American men’s tennis is at a nadir. No Grand Slam singles champion in 11 years. No Grand Slam singles semifinalist in over five years. The U.S. Open unfolding now in New York is the 12th straight Grand Slam without an American man in the quarterfinals, and the seventh of the last eight with none in the fourth round.1The only active American man to even reach a major semifinal is Robby Ginepri, who is 31 and ranked 204th in the world.American women’s tennis is led by the No. 1 player in the world, Serena Williams, who has won 17 Grand Slam titles and remains the favorite to win the U.S. Open for the third year in a row.I wondered, though: Are the American women a stronger force in world tennis than the American men are? Beyond Serena and Venus Williams — who are 32 and 34 years old, respectively — are the women any deeper and stronger than the men?To check, I downloaded the latest singles rankings from both the men’s ATP World Tour and the women’s WTA tour — every player in the world who has a professional ranking point, even just one.As of Aug. 25, the start of the U.S. Open, there are 2,232 ranked men and 1,323 ranked women. About one in 12 of the ranked women are from the U.S., more than from any other nation (Russia trails narrowly). U.S. men make up one in 16 of all ranked professional players, tied with France for most in the world.Counting ranked players is a pretty rough gauge of national tennis strength. A player outside the Top 500 will appear in few tour events, let alone Grand Slams. Getting a ranking can be a product of opportunity as much as merit. An American player who’s just as good as, say, an Algerian player lives much closer to events where he can earn points, and therefore doesn’t have to spend as much to play.So I went beyond merely counting ranked players and added up the ranking points for each nation. This is a decent proxy for how much money players have earned in the sport, because ranking points generally scale with earnings. The bigger the tournament, the more points and dollars are available; and the further a player advances, the bigger a piece of the pie she earns. By this math, Serena Williams’s 2,000 points for winning the U.S Open last year — which still counts in the latest 52-week ranking — is worth slightly more than No. 24 Sloane Stephens’s cumulative tennis accomplishments in the last year. And Serena’s annual achievements are worth about five Sloanes in national tennis strength.That feels about right. Having lots of Top 100 players is nice in the first couple of days of a Grand Slam tournament. Having one player who can consistently reach the last couple of days of a Grand Slam is much nicer.Here, the U.S. women dominate their peers, and their male counterparts. They hog 12 percent of the world’s female tennis talent — half again as much as runner-up Russia. The U.S. men have just 5 percent of global male talent. The U.S. trails four European nations — Spain, France, Serbia and Switzerland — that combined have less than one-half the population of the U.S.Just five years ago, American men and women were much closer in their global tennis standing. American men held 8 percent of tennis ranking points, compared to 10 percent for women. The women have rebounded slightly while the men have lost ground.American men’s tennis boosters can point to a few reasonable explanations. First, the men’s long-term slump is less precipitous than the women’s. I checked by downloading pre-U.S. Open rankings data from the ATP and WTA websites for prior years, with major help from my colleague, Paul Schreiber. At this stage of the season in 1999 — the first year for which WTA ranking data is available on the WTA website — American women commanded 21 percent of global tennis power. American men held 11 percent. The men have narrowed the gender gap even as they have fallen further behind the rest of the world.2Any comparison can look different depending on which dates we choose to start and end with. The U.S. men’s slow decline over the last 15 years followed a crash, from 26 percent heading into the 1990 U.S. Open and 18 percent in 1994.Globalization also has brought more competition to the men’s game. Over the last few decades, the sport’s footprint has expanded further beyond the traditional bases in the four Grand Slam-hosting nations (the U.S., U.K., France and Australia). This is particularly so in the men’s game. That’s partly because of unequal opportunities; many countries still haven’t given girls the same chance to play sports as boys, or have done so only recently. Economic incentives have also favored the men: The Grand Slams equalized pay only seven years ago, and many other tournaments still pay men more than women. There also are more men’s professional events, which helps explain why there are more ranked male players than female players.The result is that 104 countries have ranked men, compared to just 79 countries with ranked women. That represents an increase of 14 countries from this time in 1999 for the men, but a rise of just four countries for the women.American women also are competing with fewer talent bases around the world. Russia is the only other country with at least 5 percent of the world’s ranked women. Three other countries besides the U.S. have a share that big of all ranked men.Another way