NEW YORK (AP) ? Dule Hill will be tapping into his dancing roots when he joins Broadway's "After Midnight," a musical celebrating Duke Ellington's years at the famous Cotton Club nightclub in Harlem.
Producers said Wednesday the actor and trained tap dancer best known for starring in USA's hit detective series "Psych," will play the host of the show, presenting the sound and glamor of the Harlem Renaissance.
Performances start Oct. 18 at the Brooks Atkinson Theatre, with an official opening night set for Nov. 3.
Hill was last on Broadway as Spoon, a lawyer-turned-budding novelist, in Lydia R. Diamond's thoughtful family drama "Stick Fly" in 2011. Hill joins the already announced Grammy Award- and "American Idol" winner Fantasia Barrino in the lively show that will feature 17 musicians and 25 vocalists and dancers.
Emmy Award-nominated for his work as Charlie Young on "The West Wing," Hill first came to prominence as The Kid opposite Savion Glover and Jeffrey Wright in "Bring in 'Da Noise, Bring in 'Da Funk." Born and raised in New Jersey, Hill began attending dance school when he was 3 and received his first break years later as the understudy to Glover in "The Tap Dance Kid" on Broadway.
Directed and choreographed by Warren Carlyle with musical direction by Wynton Marsalis, the show appeared off-Broadway last year at New York City Center under the name "Cotton Club Parade." Songs include "Stormy Weather," ''I Can't Give You Anything But Love" and "I've Got the World on a String."
Hill may get a work-out in the show, which off-Broadway had no fewer than 24 numbers with dancing that included the Savoy swing and the Charleston. Veteran singer and dancer Brandon Victor Dixon played the role at New York City Center.
Legendary performers such as the Nicholas Brothers, Bessie Smith, Ethel Waters and a teenage Lena Horne all performed at the Cotton Club in the 1920s. The music and dancing will be augmented by Langston Hughes poetry.
___
Online: http://www.aftermidnightbroadway.com
___
Mark Kennedy can be reached at http://twitter.com/KennedyTwits
3 planets in habitable zone of nearby starPublic release date: 25-Jun-2013 [ | E-mail | Share ]
Contact: Richard Hook rhook@eso.org 49-893-200-6655 ESO
Gliese 667C reexamined
Gliese 667C is a very well-studied star. Just over one third of the mass of the Sun, it is part of a triple star system known as Gliese 667 (also referred to as GJ 667), 22 light-years away in the constellation of Scorpius (The Scorpion). This is quite close to us within the Sun's neighbourhood and much closer than the star systems investigated using telescopes such as the planet-hunting Kepler space telescope.
Previous studies of Gliese 667C had found that the star hosts three planets (eso0939 - http://www.eso.org/public/news/eso0939/, eso1214 - http://www.eso.org/public/news/eso1214/) with one of them in the habitable zone. Now, a team of astronomers led by Guillem Anglada-Escud of the University of Gttingen, Germany and Mikko Tuomi of the University of Hertfordshire, UK, has reexamined the system. They have added new HARPS observations, along with data from ESO's Very Large Telescope, the W.M. Keck Observatory and the Magellan Telescopes, to the already existing picture [1]. The team has found evidence for up to seven planets around the star [2].
These planets orbit the third fainter star of a triple star system. Viewed from one of these newly found planets the two other suns would look like a pair of very bright stars visible in the daytime and at night they would provide as much illumination as the full Moon. The new planets completely fill up the habitable zone of Gliese 667C, as there are no more stable orbits in which a planet could exist at the right distance to it.
"We knew that the star had three planets from previous studies, so we wanted to see whether there were any more," says Tuomi. "By adding some new observations and revisiting existing data we were able to confirm these three and confidently reveal several more. Finding three low-mass planets in the star's habitable zone is very exciting!"
Three of these planets are confirmed to be super-Earths planets more massive than Earth, but less massive than planets like Uranus or Neptune that are within their star's habitable zone, a thin shell around a star in which water may be present in liquid form if conditions are right. This is the first time that three such planets have been spotted orbiting in this zone in the same system [3].
"The number of potentially habitable planets in our galaxy is much greater if we can expect to find several of them around each low-mass star instead of looking at ten stars to look for a single potentially habitable planet, we now know we can look at just one star and find several of them," adds co-author Rory Barnes (University of Washington, USA).
