Friday, November 13, 2009

| No 5 Cincy to use 2 QBs vs West Virginia

No.-5-Cincy-to-use-2-QBs-vs-West-Virginia CINCINNATI -Receiver Mardy Gilyard has nicknames for both of Cincinnatis quarterbacks.

Zach Collaros? Hes Joystick, a reference to the way he darts one way and then another. Tony Pike is Pistol, inspired by how fast the ball leaves his hand.

The two very different quarterbacks have gotten the same results. Theyve kept fifth-ranked Cincinnati perfect and one victory away from setting a school record for best start.

Story continues below ↓advertisement | your ad heredocument.write{DisplayDartAdandRecordAdLoad;} // if {RecordAnyLoad;});
);

West Virginia will get to see Joystick and Pistol on Friday night.

The Bearcats plan to let the sophomore Collaros make his fourth start in place of Pike, who hurt his non-throwing forearm on Oct. 15. Pike, a senior, will get into the game at some point, his first action since the injury. And the Mountaineers will be forced to deal with the Bearcats very dynamic duo.

They are really good with a large amount of playmakers on the offensive side of the ball, so its going to be really hard to contain them, West Virginia defensive lineman Chris Neild said. They have Pike coming back and their backup is just as good as him, so its going to be a tough game for us.

In different ways, Pike and Collaros have made it tough on everyone.

Pike broke his left forearm last season, got a plate inserted, and missed two games before returning and leading the Bearcats to their first Big East title. One of the highlights was his touchdown pass in overtime for a breakthrough 26-23 victory over West Virginia in Morgantown last November.

He was one of the nations leading passers when a helmet hit to the forearm damaged the plate in South Florida on Oct. 15. Collaros came to the rescue, running for a pair of touchdowns as Cincinnati pulled away to a 34-17 victory.

Hes kept the offense running at a record-setting speed.

In 3 1/2 games as the fill-in, Collaros has completed 70 of 89 passes for 1,100 yards and eight touchdowns with one interception. He also has run for 281 yards and four touchdowns. He passed for 480 yards - the second-highest total in school history - during a 47-45 win over Connecticut last week.

While Collaros excelled, Pike healed. He was able to practice with a protective brace last week, and will have a package of plays to run against West Virginia. The plan is to let him work off some of the rust from his three-week layoff, then get him ready during a bye week to start against Illinois on Nov. 27.

Physically, I think Im almost there, Pike said. The biggest thing right now is mentally. It changes a lot from when youre in practice and in the game. Well mix me in a little bit here and there. I think its a good idea not to rush in there right away. Ill be able to kind of ease back into it.

For West Virginia, theres no easing in. The Mountaineers need to hold down Cincinnatis high-scoring offense - fifth in the nation at 40 points per game - and get big days from quarterback Jarrett Brown and running back Noel Devine, both of whom got hurt during a 17-9 win over Louisville.

Devine, the Big Easts second-leading rusher, sprained an ankle and missed most of the second half. Brown missed one play with a sore foot and finished 9 of 17 for 94 yards with an interception.

His foot was a little sprained up, but I told him, Hey, buddy, I want to you be alive in the pocket, coach Bill Stewart said. I want you to have fun this week. I want you to play like its sandlot football. Just go play and have fun. He needs to pick it up. We all need to pick it up.

The game in Morgantown last year featured one of the Big Easts wildest endings. The Mountaineers scored 13 points in the last 1:11 of regulation - safety, touchdown, onside kick recovery, field goal - to send it to overtime. When Cincinnati pulled it out, the Bearcats were in line for the league title.

To be honest, I dont know if everybody thought we could win that game, said Gilyard, who leads the Big East in receiving. We knew that was a game we needed not only for ourselves, but for our program. We knew we needed to show we could compete with the big dogs in the Big East.

Theyve taken it one step further this season. A win on Friday would keep them in the conversation about national title contenders and set up a showdown at No. 8 Pittsburgh for the league title on Dec. 5.

Obviously its going to mean a lot, not just for me but the program and the guys who put in the work to see that Cincinnatis a program that can do that year-in and year-out, Pike said. To be the first team to go 10-0 would be an amazing feat and something thats going to put our program on more of a national level and keep us in contention for the big goals we have.

