Документ взят из кэша поисковой машины. Адрес оригинального документа : http://www.aaa.org/EyepieceFiles/aaa/2009_05_May_Eyepiece.pdf Дата изменения: Sun Feb 22 20:31:05 2015 Дата индексирования: Sun Apr 10 03:35:47 2016 Кодировка: Поисковые слова: spiral galaxy

EYEPIECE
Journal of the Amateur Astronomers Association of New York May 2009 Volume 57, Number 5, ISSN 0146-7662

A Look at Astronomy's Present and Its Exciting Future
By Terrell Kent Holmes
Dr. Richard Tresch Fienberg, former editor-in-chief at Sky & Telescope, came of age at a time when mankind took its f irst steps on the Moon, Mount Palomar was the world's dominant telescope and quasar was more popular as a brand of television than an astronomical object. During his April 3 AAA lecture at the AMNH, "The More Things Change," he enthusiastically discussed the many changes that have transpired during his life in astronomy, and provided informed speculation about what might happen in the future. 2009 is the International Year of Astronomy (IYA), and the lecture coincided with "100 Hours of Astronomy," a weekend where astronomers in 100 countries trained their scopes on the skies and shared their views on a website devoted to the event. The highlight was a 24-hour online tour where 80 professional observatories worldwide provided close-up views to the public of objects like Saturn, the Sun and the Moon. As the Earth rotated, Fienberg noted, the observational reins were passed to another dark-sky site in another time zone. This kind of shared global experience exemplif ied one of the important ways in which astronomy has evolved in the past generation. At the Franklin Institute in Philadelphia, there's currently an exhibit devoted to Galileo, the centerpiece of which is the small refractor he used 400 years ago to make the observations that changed scientif ic, religious and world history forever. After proudly showing a photo of himself holding Galileo's actual telescope, Fienberg displayed the Galileoscope, an inexpensive, easy-to-assemble telescope similar to Galileo's, developed in conjunction with the IYA. Fienberg is one of the people behind the scope which, at 25 to 50 power, can capture what Galileo saw, such as Jovian moons, lunar craters and Saturnian rings. So what the great Galileo used to change the world is now mass produced to pass the time. Fienberg illustrated the new astronomical landscape with a simple question: How many planets are there in the solar system? The answer speaks to phenomena such as Kuiper Belt Objects, leading us to re-examine parameters such as planetary def inition, which subsequently led to Pluto's reassignment. The recent discovery and direct observation of extrasolar planets has expanded the boundaries of our knowledge to frontiers even beyond H.G. Wells' imagination. Fienberg also expects astronomers to f ind exoplanets orbiting stars within a habitable zone that will eventually lead to discovery of life forms. He even suggested (jokingly) that the Search for Extrater restrial Intelligence (SETI) would receive a signal from alien intelligence. Computers have changed everything forever. From providing and storing data, to online observing to the application of technology in telescopes, computers have improved observing techniques and the speed of data processing. Observing techniques are far smoother now that scopes with go-to capability eliminate much time-consuming guesswork. in f inding objects. Some large telescopes, according to Fienberg, can change the shape of their mirrors to conform to weather patterns. Fienberg discussed how the advent of adaptive optics has provided better observing and photographic experiences for all astronomers. Indeed, the gap between the quality of amateur and professional photography has narrowed considerably. Fienberg noted that many photos he chose for the cover during his tenure at Sky & Telescope wouldn't even be considered today because of their comparatively mediocre quality. We're in a kind of golden age, where excellent equipment is affordable, there's a plethora of info available online and there's a new era of collaboration between amateur and professional astronomers. But Fienberg warned of a downside to all of this. With all this progress, something will always be lost in translation, and he fears that with all of the changing nature of the media and how information is disseminated, some seemingly stalwart publications will fold. He also predicts that solid astronomy journalism will be replaced by blogs. Evidence of this shift is already occurHolmes continued on page 3