to understand the men’s relative struggles is that the Williams sisters might be outliers who skew the whole comparison. Their story often has been described as one of the most remarkable in sports history, and rightly so. Their parents, Richard Williams and Oracene Price, trained them at a very young age with the goal of making each the No. 1 player in the world. Their daughters each achieved that audacious goal, and did so outside the well funded national centers. They have remained so good, past the age that most other women’s greats retired, that they account today for more than one-third of all U.S. women’s ranking points.What if the Williams family had never picked up tennis rackets? Then U.S. women would account for less than 8 percent of global talent today, much closer to their male counterparts.3Comparable earlier figures are 5 percent before the 2009 U.S. Open, 13 percent in 2004 and 17 percent in 1999. American women other than the Williams sisters have rebounded slightly after a steep decline. That group includes a number of young players who could one day enter the Top 10 but so far have performed inconsistently, including Stephens, Christina McHale and Madison Keys. None of them — nor the other three American women who rank behind the two Williams sisters but inside the Top 50 — reached the third round of the U.S. Open.4Remove John Isner and Donald Young, the top two American men, from the sport and the U.S. men’s share of global pro tennis power drops just one percentage point, to 4 percent.Here’s an even more outrageous hypothetical: What if Richard and Oracene had trained two young sons instead of daughters, and Jupiter and Steve had the same success that Venus and Serena have had? American men would hog a greater portion of global tennis talent than American women would today.While that scenario is farfetched, it is rooted in the reality of a sport usually dominated by just a few superstars. Even when American tennis was much deeper than it is today, one or two singular talents carried most of the load for winning big tournaments and contending for No. 1. Jimmy Connors and John McEnroe gave way to Pete Sampras, Jim Courier and Andre Agassi. Those men won 41 of American men’s 46 Grand Slams in the last 42 years. Maybe it’s just a fluke that another player with that kind of talent hasn’t come around since Sampras and Agassi retired — or hasn’t played tennis.As it happens, Richard Williams, who is 72, has a two-year-old son. But if Richard has his way, Dylan won’t help pick up the mantle for the American men. “He’ll never be a billionaire in tennis,” Richard Williams said earlier this year. He wants his son to buy a gold mine.
WILMINGTON, MA — Below is a message from Book Stew host Eileen MacDougall:Hello, Book Stew viewers! It’s such a pleasure to host my first children’s book illustrator and author, Ioana Hobai.A native of Romania, Ioana grew up drawing and doodling in repressive Budapest. After coming to the US, she worked as an architect before returning to her first love, art and illustration. Ioana’s new book, “Lena’s Slippers,” is based on an incident in her own life. She’s a dream guest and I hope you’ll enjoy this episode!Watch the episode, courtesy of Wilmington Community Television, below:—Video Playerhttps://wilmington.vod.castus.tv/vod/dl.php/8/c/8/2/6/5/8c8265f4-b94f-4fc5-a21a-49ee5e3317271564418333.122+69201032.166@castus4-wilmington+15645990431564597150038576.vod.1080p.Book%20Stew.mp4Media error: Format(s) not supported or source(s) not foundmejs.download-file: https://wilmington.vod.castus.tv/vod/dl.php/8/c/8/2/6/5/8c8265f4-b94f-4fc5-a21a-49ee5e3317271564418333.122+69201032.166@castus4-wilmington+15645990431564597150038576.vod.1080p.Book%20Stew.mp4?_=100:0000:0000:00Use Up/Down Arrow keys to increase or decrease volume.— Like Wilmington Apple on Facebook. Follow Wilmington Apple on Twitter. Follow Wilmington Apple on Instagram. Subscribe to Wilmington Apple’s daily email newsletter HERE. Got a comment, question, photo, press release, or news tip? Email email@example.com.Share this:TwitterFacebookLike this:Like Loading… RelatedNEW STEW: Meet Author Ben Berkley On September’s Book StewIn “Videos”NEW STEW: Meet Author Renee Simms On June’s Book StewIn “Community”NEW STEW: Meet Author Marcia Butler On May’s Book StewIn “Videos”
© 2016 Phys.org Citation: Two super-Earth-sized planets discovered orbiting a nearby star (2016, July 20) retrieved 18 August 2019 from https://phys.org/news/2016-07-super-earth-sized-planets-orbiting-nearby-star.html (Phys.org)—NASA’s Kepler spacecraft continues its fruitful exoplanet hunt with the newest discovery of two super-Earth-sized alien worlds. The newly detected planets are orbiting a nearby sun-sized star known as HD 3167, located some 150 light years away. The results are presented in a paper published July 18 on the arXiv pre-print server. Explore further K2 light curve of HD 3167. Top: the full K2 light curve. Both the numerous, shallow transits of HD 3167 b and three deeper transits of HD 3167 c are evident in the light curve by eye. Bottom left: K2 light curve (grey dots) phase folded on the transits of HD 3167 b, and best-fit transit model (thick purple line). Bottom right: K2 light curve (grey dots) phase folded on the transits of HD 3167 c, and best-fit transit model (thick purple line). Credit: Vanderburg et al., 2016. This document is subject to copyright. Apart from any fair dealing for the purpose of private study or research, no part may be reproduced without the written permission. The content is provided for information purposes only. New system discovered with five planets More information: Two Small Planets Transiting HD 3167, arXiv:1607.05248 [astro-ph.EP] arxiv.org/abs/1607.05248AbstractWe report the discovery of two super-Earth-sized planets transiting the bright (V = 8.94, K = 7.07) nearby late G-dwarf HD 3167, using data collected by the K2 mission. The inner planet, HD 3167 b, has a radius of 1.6 R_e and an ultra-short orbital period of only 0.96 days. The outer planet, HD 3167 c, has a radius of 2.9 R_e and orbits its host star every 29.85 days. At a distance of just 45.8 +/- 2.2 pc, HD 3167 is one of the closest and brightest stars hosting multiple transiting planets, making HD 3167 b and c well suited for follow-up observations. The star is chromospherically inactive and slowly rotating, ideal for radial velocity observations to measure the planets’ masses. The outer planet is large enough that it likely has a thick gaseous envelope which could be studied via transmission spectroscopy. Planets transiting bright, nearby stars like HD 3167 are valuable objects to study leading up to the launch of the James Webb Space Telescope. Although Kepler has lost two of its four reaction wheels and therefore cannot be precisely pointed toward stars, it is still capable of detecting new exoworlds. The spacecraft is now in its extended mission, known as K2, during which it has already found over 100 new planets. The HD 3167 system is just the latest addition to the vast collection of extrasolar worlds detected by K2.HD 3167 was observed by Kepler between January 3 and March 23, 2016 during Campaign 8 of its K2 mission. This observation campaign allowed a team of astronomers, led by Andrew Vanderburg of the Harvard–Smithsonian Center for Astrophysics (CfA), to detect two transit signals that could be planets circling around this nearby star.”We identified two planet candidates transiting HD 3167 after processing pixel-level data to produce a light curve, removing systematic effects due to Kepler’s unstable pointing, and searching for planets using a Box Least Squares periodogram search,” the researchers wrote in the paper.To confirm the planetary status of these candidates, the team conducted follow-up observations employing the Tillinghast Reflector Echelle Spectrograph (TRES) on the 1.5 m telescope at the Fred L. Whipple Observatory on Mt. Hopkins, Arizona and the Robo-AO adaptive optics system installed at the 2.1 m telescope at the Kitt Peak National Observatory, also in Arizona. They also used statistical techniques to validate the planetary nature of the transiting signals.The confirmed exoplanets received designation HD 3167 b and HD 3167 c. With a radius of about 1.6 Earth radii, HD 3167 b is the inner planet, orbiting the host star in just slightly less than one day. The outer planet is nearly three times bigger in size than Earth and has an orbital period of approximately 30 days.HD 3167 could be an excellent target for further follow-up observations as it is one of the closest and brightest stars hosting multiple transiting planets. The scientists noted that this system is highly suitable for precise radial velocity observations to measure the planets’ masses.”If HD 3167 b is rocky with a mass of about four Earth masses, it should induce radial velocity variations with a semiamplitude of about 3 ms−1. Depending on its composition, HD 3167 c could induce radial velocity variations with a semiamplitude of anywhere between 1 ms−1 and 3 ms−1. These signals should be readily detectable with modern spectrographs,” the paper reads.The team also emphasized that the outer planet is one of the best currently known small planets for atmospheric characterization with transit transmission spectroscopy. However, they also noted that the short period of HD 3167 b makes it likely that spectroscopic observations of HD 3167 c’s atmosphere might overlap with a transit of the inner planet.”This could be an efficient way to rule out a hydrogen-dominated atmosphere for HD 3167 b. Observers should be cautious, however, to ensure that a transit of HD 3167 b not interfere with out-of-transit observations necessary for calibration,” the researchers concluded.
The Shiromani Akali Dal on Tuesday said it will contest from four seats in the February 7 Delhi assembly polls, a day after its ally, the BJP, released its list of 62 candidates.“The Shiromani Akali Dal will fight from four seats in Delhi as per the formula of our alliance with the BJP,” Akali Dal Delhi unit president Manjeet Singh GK said.Manjinder Singh Sirsa will be contesting from Rajouri Garden, Harmeet Singh Kalka from Kalkaji and Jitender Singh Shunty from Shahdara. The party left out Shyam Sharma from the Hari Nagar seat and instead chose Avtar Singh Hit. All the three candidates – Sirsa, Kalka and Shunty – had fought the 2013 polls from the same constituencies and won. Sharma, however, had lost from Hari Nagar. Of the four candidates, Sirsa will contest on the Akali Dal’s weighing scale symbol, while the other three candidates will fight on the BJP symbol.