Physics Update

Persistent currents in normal metals

2009-11-05T16:48:04Z

In the absence of an applied voltage, an induced electrical current rapidly decays thanks to the scattering of electrons from defects, phonons, and each other. But in a cold metal ring smaller than the electron’s coherence length, it’s possible to induce a dissipationless current, even if the metal is not superconducting. The trick, theorists predicted in the early 1980s, is to thread the ring with a magnetic field, which breaks time-reversal symmetry. The current is revealed only by its magnetic moment μ. And although researchers confirmed the effect early on, mostly using superconducting quantum interference devices (SQUIDs), complete agreement between theory and experiment, and even among experiments, has remained elusive. Jack Harris and colleagues from Yale University and the Free University of Berlin have now developed an elegantly simple alternative measurement scheme. The team deposited aluminum rings on a cantilever whose vibration frequency can be precisely monitored. In a magnetic field B, each ring’s current produces a torque τ = μ × B, recorded as a shift in the cantilever’s resonance frequency of vibration. From that frequency shift, the researchers deduce the current with a precision two orders of magnitude greater than is possible using SQUIDs. For a magnetic flux threading the ring, the current exhibits an Aharonov–Bohm effect, measurable as oscillations, shown here, whose period corresponds to the addition of one flux quantum h/e through the ring. In experiments taken over a broad range of fields, temperatures, and ring sizes, Harris and coworkers find perfect agreement with a noninteracting electron model. (A. C. Bleszynski-Jayich et al., Science 326, 272, 2009.)—R. Mark Wilson

Chromosome folding

2009-11-02T14:50:49Z

Stretched out completely, a human chromosome would be several centimeters long. It is packed, along with its 45 companions, into a few-microns-wide cell nucleus in such a way that all the necessary genes are accessible to RNA transcription. Figuring out how that packing is done is no easy task. Microscopy helps, but provides nowhere near a complete picture. Now a research team led by Eric Lander of MIT and Job Dekker of the University of Massachusetts has developed a method for probing chromosomes’ folded structures. The researchers chemically join segments of a folded chromosome that are close in space, cut away and sequence the DNA around the crosslink, and compare those sequences to genome libraries to determine which parts of the chromosome are in contact. A matrix of the observed contacts, as shown in the figure, reveals large-scale organization. Analyzing the plaid pattern, the researchers found that most of the cell’s actively transcribed DNA was spatially segregated from most of the inactive DNA. On a smaller scale, chromosome segments a millimeter or so in extended length appeared to form so-called fractal globules with self-similar structures very different from that of a tangled polymer in equilibrium. So far, the researchers have studied only cultured cell lines: one derived from a tumor and another modified by a virus. They hope to apply their method to healthy cells and to look for differences in chromosome structure among cells of different types. (E. Lieberman-Aiden et al., Science 326, 289, 2009.) —Johanna Miller

Accelerating neutral atoms

2009-10-29T17:25:48Z

The intensity gradients of inhomogeneous laser-light fields impose ponderomotive forces on charged particles. Such forces have been used to trap and manipulate ions, diffract electrons, and generate charge waves in plasmas. But they were thought to act only very weakly on neutral atoms—having to rely on the polarizability of an atom’s charge distribution. Now, however, a group at the Max Born Institute in Berlin has reported the use of intense ultrashort laser pulses to accelerate neutral helium atoms for about 100 femtoseconds at 10¹⁵m/s². That’s eight orders of magnitude greater than the acceleration (or deceleration) one can get with the continuous-wave techniques used in laser cooling of neutral atoms. The ponderomotive force of an inhomogeneous light field pushes a charged particle toward lower light intensity with a force proportional to the square of its charge—irrespective of sign—and inversely proportional to its mass. The Berlin group argues that the strong laser pulse excites an electron to the outer reaches of the helium atom where it “quivers” in the oscillating light field and experiences the ponderomotive force almost as a free electron would. But still bound to the atom’s ionic core, it tugs the much heavier core with it away from the laser beam’s focus. The figure shows how the maximum velocity thus acquired by neutral atoms in the Berlin experiment increases with pulse duration. The dashed curves show the theoretical expectation for the group’s model of electron excitation and the consequent ponderomotive force. Such “ultrastrong” acceleration of neutral atoms, they suggest, could be exploited for atomic-beam optics, atom deposition, and controlled chemical reactions. (U. Eichmann et al., Nature 461, 1261, 2009.) —Bertram Schwarzschild

