Thursday, 28 February 2013

Are Online Relationships Healthy for Young People? | Dr. Jim Taylor ...

More and more these days, young people are establishing and maintaining relationships online. These ?cyber? relationships often arise because parents, out of fear for their children?s safety, no longer allow them to be ?free range? to congregate in local parks, at malls, and on street corners. The only place that they have permission to ?meet up? is in virtual gathering such as Facebook, Twitter, and in the ?textosphere.? Plus, the reality is that your children are growing up as natives in this digital world, so it is only natural that they spend some of their time in cyberspace.

There are several questions that you must ask as your children immerse themselves in this connected world. First, are the relationships that they build online are healthy or harmful? Second, do they foster your children?s long-term positive development? Third, given that disconnecting them from this virtual world is unrealistic, how can you ensure that their online relationships are positive and life-affirming?

To be sure, many young people these days have well-developed virtual relationships that they consider real. Virtual relationships have all the appearances of real relationships, for example, connectedness, communication, and sharing. Yet, these relationships are missing essential elements that distinguish them from flesh-and-blood relationships, namely, three dimensionality, facial expressions, voice inflection, clear emotional messages, gestures, body language, physical contact, and pheromones.

Online relationships are based on limited information and, as a result, are incomplete; your children can know people online, but only so far. When connecting with others through technology, your children get bits and pieces of people?words on a screen, two-dimensional images, or a digitized voice?almost like having some, but not all, of the pieces of a puzzle. Your children get a picture of others, but they lack the pieces your children need to get a complete picture of that person.

Users of social media tend to present themselves online in ways that are, at a minimum, slightly more positive impressions of their true selves and, at a maximum, entirely distorted and aggrandized self-representations. This type of ?impression management? is much easier to do online because recipients of the information aren?t in a position to reality test what they see, read, and hear.

There are several problems with this common online practice. First, it prevents children from acknowledging and accepting that they are imperfect beings like everyone else. Nor can they learn that, despite their flaws, they are still good people worthy of being valued and liked. It is also, intentionally or otherwise, dishonest, not generally a lesson that parents want their children to learn.

As relationships develop online, this practice doesn?t allow the receivers of this information to make reasoned judgments about the kind of relationship they want with the sender of the information. Additionally, this practice, interestingly enough, may deter senders of the less-than-accurate information from migrating an online relationship to a real relationship because then they would be discovered to be imposters.

Impression management is an essential motivator among children to meet their needs for self-esteem and social acceptance. It is also a common practice that children engage in both on and offline. Yet, the ability of children to shape how others view them is much greater online than offline because there is no direct way for others to assess the truth behind the impressions that children present through cyberspace.

The brevity of online communication also mitigates the opportunity for the development of deep relationships. Most forms of social networking, for example, Facebook, Twitter, and texting, involve short and frequent communications that simply don?t provide the platform for the rich sharing of thoughts and emotions, which happen to be the superstructure of relationships.

In addition to the concerns I?ve just expressed, the simple calculus of life is that time spent in online relationships is time not being spent in face-to-face relationships. The lack of experience in engaging in real relationships can hurt your children?s ability to develop healthy relationships in the future. Think of it this way. Relationships arise through experience and require certain skills, for example, reading facial expressions, interpreting voice inflection, and feeling empathy. If your children are missing out on flesh-and-blood relationships because they spend so much time online, then they are also missing out on those opportunities to learn about and practice those skills that enable healthy relationships to develop.

It?s probably no coincidence that the dramatic rise in narcissism and decline in empathy over the past few decades has occurred along side the rise of the information age and the devotion of young people?s time to online pursuits. Of course, your children do engage in plenty of real relationships at home, with friends, and at school and in their other activities. But increasingly, today?s children are spending a significant portion of their days on line; they devote, on average, more than seven-and-a-half hours interacting with non-school-related technology. As a result, time in real relationships may be far less than you think and far less than children in past generations had. In a sense, children these days have less time to ?practice? relationships and, with less practice, they are going be less skilled at them.