Compact systems around Sun-like stars have been found to be abundant in the Milky Way. Around such stars, planets orbiting close to the parent star are very hot and are unlikely to be habitable. But this is not true for cooler and dimmer stars such as Gliese 667C. In this case the habitable zone lies entirely within an orbit the size of Mercury's, much closer in than for our Sun. The Gliese 667C system is the first example of a system where such a low-mass star is seen to host several potentially rocky planets in the habitable zone.
The ESO scientist responsible for HARPS, Gaspare Lo Curto, remarks: "This exciting result was largely made possible by the power of HARPS and its associated software and it also underlines the value of the ESO archive. It is very good to also see several independent research groups exploiting this unique instrument and achieving the ultimate precision."
And Anglada-Escud concludes: "These new results highlight how valuable it can be to re-analyse data in this way and combine results from different teams on different telescopes."
###
Notes
[1] The team used data from the UVES spectrograph on ESO's Very Large Telescope in Chile (to determine the properties of the star accurately), the Carnegie Planet Finder Spectrograph (PFS) at the 6.5-metre Magellan II Telescope at the Las Campanas Observatory in Chile, the HIRES spectrograph mounted on the Keck 10-metre telescope on Mauna Kea, Hawaii as well as extensive previous data from HARPS (the High Accuracy Radial velocity Planet Searcher) at ESO's 3.6-metre telescope in Chile (gathered through the M dwarf programme led by X. Bonfils and M. Mayor 2003-2010 described here: http://www.eso.org/public/archives/releases/sciencepapers/eso1214/eso1214b.pdf).
[2] The team looked at radial velocity data of Gliese 667C, a method often used to hunt for exoplanets. They performed a robust Bayesian statistical analysis to spot the signals of the planets. The first five signals are very confident, while the sixth is tentative, and seventh more tentative still. This system consists of three habitable-zone super-Earths, two hot planets further in, and two cooler planets further out. The planets in the habitable zone and those closer to the star are expected to always have the same side facing the star, so that their day and year will be the same lengths, with one side in perpetual sunshine and the other always night.
[3] In the Solar System Venus orbits close to the inner edge of the habitable zone and Mars close to the outer edge. The precise extent of the habitable zone depends on many factors.
More information
This research was presented in a paper entitled "A dynamically-packed planetary system around GJ 667C with three super-Earths in its habitable zone", to appear in the journal Astronomy & Astrophysics.
The team is composed of G. Anglada-Escud (University of Gttingen, Germany), M. Tuomi (University of Hertfordshire, UK), E. Gerlach (Technical University of Dresden, Germany), R. Barnes (University of Washington, USA), R. Heller (Leibniz Institute for Astrophysics, Potsdam, Germany), J. S. Jenkins (Universidad de Chile, Chile), S. Wende (University of Gttingen, Germany), S. S. Vogt (University of California, Santa Cruz, USA), R. P. Butler (Carnegie Institution of Washington, USA), A. Reiners (University of Gttingen, Germany), and H. R. A. Jones (University of Hertfordshire, UK).
ESO is the foremost intergovernmental astronomy organisation in Europe and the world's most productive ground-based astronomical observatory by far. It is supported by 15 countries: Austria, Belgium, Brazil, the Czech Republic, Denmark, France, Finland, Germany, Italy, the Netherlands, Portugal, Spain, Sweden, Switzerland and the United Kingdom. ESO carries out an ambitious programme focused on the design, construction and operation of powerful ground-based observing facilities enabling astronomers to make important scientific discoveries. ESO also plays a leading role in promoting and organising cooperation in astronomical research. ESO operates three unique world-class observing sites in Chile: La Silla, Paranal and Chajnantor. At Paranal, ESO operates the Very Large Telescope, the world's most advanced visible-light astronomical observatory and two survey telescopes. VISTA works in the infrared and is the world's largest survey telescope and the VLT Survey Telescope is the largest telescope designed to exclusively survey the skies in visible light. ESO is the European partner of a revolutionary astronomical telescope ALMA, the largest astronomical project in existence. ESO is currently planning the 39-metre European Extremely Large optical/near-infrared Telescope, the E-ELT, which will become "the world's biggest eye on the sky".