What's Up
By Tony Hoffman
The Sky for May 2009
May's Constellations. Winter's bright stars linger in the early evening sky, though they're gradually sliding into the solar glare. Sirius and Orion set early, along with Taurus. As the month opens, Mercury can be seen as a f irst-magnitude "star" next to the Pleiades. By month's end, Castor and Pollux will stand side by side above the twilight in the west, with Procyon and Capella near the horizon to their lower right and left, respectively. Virgo and Ursa Major will be on the meridian as the sky darkens, with Leo starting its westward swing. Saturn will lie in eastern Leo, below Denebola, and will shine slightly brighter than Regulus. A telescope will show its rings nearly edge-on, but more open than a few months ago. Jupiter, in Capricornus, won't rise until well after midnight. Venus will blaze in the predawn sky, lying not far from Mars around midmonth. Between the Big Dipper's bowl and Virgo's Y lies Coma Berenices, a constellation that's mostly made up of an open cluster. Although washed out from the city, it is still a f ine sight in binoculars. For those with telescopes, the Coma Berenices/Virgo/Leo/Ursa Major region will abound with galaxies. Arcturus will cross the meridian a couple hours after dark, as Scorpius--with its brilliant heart, Antares-swings up out of the southeast. Trailing Arcturus will be Corona Borealis, Hercules, and the Summer Triangle of Vega, Deneb and Altair. May 1 May 2 May 4 May 5 May 9 May 10 May 17 Jupiter. May 21 May 24 May 25 May 30 Saturn. First-quarter Moon at 4:44 p.m. Venus is at its brightest in the morning sky. Moon lies near Saturn. Eta Aquarid meteor shower peaks. Full Moon at 12:01 a.m. Moon lies near Antares. Last-quarter Moon at 3:26 a.m.; Moon lies near Moon lies near Venus and Mars. New Moon at 8:11 a.m. Moon at perigee. First-quarter Moon at 11:22 p.m.; Moon lies near

Venus Could be Seen in Bright, Blue Sky
By Joseph A. Fedrick
Venus disappeared from the evening sky during late March, but was still visible in my 10x50 binoculars as an easily discernable thin white crescent on March 21 and 22 at around 1 p. m, and March 24 and 25 at around 5:30 p. m. in a bright blue sky. The crescent of light faced southwest toward the Sun. Locating Venus in bright daylight was quite challenging. However, the fact that Venus was passing well north of the Sun made it possible to see it up to two days prior to its inferior conjunction with the Sun. Venus passed 8.2 degrees north of the Sun on March 27, but cloudy, hazy skies prevented my observing it that day. The orbit of Venus is at a 3-degree angle to the ecliptic. However, because Venus is relatively close to the Earth, the view from Earth of Venus was at a steeper 8.2-degree angle. This geometry was discussed by AAA president Rich Rosenberg at a meeting of the Observers' Group at the club's new headquarters. Jupiter climbed out of the horizon haze skies by late March so that by March 25, Galilean moons with my 60 mm refractor brown-gray equatorial cloud belts with my 50x and 100x. into dark nighttime I could see its four at 50x and the two 60 mm refractor at weren't quite edge-on, but still tilted slightly so I could see the outer dimmers of the A ring; the inner, brighter B ring, and could barely discern the Cassini division between the A and B rings. Faint cloud belts were barely discernable on Saturn's pale tan-yellow disk.

Explorers Club Program
"From Galileo to Hubble and Beyond: The Exploration Challenge" is a day-long program at the Explorers Club, 46 East 70 St., Saturday, May 2. Astronomers, astronauts and journalists will be featured at the public event, which runs from 9 a. m. to 7 p. m. and includes lunch and a reception The event will feature presentations from traditional space and aeronautical disciplines to emerging f ields in space exploration. Speakers include NASA's Jer ry Bonnell, co-creator of the astronomy picture of the day; Dr. Steve Squyres, principal investigator responsible for the scientific activities of the Mars robots Opportunity and Spirit; and astronaut Dr. Leroy Chiao, a veteran of four space flights and six space walks. Tickets will not be sold at the door. Call 212-628-8383 or e-mail reservations@explorers.org. Member and guest tickets are $55, students $25.