These limitations don?t mean that children shouldn?t have virtual relationships; they can serve a valuable purpose in both children?s social lives. The concern is that, with so much time spent online, children are substituting direct relationships for virtual ones. Rather than being just a small subset of their relationships, unguided and unfettered virtual relationships may come to dominate their relationship universe. For example, I often see groups of teenagers sitting together, but not talking, only texting. I wonder if they?re texting each other!

So what is the attraction of online relationships for children? On the plus side, social networking allows children to stay in regular touch with their friends, which is particularly important for children who don?t see each other in school every day. Cyberspace can act as a meeting place for introductions to new friends that then transfer to actual social interactions. Online relationships can help children get beyond the ill ease that can occur when they first meet by allowing them to get to know each other before they meet in person. They are also a way for children who are shy or socially anxious to practice their ?people skills? and gain comfort with new friends before they use those skills in flesh-and-blood relationships.

At the same time, online relationships may provide a bubble of safety and comfort in a social world that can be scary for children. We live in a society in which families are no longer nuclear, communities are fragmented, and children can feel isolated and disenfranchised. A popular culture that venerates ?bad boys? and ?mean girls? can create feelings of alienation and anxiety. Fears of inadequacy, rejection, and failure, heightened by a popular culture that reveres perfection, popularity, and success, add to the maelstrom of personal angst that children can feel as they explore relationships. Children who are thrown into this cauldron without adequate support or the necessary skills can feel compelled to stay in the cocoon of their own room and connect with people safely through your computer, tablet, or smartphone.

The reality is that children can fulfill many of their needs for connection, affiliation, and affirmation through virtual relationships, however limited and potentially unhealthy that route may be. In doing so, they can come to believe that their needs for friendship and intimacy can be met online without all of the risks and messiness of real-world relationships. The problem is that the absence of messiness also precludes children from experiencing the deep benefits of fully realized relationships that can only exist offline.

You as parents should be cognizant of the quality and quantity of the online relationships that your children are engaged in. I am certainly not advocating that you cut off your children from these relationships. At the same time, their virtual relationships should supplement, not replace, their face-to-face relationship. In sum, I would suggest that the amount of time that your children devote to flesh-and-blood relationships should far outweigh the time spent in online relationships.

Source: http://blog.seattlepi.com/jimtaylor/2013/02/27/are-online-relationships-healthy-for-young-people/

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Wednesday, 27 February 2013

TBS orders Pete Holmes late-night show; Conan O'Brien to produce

LOS ANGELES (TheWrap.com) - Pete Holmes, voice of the beloved E*Trade baby and host of the "You Made It Weird" podcast, is coming to TBS with a late-night comedy show, the network said Tuesday.

The as-yet-untitled series, which has received a four-week order, will premiere in the fall and will air at midnight following "Conan" Monday through Thursday.

Conan O'Brien is executive producing through Conaco LLC, which is producing the series. Jeff Ross, David Kissinger, Nick Bernstein and Dave Rath are also executive producing the show, which will be taped in front of a live audience.

The half-hour series will combine sketches, short films, live comedy, field pieces and in-studio guest interviews.

"The first half of my meeting with Conan was spent making sure this wasn't all part of a new TBS prank show called You Got Coned!" Holmes joked of the new gig. "The second half was spent expressing my sincerest enthusiasm and gratitude for this incredible dream come true."

"Pete Holmes is an enormously likable performer with an agile and innovative mind," OBrien added. "I'm really looking forward to his show, and I've already had my son program my DVR."

Source: http://news.yahoo.com/tbs-orders-pete-holmes-night-show-conan-obrien-213338102.html

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Monday, 25 February 2013

Future evidence for extraterrestrial life might come from dying stars

Future evidence for extraterrestrial life might come from dying stars [ Back to EurekAlert! ] Public release date: 25-Feb-2013
[ | E-mail | Share Share ]

Contact: Christine Pulliam
cpulliam@cfa.harvard.edu
617-495-7463
Harvard-Smithsonian Center for Astrophysics

Even dying stars could host planets with life - and if such life exists, we might be able to detect it within the next decade. This encouraging result comes from a new theoretical study of Earth-like planets orbiting white dwarf stars. Researchers found that we could detect oxygen in the atmosphere of a white dwarf's planet much more easily than for an Earth-like planet orbiting a Sun-like star.