A mantis shrimp’s extraordinary eyes

2009-10-26T17:12:00Z

Photonic devices that can detect and control the polarization of light across a range of wavelengths are rare. More common are materials such as quartz that can be made into monochromatic optical retarders, which through their intrinsic birefringence convert a specific wavelength of linearly polarized light into circularly polarized light, or vice versa. Some multilayered thin films exhibit achromatic retardation through fabricated periodic nanoscale structures that effectively combine the dispersive properties of each layer to achieve wavelength-independent birefringence. But engineering nanoscale structures is tricky, and even the best synthetic achromatic retarders perform poorly across the full visible range, varying by as much as 9.1°. But Nature has already solved the puzzle in animals that have evolved biophotonic structures for signaling, vision, and coloration (see Physics Today, January 2004, page 18). Now, an international team of researchers from the UK, Australia, and the US has discovered a near-ideal achromatic retarder in the eyes of the colorful peacock mantis shrimp, Odontodactylus scyllarus, shown in the image. This mantis shrimp’s biophotonic retarder is the R8 photoreceptor cell—a UV-photopigment-filled lipid bundle with critical radii of 26 nm and 40 nm, which are subwavelength for visible light. When subjected to linearly polarized light, the R8 cell acted as a quarter-wave retarder, converting the incident light to circularly polarized light, as confirmed by close experimental agreement with theoretically determined Stokes parameter values. Moreover, the extent of retardation varied by only 2.7° across the visible spectrum. (N. W. Roberts et al., Nat. Photonics, in press, doi:10.1038/nphoton.2009.189. Image courtesy of Roy Caldwell, University of California Berkeley.)—Jermey N. A. Matthews

Trading farms and forests for biofuel

2009-10-22T18:25:18Z

With political sentiment growing in favor of greenhouse gas (GHG) restrictions, biofuels from plant cellulose are being considered among the alternatives to fossil fuels: Plants are renewable and biodegradable, and they sequester carbon. Yet a new report validates concerns that a global biofuels program could put intense pressure on land supply and distribution. To predict the impact of a biofuels-based economy on climate change, an international team of researchers from the US, Brazil, and China linked an economic model of land use with a terrestrial biogeochemical model of global GHG levels. The team considered two cases for cellulosic biofuel crop growth: The primary focus of case1 is on converting unfarmed areas such as forests, as shown in the image; of case 2, on exploiting existing farmland to the extent possible. In both cases, biofuel feedstock becomes a dominant global crop by year 2100, but in the process, total forest area is cut—by 56% in case 1 and by 24% in case 2. The loss of carbon-sequestering trees in case 1 results in a net release of carbon. In case 2, the gains from biofuel production ultimately lead to increased carbon sequestration in the farmed soil from the addition of nitrogen fertilizer, which paradoxically releases N₂O, another potent GHG. The research suggests that stabilizing GHG levels will require a limited and more efficient use of forests and fertilizers for biofuel crop production. (J. M. Melillo et al., Science Express, 22 October 2009, doi:10.1126/science.1180251. Image courtesy of Chris Neill, Marine Biological Laboratory, Woods Hole, MA.)—Jermey N. A. Matthews

Rough surface gives drops the heave-ho

2009-10-16T21:36:21Z

A common step in industrial cooling processes is the liquefaction of a vapor on a condenser. If, however, a liquid film forms on the condenser, the cooling may be compromised. The problem can be addressed by coating the condenser with a hydrophobic material conducive to drop formation and then letting the drops slide off due to gravity. Now Chuan-Hua Chen of Duke University and his student Jonathan Boreyko report a different approach. By depositing carbon nanotubes on silicon micropillars and coating both with hexadecanethiol (C₁₆H₃₄S), they engineered a rough “superhydrophobic” surface. The water drops that condensed on it were about a hundred times smaller than those on a conventional hydrophobic surface that the Duke team considered as a standard; the surface roughening offers the promise for more efficient cooling. Furthermore, as the figure and video show, when two sufficiently large drops coalesce into a single drop, that drop literally springs off the condenser—no external prompting needed.