###
Links
Research paper- http://www.eso.org/public/archives/releases/sciencepapers/eso1328/eso1328a.pdf
Description of HARPS - http://www.eso.org/sci/facilities/lasilla/instruments/harps.html
Photos of the La Silla Observatory - http://www.eso.org/public/images/archive/category/lasilla/
eso1214 - http://www.eso.org/public/news/eso1214/ -- press release describing earlier observations of Gliese 667C by the HARPS team
eso0939 - http://www.eso.org/public/news/eso0939/ -- press release describing original observations of this star using HARPS
Las Campanas -- Magellan telescopes - http://www.lco.cl/telescopes-information/magellan
Contacts
Guillem Anglada-Escud
Institut fur Astrophysik, University of Gttingen
Gttingen, Germany
Tel: +49 0551 39 9988
Email: guillem.anglada@gmail.com
Mikko Tuomi
Center for Astrophysics Reseach, Hertfordshire University
Hatfield, UK
Tel: +44 01707 284095
Email: miptuom@utu.fi
Rory Barnes
Department of Astronomy, University of Washington
Seattle, USA
Tel: +1 206 543 8979
Email: rory@astro.washington.edu
Richard Hook
ESO education and Public Outreach Department
Garching bei Mnchen, Germany
Tel: +49 89 3200 6655
Cell: +49 151 1537 3591
Email: rhook@eso.org
[ | E-mail | 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.
3 planets in habitable zone of nearby starPublic release date: 25-Jun-2013 [ | E-mail | Share ]
Contact: Richard Hook rhook@eso.org 49-893-200-6655 ESO
Gliese 667C reexamined
Gliese 667C is a very well-studied star. Just over one third of the mass of the Sun, it is part of a triple star system known as Gliese 667 (also referred to as GJ 667), 22 light-years away in the constellation of Scorpius (The Scorpion). This is quite close to us within the Sun's neighbourhood and much closer than the star systems investigated using telescopes such as the planet-hunting Kepler space telescope.
Previous studies of Gliese 667C had found that the star hosts three planets (eso0939 - http://www.eso.org/public/news/eso0939/, eso1214 - http://www.eso.org/public/news/eso1214/) with one of them in the habitable zone. Now, a team of astronomers led by Guillem Anglada-Escud of the University of Gttingen, Germany and Mikko Tuomi of the University of Hertfordshire, UK, has reexamined the system. They have added new HARPS observations, along with data from ESO's Very Large Telescope, the W.M. Keck Observatory and the Magellan Telescopes, to the already existing picture [1]. The team has found evidence for up to seven planets around the star [2].
These planets orbit the third fainter star of a triple star system. Viewed from one of these newly found planets the two other suns would look like a pair of very bright stars visible in the daytime and at night they would provide as much illumination as the full Moon. The new planets completely fill up the habitable zone of Gliese 667C, as there are no more stable orbits in which a planet could exist at the right distance to it.
"We knew that the star had three planets from previous studies, so we wanted to see whether there were any more," says Tuomi. "By adding some new observations and revisiting existing data we were able to confirm these three and confidently reveal several more. Finding three low-mass planets in the star's habitable zone is very exciting!"
Three of these planets are confirmed to be super-Earths planets more massive than Earth, but less massive than planets like Uranus or Neptune that are within their star's habitable zone, a thin shell around a star in which water may be present in liquid form if conditions are right. This is the first time that three such planets have been spotted orbiting in this zone in the same system [3].
"The number of potentially habitable planets in our galaxy is much greater if we can expect to find several of them around each low-mass star instead of looking at ten stars to look for a single potentially habitable planet, we now know we can look at just one star and find several of them," adds co-author Rory Barnes (University of Washington, USA).
Compact systems around Sun-like stars have been found to be abundant in the Milky Way. Around such stars, planets orbiting close to the parent star are very hot and are unlikely to be habitable. But this is not true for cooler and dimmer stars such as Gliese 667C. In this case the habitable zone lies entirely within an orbit the size of Mercury's, much closer in than for our Sun. The Gliese 667C system is the first example of a system where such a low-mass star is seen to host several potentially rocky planets in the habitable zone.
The ESO scientist responsible for HARPS, Gaspare Lo Curto, remarks: "This exciting result was largely made possible by the power of HARPS and its associated software and it also underlines the value of the ESO archive. It is very good to also see several independent research groups exploiting this unique instrument and achieving the ultimate precision."
And Anglada-Escud concludes: "These new results highlight how valuable it can be to re-analyse data in this way and combine results from different teams on different telescopes."
###
Notes
[1] The team used data from the UVES spectrograph on ESO's Very Large Telescope in Chile (to determine the properties of the star accurately), the Carnegie Planet Finder Spectrograph (PFS) at the 6.5-metre Magellan II Telescope at the Las Campanas Observatory in Chile, the HIRES spectrograph mounted on the Keck 10-metre telescope on Mauna Kea, Hawaii as well as extensive previous data from HARPS (the High Accuracy Radial velocity Planet Searcher) at ESO's 3.6-metre telescope in Chile (gathered through the M dwarf programme led by X. Bonfils and M. Mayor 2003-2010 described here: http://www.eso.org/public/archives/releases/sciencepapers/eso1214/eso1214b.pdf).