"In the quest for extraterrestrial biological signatures, the first stars we study should be white dwarfs," said Avi Loeb, theorist at the Harvard-Smithsonian Center for Astrophysics (CfA) and director of the Institute for Theory and Computation.

When a star like the Sun dies, it puffs off its outer layers, leaving behind a hot core called a white dwarf. A typical white dwarf is about the size of Earth. It slowly cools and fades over time, but it can retain heat long enough to warm a nearby world for billions of years.

Since a white dwarf is much smaller and fainter than the Sun, a planet would have to be much closer in to be habitable with liquid water on its surface. A habitable planet would circle the white dwarf once every 10 hours at a distance of about a million miles.

Before a star becomes a white dwarf it swells into a red giant, engulfing and destroying any nearby planets. Therefore, a planet would have to arrive in the habitable zone after the star evolved into a white dwarf. A planet could form from leftover dust and gas (making it a second-generation world), or migrate inward from a larger distance.

If planets exist in the habitable zones of white dwarfs, we would need to find them before we could study them. The abundance of heavy elements on the surface of white dwarfs suggests that a significant fraction of them have rocky planets. Loeb and his colleague Dan Maoz (Tel Aviv University) estimate that a survey of the 500 closest white dwarfs could spot one or more habitable Earths.

The best method for finding such planets is a transit search - looking for a star that dims as an orbiting planet crosses in front of it. Since a white dwarf is about the same size as Earth, an Earth-sized planet would block a large fraction of its light and create an obvious signal.

More importantly, we can only study the atmospheres of transiting planets. When the white dwarf's light shines through the ring of air that surrounds the planet's silhouetted disk, the atmosphere absorbs some starlight. This leaves chemical fingerprints showing whether that air contains water vapor, or even signatures of life, such as oxygen.

Astronomers are particularly interested in finding oxygen because the oxygen in the Earth's atmosphere is continuously replenished, through photosynthesis, by plant life. Were all life to cease on Earth, our atmosphere would quickly become devoid of oxygen, which would dissolve in the oceans and oxidize the surface. Thus, the presence of large quantities of oxygen in the atmosphere of a distant planet would signal the likely presence of life there.

NASA's James Webb Space Telescope (JWST), scheduled for launch by the end of this decade, promises to sniff out the gases of these alien worlds. Loeb and Maoz created a synthetic spectrum, replicating what JWST would see if it examined a habitable planet orbiting a white dwarf. They found that both oxygen and water vapor would be detectable with only a few hours of total observation time.

"JWST offers the best hope of finding an inhabited planet in the near future," said Maoz.

Recent research by CfA astronomers Courtney Dressing and David Charbonneau showed that the closest habitable planet is likely to orbit a red dwarf star (a cool, low-mass star undergoing nuclear fusion). Since a red dwarf, although smaller and fainter than the Sun, is much larger and brighter than a white dwarf, its glare would overwhelm the faint signal from an orbiting planet's atmosphere. JWST would have to observe hundreds of hours of transits to have any hope of analyzing the atmosphere's composition.

"Although the closest habitable planet might orbit a red dwarf star, the closest one we can easily prove to be life-bearing might orbit a white dwarf," said Loeb.

###



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Future evidence for extraterrestrial life might come from dying stars [ Back to EurekAlert! ] Public release date: 25-Feb-2013
[ | E-mail | Share Share ]

Contact: Christine Pulliam
cpulliam@cfa.harvard.edu
617-495-7463
Harvard-Smithsonian Center for Astrophysics

Even dying stars could host planets with life - and if such life exists, we might be able to detect it within the next decade. This encouraging result comes from a new theoretical study of Earth-like planets orbiting white dwarf stars. Researchers found that we could detect oxygen in the atmosphere of a white dwarf's planet much more easily than for an Earth-like planet orbiting a Sun-like star.

"In the quest for extraterrestrial biological signatures, the first stars we study should be white dwarfs," said Avi Loeb, theorist at the Harvard-Smithsonian Center for Astrophysics (CfA) and director of the Institute for Theory and Computation.