The post-combination drop has less surface energy than do the two drops from which it forms. Most of the released surface energy is dissipated, but Chen and Boreyko observed that the vertical component of the drop’s velocity can be as much as one-sixth of the theoretical maximum. Nature has her own version of the jumping trick. Coalescence of a wet portion of a spore with a dew drop provides the energy for spore ejection in certain mushrooms. (J. B. Boreyko, C.-H. Chen, Phys. Rev. Lett., in press.) —Steven K. Blau

Yoctosecond light pulses from quark-gluon plasmas

2009-10-16T13:45:51Z

In recent years, photon pulses in the attosecond (10^-18 s) regime have been precisely engineered and are being increasingly put to work—for example, in experimental quantum control and chemical dynamics (see Physics Today, March 2005, page 39). But can much shorter pulses be generated and put to use? Three physicists at the Max Planck Institute for Nuclear Physics in Heidelberg, Germany, have proposed some answers. They modeled the photon emission in the early expansion of a quark–gluon plasma, a hot dense stew of fundamental particles created when heavy nuclei smash into each other at relativistic speeds. Prompt gamma rays in the GeV range, produced primarily by quark–gluon Compton scattering and quark–antiquark annihilation, would exit the expanding QGP in at most a few yoctoseconds (10^-24 s). With certain collision parameters and detectors nearly aligned with the collision axis, the model predicts a double-peaked pulse before the QGP disappears. One peak is blueshifted, arising from the approaching side of the QGP, the other is redshifted from the receding side, and the peaks are separated roughly by the light-travel time across the hot soup. The dip between the peaks occurs during an intermediate time at which the stew acquires an anisotropy and emits nothing in that direction. If the model proves correct, such a double pulse could enable pump–probe experiments at the nuclear scale, though new detection schemes would first need to be invented. (A. Ipp, C. H. Keitel, J. Evers, Phys. Rev. Lett. 103, 152301, 2009.) —Stephen G. Benka

Nanoscale view of colossal magnetoresistance

2009-10-12T13:49:57Z

Colossal magnetoresistance is aptly named. By subjecting a piece of appropriately doped manganite to a strong magnetic field and a moderately low temperature, one can raise its electrical conductivity by 10 000%. Despite its prodigious magnitude, CMR has not led to any commercial devices since its discovery 15 years ago. Still, it continues to fascinate physicists. At its most basic level, CMR arises as a paramagnetic insulating phase yields to a ferromagnetic conducting phase. But evidence suggests that a third, charge-ordered antiferromagnetic phase could play a role too. To elucidate the issue, Jing Tao of Brookhaven National Laboratory and her collaborators developed a new experimental technique. Called scanning electron nanoscale diffraction (SEND), their technique combines electron diffraction's ability to reveal the presence of ordered structures with scanning microscopy's ability to reveal those structures' real-space distribution. The patches in the figure correspond to charge-ordered regions. As the temperature approaches the 253-K CMR transition, the volume occupied by the charge-ordered phase increases. Simulations by Elbio Dagotto of Oak Ridge National Laboratory and his collaborators suggest an explanation: The charge-ordered phase vies with the ferromagnetic phase to become the predominant phase below the transition temperature. Although it loses the battle, the charge-ordered phase nevertheless delays and thereby intensifies the onset of CMR. (J. Tao et al., Phys. Rev. Lett. 103, 097202, 2009.)—Charles Day

Understanding ferromagnetism in graphite

2009-10-08T17:16:33Z

Ferromagnetism usually arises from transition metals rich in 3d and 4f electrons. The occurrence of ferromagnetism in pure carbon, which contains only s and p electrons, is thus surprising—even controversial, given the weakness of the magnetic signal and a Curie temperature well above room temperature. Using magnetic force microscopy and a superconducting quantum interference device to probe the surface and bulk magnetization of graphite, Netherlands researchers Jiri Červenka and Kees Flipse (Eindhoven University of Technology) and Mikhail Katsnelson (Radboud University) offer evidence that the ferromagnetism arises from a two-dimensional network of point defects at grain boundaries. The breaking of the lattice’s translational symmetry by the defects leads to localized electron states at the Fermi level. Because of electron–electron interactions, those states become polarized, which, in turn, leads to the formation of local magnetic moments. Grain-boundary defects are more complicated than single vacancies: The figure here shows a 2D plane of periodic defects, each an extended zigzag discontinuity that propagates through individual graphene sheets of the bulk crystal. A magnetic moment can be associated with each defect; and the step edge at the surface is a manifestation of the grain boundary buried underneath it. The Curie temperature deduced from experiment is, reassuringly, comparable to the theoretical value based on weak interlayer coupling. (J. Červenka, M. I. Katsnelson, C. F. J. Flipse, Nat. Phys., in press, doi:10.1038/nphys1399.)—R. Mark Wilson