[2] The team looked at radial velocity data of Gliese 667C, a method often used to hunt for exoplanets. They performed a robust Bayesian statistical analysis to spot the signals of the planets. The first five signals are very confident, while the sixth is tentative, and seventh more tentative still. This system consists of three habitable-zone super-Earths, two hot planets further in, and two cooler planets further out. The planets in the habitable zone and those closer to the star are expected to always have the same side facing the star, so that their day and year will be the same lengths, with one side in perpetual sunshine and the other always night.
[3] In the Solar System Venus orbits close to the inner edge of the habitable zone and Mars close to the outer edge. The precise extent of the habitable zone depends on many factors.
More information
This research was presented in a paper entitled "A dynamically-packed planetary system around GJ 667C with three super-Earths in its habitable zone", to appear in the journal Astronomy & Astrophysics.
The team is composed of G. Anglada-Escud (University of Gttingen, Germany), M. Tuomi (University of Hertfordshire, UK), E. Gerlach (Technical University of Dresden, Germany), R. Barnes (University of Washington, USA), R. Heller (Leibniz Institute for Astrophysics, Potsdam, Germany), J. S. Jenkins (Universidad de Chile, Chile), S. Wende (University of Gttingen, Germany), S. S. Vogt (University of California, Santa Cruz, USA), R. P. Butler (Carnegie Institution of Washington, USA), A. Reiners (University of Gttingen, Germany), and H. R. A. Jones (University of Hertfordshire, UK).
ESO is the foremost intergovernmental astronomy organisation in Europe and the world's most productive ground-based astronomical observatory by far. It is supported by 15 countries: Austria, Belgium, Brazil, the Czech Republic, Denmark, France, Finland, Germany, Italy, the Netherlands, Portugal, Spain, Sweden, Switzerland and the United Kingdom. ESO carries out an ambitious programme focused on the design, construction and operation of powerful ground-based observing facilities enabling astronomers to make important scientific discoveries. ESO also plays a leading role in promoting and organising cooperation in astronomical research. ESO operates three unique world-class observing sites in Chile: La Silla, Paranal and Chajnantor. At Paranal, ESO operates the Very Large Telescope, the world's most advanced visible-light astronomical observatory and two survey telescopes. VISTA works in the infrared and is the world's largest survey telescope and the VLT Survey Telescope is the largest telescope designed to exclusively survey the skies in visible light. ESO is the European partner of a revolutionary astronomical telescope ALMA, the largest astronomical project in existence. ESO is currently planning the 39-metre European Extremely Large optical/near-infrared Telescope, the E-ELT, which will become "the world's biggest eye on the sky".
###
Links
Research paper- http://www.eso.org/public/archives/releases/sciencepapers/eso1328/eso1328a.pdf
Description of HARPS - http://www.eso.org/sci/facilities/lasilla/instruments/harps.html
Photos of the La Silla Observatory - http://www.eso.org/public/images/archive/category/lasilla/
eso1214 - http://www.eso.org/public/news/eso1214/ -- press release describing earlier observations of Gliese 667C by the HARPS team
eso0939 - http://www.eso.org/public/news/eso0939/ -- press release describing original observations of this star using HARPS
Las Campanas -- Magellan telescopes - http://www.lco.cl/telescopes-information/magellan
Contacts
Guillem Anglada-Escud
Institut fur Astrophysik, University of Gttingen
Gttingen, Germany
Tel: +49 0551 39 9988
Email: guillem.anglada@gmail.com
Mikko Tuomi
Center for Astrophysics Reseach, Hertfordshire University
Hatfield, UK
Tel: +44 01707 284095
Email: miptuom@utu.fi
Rory Barnes
Department of Astronomy, University of Washington
Seattle, USA
Tel: +1 206 543 8979
Email: rory@astro.washington.edu
Richard Hook
ESO education and Public Outreach Department
Garching bei Mnchen, Germany
Tel: +49 89 3200 6655
Cell: +49 151 1537 3591
Email: rhook@eso.org
[ | E-mail | 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.
JOHANNESBURG (AP) ? Nelson Mandela's health has deteriorated and he is now in critical condition, the South African government said Sunday.