When a star like the Sun dies, it puffs off its outer layers, leaving behind a hot core called a white dwarf. A typical white dwarf is about the size of Earth. It slowly cools and fades over time, but it can retain heat long enough to warm a nearby world for billions of years.

Since a white dwarf is much smaller and fainter than the Sun, a planet would have to be much closer in to be habitable with liquid water on its surface. A habitable planet would circle the white dwarf once every 10 hours at a distance of about a million miles.

Before a star becomes a white dwarf it swells into a red giant, engulfing and destroying any nearby planets. Therefore, a planet would have to arrive in the habitable zone after the star evolved into a white dwarf. A planet could form from leftover dust and gas (making it a second-generation world), or migrate inward from a larger distance.

If planets exist in the habitable zones of white dwarfs, we would need to find them before we could study them. The abundance of heavy elements on the surface of white dwarfs suggests that a significant fraction of them have rocky planets. Loeb and his colleague Dan Maoz (Tel Aviv University) estimate that a survey of the 500 closest white dwarfs could spot one or more habitable Earths.

The best method for finding such planets is a transit search - looking for a star that dims as an orbiting planet crosses in front of it. Since a white dwarf is about the same size as Earth, an Earth-sized planet would block a large fraction of its light and create an obvious signal.

More importantly, we can only study the atmospheres of transiting planets. When the white dwarf's light shines through the ring of air that surrounds the planet's silhouetted disk, the atmosphere absorbs some starlight. This leaves chemical fingerprints showing whether that air contains water vapor, or even signatures of life, such as oxygen.

Astronomers are particularly interested in finding oxygen because the oxygen in the Earth's atmosphere is continuously replenished, through photosynthesis, by plant life. Were all life to cease on Earth, our atmosphere would quickly become devoid of oxygen, which would dissolve in the oceans and oxidize the surface. Thus, the presence of large quantities of oxygen in the atmosphere of a distant planet would signal the likely presence of life there.

NASA's James Webb Space Telescope (JWST), scheduled for launch by the end of this decade, promises to sniff out the gases of these alien worlds. Loeb and Maoz created a synthetic spectrum, replicating what JWST would see if it examined a habitable planet orbiting a white dwarf. They found that both oxygen and water vapor would be detectable with only a few hours of total observation time.

"JWST offers the best hope of finding an inhabited planet in the near future," said Maoz.

Recent research by CfA astronomers Courtney Dressing and David Charbonneau showed that the closest habitable planet is likely to orbit a red dwarf star (a cool, low-mass star undergoing nuclear fusion). Since a red dwarf, although smaller and fainter than the Sun, is much larger and brighter than a white dwarf, its glare would overwhelm the faint signal from an orbiting planet's atmosphere. JWST would have to observe hundreds of hours of transits to have any hope of analyzing the atmosphere's composition.

"Although the closest habitable planet might orbit a red dwarf star, the closest one we can easily prove to be life-bearing might orbit a white dwarf," said Loeb.

###



[ Back to EurekAlert! ] [ | E-mail | Share Share ]

?


AAAS and EurekAlert! are not responsible for the accuracy of news releases posted to EurekAlert! by contributing institutions or for the use of any information through the EurekAlert! system.


Source: http://www.eurekalert.org/pub_releases/2013-02/hcfa-fef022513.php

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Thursday, 14 February 2013

Disney Cruise Announces New Ports for 2014 | Leisure Group Travel

In 2014, Disney Cruise Line will offer new itineraries, including an expanded collection of European cruises highlighting the Greek Isles. Plus, Disney Cruise Line will depart for the first time from homeports in Venice, Italy and San Juan, Puerto Rico.

Mediterranean from Venice and Barcelona
From May to August 2014, the Disney Magic returns to the Mediterranean, using Venice, Italy as a homeport for select sailings. During these cruises, the Disney Magic overnights in Venice.

The line also will visit new destinations in the Greek Isles and Sicily for the very first time, including Katakolon, Rhodes, Heraklion (Crete), Santorini and Corfu, Greece and Catania, Sicily.