Nobel Physics Prize honors optical fibers and CCD sensors

2009-10-07T16:11:26Z

The winners of this year's Nobel Prize in Physics are Charles K. Kao for what the Royal Swedish Academy of Sciences cites as "groundbreaking achievements concerning the transmission of light in fibers for optical communication" and Willard S. Boyle and George E. Smith for "the invention of an imaging semiconductor circuit—the CCD sensor."

]]> Fiber-optic cables are the world's information arteries. They carry internet traffic under the oceans, across cities, into offices, and, increasingly, into our homes. Today's fastest commercial cables operate at 10 terabytes per second—enough to transmit all 22 James Bond movies in 10 milliseconds. In the mid-1960s, while he was at Standard Telephones and Cables (STC) Ltd outside London, Kao and his small group of collaborators worked out the essential properties of the first generation of optical fibers for telecommunications.

Digital CCD cameras are more sensitive than their film-based predecessors and, because they produce intrinsically digital images, are far more convenient. Besides spawning a boom in personal photography, CCD sensors have revolutionized astronomy and are steadily improving diagnostic medicine. The images of nebulae, galaxies, and other celestial objects taken by the Hubble Space Telescope are not only famously gorgeous, they have also led to significant discoveries. Boyle and Smith invented the CCD sensor at Bell Labs in the late 1960s.

Higher capacity

The higher the frequency of an electromagnetic wave, the more information it can carry. By the 1960s, when Kao began his pioneering work, the UK's Post Office, AT&T, and other telecommunications companies were trying to develop optical communication. Signal generation was not the biggest hurdle. The recently invented laser, though still neither cheap nor convenient, could produce an information-carrying modulated signal.

Signal transmission, however, remained a formidable challenge. To be practical, a transmission conduit must retain information with as little loss as possible and be capable of going around corners. Some kind of transparent cable was needed. Flexible, dielectric waveguides made from plastic were already in use for microwave transmission. Could they be made to work in the optical waveband?

Kao and George Hockham, his colleague at STC, tackled the problem in a landmark 1966 paper.¹ Like others before them, they realized that a sufficiently narrow waveguide would transmit only one mode, thereby forestalling the smearing of information due to dispersion. Their key insight was to identify the role played by impurities, notably metal ions, which scatter and absorb the signal. In a perfectly pure material, the loss to Rayleigh scattering would be 1 dB/km. An impure material would suffice for practical transmission, provided loss was kept below 20 dB/km.

Of the materials Kao and Hockham tested, fused silica was the most promising. As one of Earth's most abundant materials, silica was certainly cheap, but whether it could be made into low-loss kilometers-long fibers was unclear. Although Kao's work at STC had been funded by the UK Post Office, he could not persuade the organization to finance the materials research needed to develop his idea. His overtures to AT&T also failed.

Corning Glass Works, however, did take up the challenge. By 1970, Corning's Robert Maurer and his coworkers had developed a method, based on chemical vapor deposition, to make long silica fibers from silicon tetrachloride. Doping the fibers with titanium reduced the loss to 17 dB/km, below the threshold Kao and Hockham had predicted.

A digital sensor

The impetus for Boyle and Smith's invention of the CCD came from two quite different Bell Labs projects: magnetic bubble memory and the silicon diode camera. In the 1960s Andrew Bobeck had the idea to store and retrieve data in magnetic domains or bubbles in a magnetorestrictive material. Applying a current would shift those domains underneath an array of read heads. No mechanical moving parts would be necessary.

Smith was working to develop a silicon diode camera to meet AT&T's goal of creating a telecommunications device that could transmit video as well as voice. In its underlying physics the silicon diode array is almost identical to a CCD. Photons impinging on a silicon substrate excite electrons across the material's bandgap to create a temporarily charged region. An image can be derived from those regions of photoelectric charge—provided the charge can be efficiently transferred from each individual diode.

That transfer step proved challenging. At a one-hour meeting on 16 October 1969, Boyle and Smith came up with a solution. In their proposed device, charge, like the domains of bubble memory, would reside not in individual lumps of material, but in a continuous piece. The pixels would be formed electronically by a grid of metallic electrodes that creates an array of positively charged potential wells for trapping photoelectrons.