© 2009 The Associated Press. All rights reserved. This material may not be published, broadcast, rewritten or redistributed.

function nm_mi {
if {
window.clearTimeout;
nm_tDis = 0;

}
if {
if {
nm_aDef = new Array;
return;

} else {
window.clearTimeout;
nm_tNew = 0;
nm_nNew = 0;

}

}
var b = == *) && ;
nm_mx;
if {
var body = document.body,
dxCli,
dyCli,
dxOff,
dyOff,
sId = sU.slice;
if {
dyCli = body.clientHeight;
dxOff = body.scrollLeft;
dyOff = body.scrollTop;

} else {
dxCli = window.innerWidth - 14;
dyCli = window.innerHeight - dyNetScrFudge;
dxOff = window.pageXOffset;
dyOff = window.pageYOffset;

}
var isNBCSports=.indexOf==-1)?false:true);
var oX = new nm_xy,
xPar = oX.x,
yPar = oX.y,
dxPar = oX.dx,
dyPar = oX.dy;
dxOff -= oX.xP;
dyOff -= oX.yP;
if && || && )) {
var sas = nm_as;
if {
if != *) sas = +|Latest headlines| + sas;
sas = sas.replace;
var nmC = || == -1)) ? 1: 2;

nm_sSuf = sS;

} else {
sas = sas.replace;

}
var as = sas.split,
cs = as.length - 1,
sS,
s = new Array,
sV,
sW,
sT;
nD = nD + 1;
nm_nD = nD;

//init omniture link track values
var omni_nm_pn = Omni.NewsMenu.ProjectName;
var omni_nm_ct = ;
var omni_nm_cn = ;
var topicset=false;

s.push;
var ceCnt = 0,
CM = ,
temp;
for {
sT = as;
if == ) sT = sT.replace;
sV = sW = nm_link;
var arrowflavor = ;
var sn = ;

//get the parent omniture link track data ct value
var omni_parent_ct = o.getAttribute;
var omni_parent_cn = o.getAttribute || ; //default value statement

if == *) {
temp = sV.slice;
if
continue;
temp = nm_as.split;
if sT = temp.substr;
sV = nm_link;
sS = arrowflavor = F;
sn = sW.substring;
if == undefined || nm_as == ) arrowflavor = E;
if ceCnt = 0;
CM = F;

//Omniture news menu link track, assign first subsection flyout ct value and cn value
//ct == component type
if {
omni_nm_ct = Omni.NewsMenu.FirstFront;
omni_nm_cn = sT.substr;
//cn is subsection name, limited to first 30 characters

}

}
else if != +) //headline
{
//Omniture new menu link track, determine parent ct value and assign headline ct value and cn value
if
{
if
{
omni_nm_ct = Omni.NewsMenu.FirstHeadline;
omni_nm_cn = omni_parent_cn;

}
else if
{
omni_nm_ct = Omni.NewsMenu.ExpandHeadline;
omni_nm_cn = omni_parent_cn;

}
else if
{
omni_nm_ct = Omni.NewsMenu.SecondHeadline;
omni_nm_cn = omni_parent_cn;

}

}

sS = arrowflavor = E;
if ceCnt = 0;
CM = S;

}
sV = nm_su;
if == +) {
if
{
s.push onmouseover=nm_mi + ,null, + nD + , + gS + )> + sT + );
}
else
{
if
{
s.push;
topicset=true;
}
else
{
s.push onmouseover=nm_mi + ,null, + nD + , + gS + )> + sT + );
}
}
}
else
{
if
{
s.push + CM + gS + CE= + sId + - + + class=nmI + arrowflavor + nmLink onclick=Omni.LinkTrack.OnclickHandler;nm_mc + ) onmouseout=nm_mo onmouseover=nm_mi + ,null, + nD + , + gS + ) pn= + omni_nm_pn + ct= + omni_nm_ct + cn= + omni_nm_cn + > + sT + );
}
}

}

if
{
s.push;
}

s.push;
var oC = document.getElementById;
oC.innerHTML = s.join,
dx = oT.offsetWidth,
dy = oT.offsetHeight;
var x = xPar,
y = yPar;
if {
y += dyPar;
if x = - dx; //j-chicks

} else if != -1) {
y = y + o.offsetHeight + 6;
dx = oT.parentNode.offsetWidth;
if {
if x = xPar + o.offsetWidth - dx;
else x = - dx;

}
if x = dxOff; //end j-chicks

} else {
var dxOverlap = ? 0: 2;
x += dxPar - dxOverlap;
x += 6;
y += 1;
if y -= 1;
if {
if x = xPar + dxOverlap - dx;
else x = - dx;

}
if x = dxOff;
if {
y = - dy;
}
if y = dyOff;

}

var oD = document.getElementById;
oD.style.pixelWidth = oD.style.width = dx;
oD.style.pixelHeight = oD.style.height = dy;
oD.style.pixelLeft = oD.style.left = x;
oD.style.pixelTop = oD.style.top = y;
oD.style.zIndex = 100000000;
nm_os;
if nm_of != H) {
o.className += H;
if o.firstChild.className += H;
}
} - | No 5 Cincy to use 2 QBs vs West Virginia |

Monday, November 9, 2009

| Stars: Cosmic road signs to intelligent aliens?