Southern Caribbean from San Juan
Disney Cruise Line will homeport in San Juan for the first time in 2014. The Disney Magic will sail four cruises to the Southern Caribbean, including Grenada ? a new port of call for Disney. Other ports on seven-night cruises include Antigua, St. Lucia, Barbados and St. Kitts, with departures on Sept. 20 and 27 and Oct. 4 and 11.

Alaska from Vancouver
In 2014 the Disney Wonder will sail seven-night cruises from Vancouver to Tracy Arm, Skagway, Juneau and Ketchikan, Alaska. One special nine-night cruise calls on Sitka, Alaska ? a first for Disney Cruise Line.

Bahamas and Western Caribbean from Miami
In 2014 Disney Cruise Line will sail from Miami on four-night Bahamian and five-night Western Caribbean cruises. The Disney Wonder sails from January to April, the Disney Magic October to December.

Caribbean and Bahamas from Port Canaveral
The line will sail from Port Canaveral to the Caribbean and Bahamas on a variety of itineraries in 2014.? Every cruise departing from Port Canaveral includes a stop at Disney?s private island, Castaway Cay.
(www.disneycruise.com)

Source: http://leisuregrouptravel.com/disney-cruise-announces-new-ports-for-2014/

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Microsoft suggests fix for iOS 6.1/Exchange problem: Block iPhone users

That's one way to disable an iPhone.

iOS 6.1 devices are hammering Exchange servers with excessive traffic, causing performance slowdowns that led Microsoft to suggest a drastic fix for the most severe cases: throttle traffic from iOS 6.1 users or block them completely.

"When a user syncs a mailbox by using an iOS 6.1-based device, Microsoft Exchange Server 2010 Client Access server (CAS) and Mailbox (MBX) server resources are consumed, log growth becomes excessive, memory and CPU use may increase significantly, and server performance is affected," Microsoft wrote on Tuesday in a support document.

The problem also affects Exchange Online in Microsoft's Office 365 cloud service. Office 365 customers may get an error message on iOS 6.1 devices stating "Cannot Get Mail: The connection to the server failed." The Microsoft support article says both Apple and Microsoft are investigating the problem.

Microsoft suggests several fixes, starting out gently, then escalating to the complete blockage of iOS 6.1 devices. Based on the fixes suggested, the problems may be caused when iOS devices connect to Exchange calendars.

The first workaround is "do not process Calendar items such as meeting requests on iOS 6.1 devices. Also, immediately restart the iOS 6.1 device."

If that doesn't work, users are instructed to remove their Exchange accounts from their phones or tablets while the Exchange Server administrator runs a "remove device" command on the server side.?After 30 minutes, users can add the Exchange accounts back onto their devices but should be advised "not to process Calendar items on the device."

If that doesn't work, the fixes get more serious. The next method is for the server administrator to create a custom throttling policy limiting the number of transactions iOS 6.1 users can make with the server. "The throttling policy will reduce the effect of the issue on server resources," Microsoft notes. "However, users who receive the error should immediately restart their devices and stop additional processing of Calendar items."

One Exchange administrator who created a throttling policy through PowerShell to solve the problem provides a guide here, but Microsoft also has a page providing instructions.

Finally, the last method Microsoft recommends is to block iOS 6.1 users. "You can block iOS 6.1 users by using the Exchange Server 2010 Allow/Block/Quarantine feature," Microsoft notes. (See this post for more detailed instructions.)

We don't know exactly how widespread this problem is. It's clearly not affecting everyone, but the impact seems to run the gamut from small businesses to large.

"We're using Exchange 2010 in a small software firm with about a dozen iOS users (each with multiple iOS devices)," Shourya Ray, chief administrative officer of Spin Systems in Virginia, told Ars via e-mail. "Last week our Exchange server froze (internal mail was being routed, but external mail stopped flowing)."

It turned out that the 300GB VMware virtual machine hosting the Exchange server was full. "You can imagine our surprise when that VM filled up overnight," Ray said. "If we were running Exchange in a typical hardware-based server with a 1TB drive, it would have taken us a week to realize the problem."