Saturn presented a spectacular view of its rings in Michael O'Gara's 76 mm apochromatic Pronto refractor at approximately 120x with use of a Barlow lens. The rings

2


A Message from AAA President Richard Rosenberg
Hello members: The annual meeting of the Amateur Astronomers Association will be held on Wednesday, May 20 at our headquarters, 120 Warren Street in lower Manhattan. We'll be in the large room on the ground floor. The meeting will get underway with a buffet dinner at 6 , a half hour earlier than in past years. The business meeting will begin at 7:15. Officers and committee chairs will speak, letting you know how we're doing and what issues we're currently dealing with. Members will then vote to fill six of the 18 seats on our board of directors. If you haven't been to an annual meeting, or even if you have, officers and committee chairs would very much like to meet you and hear your opinions: what we're doing well, what not so well and changes you'd like to see. After the annual meeting, the board will meet to elect officers for the coming year. On Friday, May 1, AAA member Denton Ebel of the American Museum of Natural History will conclude our 2008-09 annual lecture series at the museum. Dr. Ebel will speak on "Stardust Findings and Meteorites: New Constraints on Solar System Formation Models." The lecture runs from 6:15 to 8 p. m. The following Tuesday, May 5, at 7 p. m., I will speak on the spring sky at the Avenue U Salt Marsh Nature Center in Brooklyn. Weather permitting, this will be followed by observing (the location is quite dark by NYC standards). For directions, check our website at www.aaa.org or call me. Spring is finally here. We have observing sessions at no fewer than eight locations in May, plus the Observers' Group meeting

AMNH Geologist Ebel to Address the AAA May 1
Denton Ebel, curator-in-charge of the Department of Earth and Planetary Sciences at the American Museum of Natural History, will deliver the f inal lecture of the AAA's 200809 lecture series when he discusses "Stardust Findings and Meteorites: New Constraints on Solar System Formation Models" Friday, May 1. The free public lecture begins at 6:15 p. m. in the Kaufmann Theater of the museum. The Stardust mission returned to Earth the f irst solid extraterrestrial samples since the Apollo era, Ebel notes. "Combined with meteorites and interstellar dust particles (IDPs), this sample suite provides fundamental facts that must be explained by all theories that are proposed to explain dynamic phenomena in our early solar system (and others). These are `constraints' in that any theory of solar-system formation must explain them. I will discuss Stardust, meteorite and IDP evidence that all bear on the processes at work in the earliest protoplanetary disk." Ebel, a geologist specializing in the study of rocks from space, is the curator of the AMNH's meteorite collection. "Our mission is to make meteorite samples available for research by scientists throughout the world. Collections-based research is vital to the exploration of space and a better understanding of our origins." In 2003, Ebel served as lead curator in reimagining the museum's new Arthur Ross Hall of Meteorites. One focus of his research is modeling how gas, solid and melt phases interact at high temperatures and low pressures to understand formation of the f irst solids, and molten (liquid) rock droplets in the solar system, which eventually led to accretion of planets. He also applies X-ray, CAT-scan and microscopic imaging to meteorites to get two- and three-dimensional images of how they're put together. Ebel began his career by investigating how silver, copper, nickel and platinum-group metal ores form in the Earth. By seeing how sulf ide minerals react, he was able to model their thermodynamic properties and develop predictive tools to f ind metal-rich rock in existing Holmes continued from page 1 ring as newspapers cut science reporting. Another thing that may fall by the wayside, Fienberg warned, are signif icant discoveries, such as comets, made by amateurs. The prevalence and quality of professional equipment, and the improvement of around-the-clock observing, make it less likely for amateurs to f ind a significant wedge through which to make such discoveries. The playing f ield has expanded to the point where, on this level, it has nearly defeated its purpose. (But Fienberg's successor at Sky & Tel, Robert Naeye, last month noted the major amateur role in exoplanet detection--see story on page 5.)