The office of President Jacob Zuma said in a statement that he had visited the 94-year-old anti-apartheid leader at a hospital Sunday evening and was informed by the medical team that Mandela's condition had become critical in the past 24 hours.
"The doctors are doing everything possible to get his condition to improve and are ensuring that Madiba is well-looked after and is comfortable. He is in good hands," Zuma said in the statement, using Mandela's clan name.
Zuma also met Graca Machel, Mandela's wife, at the hospital in Pretoria and discussed the former leader's condition, according to the statement. Zuma was accompanied on the visit by Cyril Ramaphosa, the deputy president of the country's ruling party, the African National Congress.
Mandela, who became South Africa's first black president after the end of apartheid in 1994, was hospitalized on June 8 for what the government said was a recurring lung infection.
In the statement, Zuma also discussed the government's acknowledgement a day earlier that an ambulance carrying Mandela to the hospital two weeks ago had engine trouble, requiring the former president to be transferred to another ambulance for his journey to the hospital.
"There were seven doctors in the convoy who were in full control of the situation throughout the period. He had expert medical care," Zuma said. "The fully equipped military ICU ambulance had a full complement of specialist medical staff including intensive care specialists and ICU nurses. The doctors also dismissed the media reports that Madiba suffered cardiac arrest. There is no truth at all in that report."
Zuma appealed to South Africans and the rest of the world to pray for Mandela, his family and the medical team that is attending to him.
On April 29, state television broadcast footage of a visit by Zuma and other leaders of the African National Congress to Mandela's home. Zuma said at the time that Mandela was in good shape, but the footage ? the first public images of Mandela in nearly a year ? showed him silent and unresponsive, even when Zuma tried to hold his hand.
Mandela was jailed for 27 years under white racist rule and was released in 1990. He then played a leading role in steering the divided country from the apartheid era to democracy, becoming South Africa's first black president in all-race elections in 1994.
As a result of his sacrifice and peacemaking efforts, he is seen by many around the world as a symbol of reconciliation.
LOS ANGELES (TheWrap.com) - Gary David Goldberg, creator of the 1980s NBC sitcom "Family Ties," died Sunday following a battle with brain cancer, according to media reports. He was 68.
Born in Brooklyn, Goldberg began writing his career as a writer working for "The Bob Newhart Show," moving on to "The Tony Randall Show" and "Lou Grant," serving as writer and producer on both series.
After founding his own production company Ubu Productions (named after his dog, and featuring the line "Sit, Ubu, sit" in the closing credits for its shows; see video below), Goldberg created "Family Ties," which propelled Michael J. Fox into stardom as Alex P. Keaton, the Reagan Era, conservative son of liberal parents. The series ran for seven seasons.
Goldberg would later go on to work with Fox on the sitcom "Spin City," which Goldberg co-created with Bill Lawrence.
"Everyone has a mentor (or two hopefully) that touches his/her life," Lawrence tweeted Sunday night. "Gary Goldberg passed away today. Wish I had thanked him more."
The website for Ubu Productions and Goldberg's website have not yet made mention of his death. Goldberg's agent and a representative for the publisher of his autobiography, "Sit, Ubu, Sit: How I Went from Brooklyn to Hollywood with the Same Woman, the Same Dog, and a Lot Less Hair," have not yet responded to TheWrap's request for comment.
In addition to his television work, Goldberg worked on films such as "Must Love Dogs" and "Bye Bye Love."
Cooking is more than just following a recipe. The key is to know the right ways to prep, to use your ingredients, to clean up and how to prevent things from going wrong. Click through to check out some of our best cooking tips, and share your own in the comments!
Katie is a freelance writer focused on pets, food and women?s issues. A Chicago native and longtime resident of the Pacific Northwest, Katie now lives in Oakland, California.
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If you weren't able to scrounge up enough coin to snap up the lastfew Apple I computers to be auctioned off, another chance to score one -- and empty your bank account -- is headed your way. Starting today, Christie's will be auctioning a functional Apple I until July 9, with a starting bid of $300,000. If last month's record-breaking $671,400 sale of a similar rig is anything to go by, this machine may rake in more than its estimated $500,000 value. The owner of the Apple I, who picked it up over three decades ago in a swap, modified it with a keyboard, monitor and a tape deck for storage - in other words, just the motherboard is original. Those more interested in window shopping can ogle the classic hardware at Mountain View's Computer History Museum beginning tomorrow.
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Public release date: 25-Jun-2013
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