How did it happen, and how did the company get things working "normally" again? "The transaction log had 200,000 records and was the indication of a problem," Ray said. "Our temporary solution has been to ask iOS users to switch to manual pull rather than ActiveSync push. For heavy e-mail users, we are recommending an automatic pull every 30 minutes. So far, that seems to have kept Exchange happy with no other issues since last week. Let's hope that Apple and Microsoft put their heads to together and fix this soon."

We heard from several other people on Twitter that they have been bit by the iOS 6.1/Exchange problem. One said, "My 22,000+ employee enterprise has blocked iOS 6.1, execs all have iOS."

A support thread on Microsoft's Exchange Server site was opened January 31 to discuss the excessive logging caused by iOS 6.1. The server administrator who began the thread identified an iPad that "caused over 50GB worth of logs" on a single database.

The thread got more than a dozen replies. One Exchange administrator explained that "malformed meetings on a device cause the device to get into a sync loop which causes excessive transaction log growth on the Exchange mailbox servers." This in turn "will cause Exchange performance issues and potentially transaction log drives to run out of disk space which would then bring down Exchange."

To solve the problem, this admin simply "disabled all iOS 6.1 on our Exchange system."

iOS 6.1 was released on January 28. iOS 6.1.1 came out a couple of days ago, but for now it can only be installed on the iPhone 4S and is designed to fix cellular performance and reliability. Apple didn't mention anything about Exchange fixes when releasing this latest version.?Last year, iOS 6.0.1 fixed an Exchange problem that could lead to entire meetings being canceled when even a single iOS user declined a meeting invitation.

The iOS 6.1 problem isn't the first time iOS has caused Exchange servers to perform poorly. An Apple support article from 2010 describes sync problems in iOS 4 and says, "Exchange Server administrators may notice their servers running slowly." At the time,?Microsoft noted iOS 4 led to "Exchange administrators... seeing heavier than normal loads on their servers from users with iOS devices." Microsoft got in touch with Apple to fix that problem.

We've asked both Apple and Microsoft how many users are impacted by the latest problem, and when a more permanent fix is coming. We also asked Apple if it agrees with the workarounds suggested by Microsoft. Microsoft told us it has nothing else to say, as the "support article contains the latest." Apple has not responded to our request for comment as of yet.

UPDATE: Apple posted a support document of its own today,?describing the problem thusly:

When you respond to an exception to a recurring calendar event with a Microsoft Exchange account on a device running iOS 6.1, the device may begin to generate excessive communication with Microsoft Exchange Server. You may notice increased network activity or reduced battery life on the iOS device. This extra network activity will be shown in the logs on Exchange Server and it may lead to the server blocking the iOS device. This can occur with iOS 6.1 and Microsoft Exchange 2010 SP1 or later, or Microsoft Exchange Online (Office365).

Apple's suggested fix is to turn the Exchange calendar off and back on again within the iPhone's settings. An operating system update to fix the problem is on the way. "Apple has identified a fix and will make it available in an upcoming software update," Apple said.

Source: http://arstechnica.com/information-technology/2013/02/microsoft-suggests-fix-for-ios-6-1exchange-problem-block-iphone-users/

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Michelle Jenneke Sports Illustrated Video: Australian Hurdler Jumps Into Swimsuit Modeling

When it comes to expanding her celebrity, Michelle Jenneke still has some wiggle room. The Australian hurdler now appears in the Sports Illustrated Swimsuit Issue, and those interested in getting a behind-the-scenes look at her photo shoot can watch the video above.

Jenneke, 19, has used her killer smile, world-class bod and YouTube fame off her pre-race bouncing at the IAAF World Junior Championship last summer to overcome moderate cred as a competitor. (She's still more than a second slower than fellow Aussie and Olympic champ Sally Pearson.)

But at least for Jenneke's SI bikini shoot, the stopwatch is off.

"I looked at the pictures and I think, wow, is that really me?" Jenneke says in video.

In December, the young athlete appeared as a lonely man's fantasy object in a comedy short by The Chive. She did her well known gyrating dance in the skit, just as she did when the Internet took notice of her charms.

By the looks of her Sports Illustrated shoot, she's just getting warmed up.

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Source: http://www.huffingtonpost.com/2013/02/13/michelle-jenneke-sports-illustrated-swimsuit-modeling_n_2677696.html

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