3


A Memorable Lights-Out Night in Inwood Park
By Jason Kendall
April 3rd. What a night. The result of collaboration with the Parks Department to create a darksky environment in Inwood Hill Park. The clouds looked foreboding, but we persevered. I made the call to goforward at about 10 a. m. The Clear Sky Clock looked f ine, even improving. I told the Parks Department we were on. The night before,the Park Rangers and I spoke about what we would do in case of clouds,which basically amounted to me standing under an umbrella saying I am sorry. I was at the entrance at 6:30, with papers, bags and a GalileoScope,but no one else. It was just me and the clouds, lowering ominously over my head. However, I was conf ident the clouds would clear and amateur astronomers would appear. Very soon, they did. For about 20 minutes,clear sky popped out to show the Moon overhead in the blue sky. Feeling a bit cocky about the exiting clouds, I tried to hand-hold the Galileoscope up to the Moon. It was tricky, but I could see it nicely through the f inder. I tripod really helps. Shortly after 7:15, the telescopes arrived! Howard, Alice, Javier, Daryl, Tony, Tom and others. They walked into the park or drove in to drop off their wares. They were glad the event was going forward, even though clouds, and once or twice lightning, to the north gave warning. But here we were, and the Rangers showed up. We set up a table. Stragglers walked by. I started cutting up shreds of red cellophane for flashlights. People unexpectedly started arriving. Jennifer Hoppa, head of Northern Manhattan Parks, showed up. The crowd was only a bit put off by drizzle at 7:50. People were lively and animated, but their faces wished it was a lazy summer night with stars above rather than a slightly rainy night with iffy possibilities. At 8:30, with 50 people waiting to go in, Jennifer and electricians drove into the park. The crowd then walked north into the park to waiting astronomers. David Teich and I stood at the entrance in a slight drizzle, feeling forlorn and looking at the clouds. Then we saw the park lights go out. There we were, David and I, standing in front of a darkened park's entrance under an umbrella in a drizzle. The dream seemed a Pyrrhic victory. Working so hard and pushing so hard, only to see it cloudy and a bit rainy. At this point, Manhattan Parks Commissioner William T. Castro and Fort Tryon Preservation Society President Nancy Bruning walked up. We had a brief chat, and David graciously stood at the entrance while I walked into the park with them. The commissioner was quite pleased with the event, and wanted to do it again. I was also able to tell him how the parks could save money with downward-directed lighting f ixtures. He commissioner was all ears about saving money. At the location, my spirits rose. Here were all these people, and the telescopes all set up, hoping the clouds would clear. The park lights were out. The work we had all done had reached fruition. I hopped onto a table and started talking to the crowd, trying to keep the mildly let-down group from walking away. After introducing AAA members Tom Haeberle, Tony Hoffman and Alice Barner, I introduced the commissioner. Everyone noticed they could see better in the dark than they thought they could. It stayed cloudy until about 10. Then the clouds began to break, and the astronomers jumped at the chance to show people the sky. The Moon shone f iercely through, then Saturn in the high east. The clouds suddenly parted to show the entire Big Dipper. Castor and Pollux leaped out. All the stars were bright against the high darkness. Without the park lights, people could make out the brightest stars. Everyone had a chance to see Saturn, with its brilliant edge-on rings. One attendee even used his iPhone to snap a shot through Javier's 8" Celestron. There were a lot of people who'd never looked through a telescope. That was the most important aspect of the evening. For the next half-hour, oohs and aahs could be heard. During the evening, everyone I talked to said they knew a few people who would have come if it were not cloudy. By counting their estimates, the parks people and I thought a clear night would have produced 2,000 people. Commissioner Castro told me we need to do this again. And we shall. AAA Members should write a letter thanking him for putting on the event, the f irst lights out of a New York City park. Borough Commissioner William T. Castro is at Arsenal West, 24 West 61st Street, 5th Floor, New York, NY 10023. We need to show the city our appreciation for f inding the resources to do something that was thought impossible by most.