After one exposure time, the image, consisting of the trapped charges (or absence of charges), could be extracted by applying a sequence of voltage pulses. The first pulse transfers the first row of charges to an analog-to-digital converter for readout and all the other rows of charges into the adjacent rows. Successive pulses send successive rows to the ADC until the entire image has been read out.

Within a week of their first meeting, Boyle, Smith, and their coworkers had made a prototype to test the all-important charge transfer concept. By April the following year, they published two papers in the Bell System Technical Journal: one describing the CCD concept,² the other describing a working device.³ That early device had an integration time of 16 s and could transfer all but 2% of the total photoelectric charge. Today's fastest CCD cameras can integrate images in a few 100 microseconds, and the most efficient can transfer all but 1 in 100 000 electrons.

Charles Day

1. C. K. Kao, G. A. Hockham, Proc. Inst. Electr. Eng. 113, 1151 (1966).
2. W. S. Boyle, G. E. Smith, Bell Syst. Tech. J. 49, 587 (1970).
3. G. F. Amelio, M. F. Thompsett, G. E. Smith, Bell Syst. Tech. J. 49, 593 (1970).

A new dimension in optical spectroscopy

2009-10-05T13:38:10Z

Two-dimensional spectroscopy of materials, in its simplest form, measures the change in a sample’s interaction with radiation at one frequency caused by excitation at another. First used in nuclear magnetic resonance and later applied at IR and optical frequencies, the technique can separate overlapping peaks in a complicated spectrum or probe the flow of energy through systems such as the light-harvesting molecules involved in photosynthesis. (See Physics Today, July 2005, page 23.) In 2D Fourier-transform optical (FTOPT) spectroscopy, the sample is excited not with monochromatic light but with a pair of phase-related femtosecond pulses separated by a variable delay t₁; the time-domain data are transformed into a spectrum as a function of frequency ω₁. The second field is likewise replaced by a pair of phase-related pulses, one of which is a so-called local oscillator that allows the radiated field to be recorded as a function of time t₃ or frequency ω₃. Now, Keith Nelson and colleagues at MIT have produced 3D FTOPT spectra, in which the signal is a function of ω₁, ω₃, and also ω₂, corresponding to the time t₂ between the two pulse pairs. Applying their technique to semiconductor quantum wells—a system in which electrons are excited from nondegenerate valence-band states into the same conduction-band states—they found that important pathways whose signals were indistinguishable in a 2D spectrum could often be separated in a 3D spectrum. (D. B. Turner et al., J. Chem. Phys., in press.) —Johanna Miller

Galactic cannibalism

2009-10-01T14:56:07Z

In hierarchical models of galaxy formation, large galaxies grow by ingesting dwarf galaxies and the spherical minihalos of dark matter that envelop them. Some of those dwarfs would be tidally shredded when they venture too close to the center of the “host” galaxy’s enormous halo, leaving streams of stars as long-lasting relics of the carnage. Searching within the halo of our neighboring Andromeda galaxy for such relics and for dwarf galaxies surviving intact, the Pan-Andromeda Archaeological Survey has been systematically imaging the galaxy’s environs out to a radius of half a million light-years. The newly published PANDAS stellar population-density map of the halos of Andromeda and the adjacent Triangulum galaxy shows seven relic tidal streams (circled numbers in the figure) stretching over enormous distances. One of them, emanating from Triangulum, gives evidence of a cataclysmic encounter between the two galaxies two or three billion years ago, as shown in the linked animation. The survey results thus far already put an upper limit of about 90 on the total number of surviving dwarf galaxies brighter than the detection limit (Roman numerals in the figure) within Andromeda’s halo. That’s an order of magnitude less than the number of minihalos expected from dark-matter simulations. There has long been evidence of such shortfalls around large galaxies, but PANDAS is the most systematic census of satellite dwarf galaxies to date. Perhaps, theorists suggest, dark-matter minihalos are as abundant as the simulations predict but the shortfall appears because actual star formation in most minihalos is aborted by some threshold-mass effect. (A. McConnachie et al., Nature 461, 66, 2009.)—Bertram Schwarzschild