Stars:-Cosmic-road-signs-to-intelligent-aliens? When scientists search the heavens for habitable worlds beyond Earth, they dont necessarily know what to look for. A new study has found that the most probable place to find intelligent life in the galaxy is around stars with roughly the mass of the sun, and surface temperatures between 5,300 and 6,000 Kelvin — in fact, stars very similar to our own sun.  

Learning that sun-like stars are good candidates for life may not sound surprising, but it isnt always what scientists have thought.

The principle of mediocrity says that, barring any evidence to the contrary, our observations should be typical among those of all intelligent observers, said researcher Daniel Whitmire, a physicist at the University of Louisiana at Lafayette. But the typical star is not like the sun —the typical star is a low mass star. We dont find ourselves around a typical star and we show the reason why in this paper. Our results confirm the principle of mediocrity as applied to the sun.

Sun-like stars are actually a minority in the galaxy — 93 percent of stars in the Milky Way are less massive, less luminous and cooler than the sun. Though the typical star in the galaxy weighs between one-tenth and half the mass of the sun, life is more likely to be found around the more unusual variety of stars like our own, the researchers found.

To make their calculation, Whitmire and colleague John Matese combined models of how planets form with data on the distribution of stars in the galaxy as a function of mass. The planet models show when worlds are most likely to form in the habitable zone — a Goldilocks region around a star in which a planet would be just right for life - not too close that its surface would be boiling, and not too far that it would be frigid either. Planets in the habitable zone are the best candidates for having liquid water, which is thought to be a prerequisite of life.

In general, the planet-formation theories predict that more massive stars are the most likely to have planets in the habitable zone. So the larger a parent star is, the more likely its planets will have environments conducive to life.

But this advantage of larger stars is counteracted by the fact that more massive stars are less abundant — there are fewer big stars out there. In addition, the more massive a star is, the shorter its lifetime. That makes it hard to find very massive stars that have lived long enough for complex life to develop.

The researchers weighed these factors against each other to calculate the distribution of stars most likely to host thinking, living creatures. Its a tradeoff between the numbers of stars out there and the probability of habitable planet formation increasing with mass. Whitmire said. We show its no accident we find ourselves around a star like the sun. The distinction between habitable planets and planets harboring intelligent life is based on the fact that intelligent life requires stars with lifetimes greater than the time required for intelligence to evolve. For example, in the case of this solar system, we could not find ourselves around a star with a lifetime less than 4.5 billion years.

Indeed, sun-like stars seem to have the right balance: They are of high enough mass that they are more likely to host habitable planets, but they are of low enough mass that they live long enough for intelligent life to develop, and are not extremely scarce. Whitmire estimates that 10 percent of the Milky Ways stars might fall into the category theyve outlined. This would still leave over 10 billion candidate stars in the Milky Way alone.

The results mitigate the most commonly used argument that intelligent life must be extremely rare, Whitmire said. This idea, based on the anthropic principle, was outlined by astrophysicist Brandon Carter. There is an approximate coincidence between the time it took intelligence to evolve on Earth and the lifetime of the sun. Assuming these two timescales are independent, this coincidence makes sense if intelligent life is extremely improbable, Carter argued. In most cases, he claimed, the time it takes for intelligent life to emerge is much longer than the portion of a stars existence that is conducive to such life.

In the paper we explain one number in the coincidence — why the lifetime of the sun is what it is, Whitmire said. The additional assumption necessary to counter the Carter argument is that intelligent life requires at least a few billion years to evolve, as expected if we are typical.

The study is detailed in the September 2009 issue of the Astrobiology Journal.

© 2009 Space.com. All rights reserved. More from Space.com.var url=location.href;var i=url.indexOf + 1;if{i=url.indexOf + 1;}if{i=url.indexOf;}if{url = url.substring;document.write;if{window.print;}}
MSN Privacy .
Legal © 2009 MSNBC.com - | Stars: Cosmic road signs to intelligent aliens? |