The AAA's Annual Meeting Is Wednesday, May 20 See President's Letter on page 3 for Details

4


Democratic Takeover of State Senate May Aid Light Bill
By Dan Harrison
The Democratic takeover of the New York State Senate in last year's election creates a "really good chance" of passage of light-pollution legislation this year, Assemblywoman Linda Rosenthal (D-Manhattan), lead sponsor of such legislation in the Assembly, told Eyepiece last month. Further enhancing chances of passage is the fact that Senator Antoine Thompson, the new lead sponsor in the upper chamber, heads the Senate's Environmental Conservation Committee, to which the bill has been referred. Rosenthal terms the bill (A7281, S2714), introduced in late March, one that Republicans and Democrats can agree on. "The whole topic of light pollution and people's growing interest in seeing the night sky without glare" should be further boosts to the bill, she said. Another factor that may help the bill is that Thompson is from upstate. He represents a district that includes Niagara Falls and part of Buffalo. Observers believe that the combination of New York City and upstate prime sponsors often enhances chances for a bill's passage. "Buffalo is a good balance," Rosenthal said. "It signals support from disparate areas. You can't use excuses based on geography." Yet another factor, says a source, is that "Thompson won't check with New York City the way [Nassau Republican Carl] Marcellino [the previous prime sponsor in the Senate] did." On the other hand, Democrats have a razor-thin majority of three seats in the Senate, and no Republican voted for the state budget. In an interview with Eyepiece, Thompson agreed that chances for passage of light-pollution legislation have been tangibly enhanced by the Democratic takeover of the Senate. As for why he is lead sponsor for the bill, he said, "Being chair of the Senate Enviroment Conser vation Committee, I'm trying to move New York into more 'green' initiatives, and this is just another way of doing that. The environment is very important and we need to take care of it. But Thompson disagreed that lead sponsors from New York City and upstate enhance the chances for legislation: "We're not upstate or downstate. We're one New York and it's not about where the sponsors are from. It's about what is good for New York." For the past decade, such legislation has usually been bottled up in Senate committee. The one time a light bill was passed by the full Senate, in addition to typical passage by the Assembly, it was vetoed by then-Governor George E. Pataki. Rosenthal said she expects a full Senate vote this time around. The Healthy, Safe and Energy Eff icient Outdoor Lighting Act restricts installation of new lighting by state agencies or public corporations operating in the state to fully-shielded luminaries. Various exemptions to the requirement are contained in the bill. The Public Service Commission is directed to require that every electric corporation or municipality providing electric service include educational pamphlets in bills to customers. Luminaire-eff iciency and lamp-luminous-eff icacy standards must be developed. The Department of Environment Conservation (DEC) is empowered to identify and nominate areas for dark-sky preserves. State agencies, public corporations and electric corporations providing roadway lighting under contract to a public corporation are exempted from light-trespass restrictions. This is viewed as a key concession. However, the DEC, in consultation with relevant authorities, must promulgate regulations on light trespass. The DEC must prepare and distribute a model outdoor lighting ordinance to municipalities. And the department would be required to develop and widely disseminate a pamphlet describing the purposes and provisions of the act. In addition to this bill, Rosenthal has introduced several others: · A 5769 "expands the powers and duties of the Department of Health to engage in and support research into the health effects of artif icial night light." ·A 5655 "adds the elimination of wasteful artif icial night lighting to state lighting eff iciency standards. · A 5656 "expands the type of energy information compiled by NYSERDA to include energy-eff icient and environmentally sound outdoor lighting." · A 7276 "amends the Environmental Conservation Law to include the preservation of the "nighttime sky" as part of the declared policy of New York State."