Element 114 verified

2009-09-28T14:27:00Z

In the 10 years since researchers at the Joint Institute for Nuclear Research in Dubna, Russia, first reported producing the superheavy element 114 (see Physics Today, April 1999, page 21), some tens of other sightings of the element (as well as elements 115, 116, and 118) have been documented—but all by the same group. Now a team at Lawrence Berkeley National Laboratory, led by Heino Nitsche and Ken Gregorich, has confirmed the results. Such independent verification is important, particularly given evidence of fabricated results for other superheavy elements (see Physics Today, September 2002, page 15), but it is complicated by experimental challenges, including picobarn (10⁻⁴⁰ m²) reaction cross sections and radioactive targets. Working with the lab's 88-inch cyclotron, the Berkeley team followed a process similar to that used at Dubna: They aimed an accelerated beam of calcium-48 ions at a target containing plutonium-242. The reaction products passed through a gas-filled mass spectrometer, which separated out the nuclei of interest, to a detector that yielded energy and timing information not only for the products but also for any alpha particles or fission fragments they emitted. Amid the data the researchers collected over their eight days of running the experiment, they found two correlated chains of decays that they identified as starting with ²⁸⁶114 and ²⁸⁷114. Although the lifetimes (tenths of seconds), decay modes, and decay energies agree with the Dubna results, the cross sections measured by the Berkeley team are lower. That discrepancy, say the researchers, could be due to statistical fluctuations or to some of the element-114 nuclei overshooting the detector. (L. Stavsetra et al., Phys. Rev. Lett. 103, 132502, 2009.)—Richard J. Fitzgerald

Shaping a cell's metabolic network

2009-09-24T14:19:26Z

In a single cell, thousands of simultaneously occurring biochemical reactions carry out such functions as converting and storing energy and regulating nutrient levels; together, those processes make up the cell’s metabolic network. Computational biology involves, among other things, the linking of metabolic pathways to form a metabolic network model, a promising tool for preclinical drug studies and other medical research. However, such computational models do not traditionally include the function-determining structural details of a network’s macromolecules; for example, an enzyme’s ability to catalyze reactions and regulate the cell’s response to external stimuli is determined by its three-dimensional configuration. Now, an international team led by Adam Godzik at the Burnham Institute for Medical Research in California has taken a rare step and introduced atomic-level protein structural data to the metabolic network model of an ancient thermophilic bacterium, Thermotoga maritima, shown in this optical microscope image. The image also shows schematics of proteins in their 3D configurations, which, when they were expressed in the reconstructed metabolic network, helped the research team solve the puzzle of how proteins evolve when their cell networks grow larger.

It turns out that only 37% of T. maritima’s proteins are essential to the formation of its metabolic network; those “core-essential” proteins adopt the bulk—61%—of the bacterium’s relatively few unique 3D configurations. The finding suggests that the core-essential proteins evolved their structure to perform additional functions in distinct pathways. (Y. Zhang et al., Science 325, 1544, 2009.)—Jermey N.A. Matthews

An exoplanet as dense as Earth

2009-09-21T13:52:41Z

Of the more than 350 planets that have been observed to date orbiting alien suns, only a handful have known densities. (For more on exoplanets, see Physics Today, May 2009, page 46.) Now an international team led by Didier Queloz (Geneva Observatory, Switzerland) has introduced the newest member of that club, Corot-7b, the only exoplanet to have a measured density comparable to that of Earth. The result suggests that Corot-7b, like Earth, has a rocky composition. The planet and its host star Corot-7 were named after the Convection, Rotation, and Planetary Transits satellite, which in 2008 observed a star whose intensity periodically dimmed once every 20.4 hours—the result of a planet partially eclipsing the star. The small degree of dimming and the known size of the star established that Corot-7b has a radius about twice that of Earth’s. To obtain the mass of the planet, Queloz and colleagues turned to the High Accuracy Radial Velocity Planet Searcher, a spectrograph that could precisely measure the sinusoidally modulating Doppler shifts in the light emitted by Corot-7 as it is gravitationally tugged to and fro by the small planet orbiting it. The greater the amplitude of oscillation, the greater the planet’s mass. The result required that the Queloz team filter out obscuring noise due to sunspot-like activity on the star. As a bonus, the residual signal included a component with a 3.69-day period. Queloz and colleagues attribute that to a previously unknown second planet, about eight times as massive as Earth. (D. Queloz et al., Astron. Astrophys., in press, doi:10.1051/0004-6361/200913096.) —Steven K. Blau