive planet causes the same observed back and forth motion of the star as a lighter planet in a less tilted orbit and it is not possible to separate the two effects.

[6] Thermal inversions are thought to be characterised by molecular features in emission in the spectrum, rather than in absorption, as interpreted from photometric observations of hot Jupiters with the Spitzer Space Telescope. The exoplanet HD209458b is the best-studied example of thermal inversions in the exoplanet atmospheres.

[7] This observation supports models in which strong ultraviolet emission associated to chromospheric activity -- similar to the one exhibited by the host star of Tau Bootis b -- is responsible for the inhibition of the thermal inversion.

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Story Source:

The above story is reprinted from materials provided by ESO.

Note: Materials may be edited for content and length. For further information, please contact the source cited above.

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Journal Reference:

1. Matteo Brogi, Ignas A. G. Snellen, Remco J. de Kok, Simon Albrecht, Jayne Birkby, Ernst J. W. de Mooij. The signature of orbital motion from the dayside of the planet ? Bo?tis b. Nature, 2012; 486 (7404): 502 DOI: 10.1038/nature11161

Note: If no author is given, the source is cited instead.

Disclaimer: Views expressed in this article do not necessarily reflect those of ScienceDaily or its staff.

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