5


Amateurs Will Still Play Big Role in Exoplanet Detection
By Dan Harrison
Amateur astronomers, who have played a major role in detecting exoplanets, will continue to do so and broaden their activities, Sky & Telescope editor-in-chief Robert Naeye told the Northeast Astronomy Forum in Suffern, N. Y., April 19. "Against all predictions, amateurs in their own backyards are involved in exoplanet discoveries," Naeye said. "They've made very signif icant contributions in transiting discoveries and g ravitational microlensing. Ver y few astronomers would have predicted this 20 years ago, when planets outside the solar system were unknown." Professionals depend on amateur data and want amateurs to continuethis work, Naeye said. "Professionals are very deeply respectful and appreciate the role played by amateurs. Thanks to the combined efforts of professionals and amateurs, we're starting to get pretty good ideas of what the numbers are." Of the 340 exoplanets discovered since 1991, there are 58 known transiting planets, and then number is rising fast, Naeye noted. "Most have been detected by amateurs, including all of the really scientif ically signif icant ones. Amateurs are focusing many efforts through transit search.org, which focuses on longer-period planets, ones that professionals won't or rarely bother to observe because of the low probability of transits. Naeye expects that many transiting exoplanets will be found, including those smaller in size than gas giants will be found. The radial-velocity or "wobble" method has borne the most fruit, Naeye said, resulting in a large majority of exoplanets found. "An alien could easily f ind Jupiter and Saturn by this method." The wobble method is geared to f inding massive planets relatively close to their host stars. "Amateurs have detected exoplanets using radial velocity. There haven't been amateur discoveries yet, but stay tuned," Naeye said. "Lower-mass exoplanets have the best prospects for f inding life as we know it." A key to all this amateur activity has been improvements in technology. "By 2000, amateurs had access to very high-quality and affordable CCD cameras that allowed them to monitor stars' brightness to a precision of about 1%. This is easily enough to detect a drop in a star's light from transit of a hot Jupiter. "So suddenly amateurs could enter this game and play a meaningful role. Since then, with improved equipment and software, precision is now down to 0.1%." This brings in a whole host of transiting exoplanets amateurs can detect. They can also detect elements and molecules in some exoplanets, at least in upper atmospheres, due to absorption lines in the spectrum. "In sionals narrow did this one case, the data were so good that some profesmonitoring this used his data in a paper. It helped down the diameter of the planet. And the amateur just a few days after hearing of the transits."

In 2005, Naeye recalled, an exoplanet was detected by professionals. "Before the transit was announced, an amateur detected it and a much smaller planet with only a .003 magnitude decrease in the star's brightness. Early amateur successes motivated some professionals to start organizing amateur efforts to f ind transiting exoplanets. This led to transit.org, which has assembled a worldwide network of amateurs to measure brightness to a precision better than 1%. It's organized at least 20 observing campaigns, concentrating on stars known from radial-velocity surveys." The 1%-10% probability of a planet transiting a star isn't good enough for professionals, Naeye noted, "but you have an eager group of skilled amateurs around the world. The jackpot for transitsearch.org came in 2007, when a transiting planet that wasn't a hot Jupiter was found transiting its star. It has a 21-day orbit vs. the previous record of f ive-to-seven days. Since then, the new record has come in at 111 days. The two planets have highly eccentric orbits. Gravitational microlensing, another key way of discovering exoplanets, has been fruitful for amateurs, Naeye said. In 2005, amateurs not only discovered a transit but the planet itself. "Gravitational microlensing could reveal the existence of an Earth-mass planet. It's a very sensitive method." Amateurs have helped discover a system containing a star with two planets, analogs of Jupiter and Saturn. In the future, Naeye predicted, amateurs will be able to discover new planets in a system in addition to a transiting planet by observing seeing variations in timing--i. e., gravitational perturbations indicating a second body. In addition, there will be more amateur discoveries of long-period transiting exoplanets. There will be more gravitationalmicrolensing discoveries, including low-mass exoplanets perhaps just a few times Earth mass. Finally, "Amateurs could discover or conf irm a moon orbiting an exoplanet through a wobble by a planet from a massive moon.

6


Review: Do Exoplanets Crowd the Universe?
By Tony Hoffman
We live in perhaps the most exciting period of astronomical discovery since Galileo f irst pointed his telescope to the skies 400 years ago. Nowhere is that more evident than the hunt for exoplanets. Since 1996, more than 340 such worlds have been discovered. In "The Crowded Universe: The Search for Living Planets" (Basic Books, $26), Alan Boss, a Carnegie Institution astrophysicist, provides a lively account (for the most part) of these extraordinary times through the eyes of someone who's been at the forefront of the quest for other Earths. The book begins with an involved explanation of the Doppler Effect as it applies to spectroscopic observation of starlight. It's used to detect the slight wobble in a star's motion indicating the presence of an unseen companion that could be a planet. On reading that section, I was concerned the book would be diff icult, delving deep into science, a necessary part of understanding the subject at the expense of readability. On that score, I was pleasantly mistaken. While it doesn't skimp on the science--Boss is particularly thorough on the subject of planetary formation, on which he is an expert--it's by and large fairly easy and often absorbing reading, a chronology broken into dated entries, spread over the past 14 years, from before the f irst exoplanet discovery in 1995 until late last year, as the Kepler mission to search for Earthlike worlds (for which Boss has served as a science advisor) awaited clearance to launch. Much of the account describes discoveries of the growing and varied menagerie of exoplanets (loosely classed as Jupiters, Neptunes or super-Earths depending on their size, and hot or cold by how closely they orbit their star) by competing teams of astronomers using several techniques: spectroscopy (using the Doppler effect to detect changes in a star's radial velocity); the transit method (f inding planets by measuring the slight, periodic dimming of a star when a planet passes in front of it); and microlensing (the bending of light by the gravity of an unseen object to cause a more distant star to brighten briefly). Boss details the f inding of ever-smaller worlds in the quest to f ind other Earths. We're not quite there yet, but are coming close, and he has every expectation the Kepler mission will f ind many of them. Kepler employs a 38-inch space telescope that will monitor a f ield of 100,000 stars for four years, looking for the minute changes in brightness that could signal the presence of a planet transiting a star's face. The smaller, European CoRoT space telescope is conducting a similar quest. The planets it's found so far have been larger than Earth. Boss covery of demotion planet is, also touches on related topics such as the (alleged) dismicro-organisms in a meteorite of Martian origin, the of Pluto and the controversy over def ining what a and especially the turf wars and personnel changes at NASA as well as the agency's budget battles, particularly after the Bush Administration diverted money from NASA's scientific missions to its plans to return men to the Moon and eventually to Mars. This has resulted in downsizing or cancellation of exoplanet search missions, as well as delaying Kepler. At the end of the book, Boss looks ahead to the Kepler mission, which was launched two months ago and released its f irst test images last month. The book's epilogue, "Why Don't You Ever Call?" tackles the subject of possible life elsewhere in the cosmos, based on the latest science and Boss' own informed speculation--he's clearly an optimist. He writes, "Given that Kepler will be able to produce a good measure of the frequency of Earth-like worlds, provided this frequency is 5% or more [that is, 5% of Sun-like stars possess such planets], there is every expectation that the Kepler Mission will succeed in determining this most basic parameter in any estimate of the prevalence of life in the universe. Even the CoRoT mission has a good chance of discovering an Earth or two in such a crowded universe."

Arthur Code Dies at 85
Arthur D. Code, one of the most noted astrophysicists of his generation, died March 11 at 85. He was a pioneer in space astronomy, leading initiatives to put telescopes and other instruments in space. Long before the Hubble, Code worked to get telescopes into space. He built the world's f irst successful orbiting obser vator y, the Orbiting Astronomical Obser vator y, launched in 1968. The satellite carried light meter