testing

Actually, two types of spiral galaxies are normally recognized: "ordinary" spirals, such as M74, above. In these the spiral arms reach all the way in to the center of the galaxy. However, in the variant known as a "barred" spiral the arms originate at either end of a "bar" through the center of the galaxy. The figure to the right shows how the Milky Way it thought to appear if viewed from outside.

Physical sciences news, 12/24/07 - 12/30/07

High-energy galactic objects

Objects in our galaxy that are capable of generating hard X-rays or the even higher-energy gamma-rays are quite unusual, and therefore of significant scientific interest. A European ground-based observatory known as H. E. S. S. (High Energy Stereoscopic System) is capable of indirectly detecting TeV gamma-rays. One of the sources it has found, designated as HESS J1837-069, has also been detected by the Japanese Suzaku satellite X-ray observatory, and is suspected to be what is called a "pulsar wind nebula". A similar object, HESS J1614-518, which is the brightest extended TeV gamma-ray source discovered in the H. E. S. S. galactic plane survey, has also been observed as a weak X-ray source by Suzaku.

• Mysterious Cosmic Powerhouses Explored
• Discovery of Extended X-Ray emission from the unidentified TeV source HESS J1614-518 using the Suzaku Satellite
• The INTEGRAL - HESS/MAGIC connection: a new class of cosmic high energy accelerators from keV to TeV

X-rays from rotating radio transients

Compact objects first known only by periodic short bursts of radio-frequency photons have been suspected to be rotating neutron stars and are called "rotating radio transients". Periodic X-ray bursts occurring much more frequently from one such object (J1819-1458) have been detected by the XMM-Newton satellite X-ray observatory, and they support the identification of the object as a neutron star.

• XMM-Newton Detects Pulsed Heartbeat Of A Weird New Type Of Star
• Pulsed Heartbeat Star
• Discovery of Pulsations and a Possible Spectral Feature in the X-ray Emission from Rotating Radio Transient J1819-1458

Star formation

Yet another illustration of the value of observing astronomical objects in diverse portions of the spectrum comes from studies of a protostar known as HH-211. Radio-frequency observations show jets of matter emerging from the poles of the rotating protostar, while infrared observations show emissions from shocked molecular hydrogen in a region of gas surrounding the jets. The observations support the hypothesis that the jets carry off angular momentum, allowing gradual growth of the protostar.

• Jets Are a Real Drag
• Jets Spiral in 'Reverse Whirlpool' from Star
• Submillimeter arcsecond-resolution mapping of the highly collimated protostellar jet HH 211

Extrasolar planets

The existence of most extrasolar planets detected so far has been deduced indirectly from perturbations in the movement of its parent star. But extrasolar planet HD 189733b has proven to be one of the most amenable extrasolar planets to direct observation. (For example, here.) Now it has actually been observed by reflected light from the stellar parent.

• Polarization technique focuses limelight
• Studying Planets With Sunglasses
• First Reflected Light from an Exoplanet?

Nanoparticle medicine

In the last year or so there has been quite a flood of reports of the use of nanoparticles as medical diagnostic tools or mechanisms for combating cancer and infectious diseases by heating or delivery of drugs. The past week has brought two more examples, involving gold nanoparticles. In one example the nanoparticles bind specifically to tumor cells, where they can be observed using laser illumination. In a second example the nanoparticles bind to the parasite responsible for toxoplasmosis. The parasite is destroyed when the nanoparticles are heated using suitable illumination from a laser.

• Gold Nanoparticle Probes May Allow Earlier Cancer Detection
• 'Golden Bullet' Shows Promise For Killing Common Parasite

Physical sciences news, 12/17/07-12/23/07

Gamma-ray bursts

There are several types of gamma-ray events that go under the name of "gamma-ray bursts", but the two main categories are "long" and "short" – referring to the duration of the burst. Long bursts have been generally attributed to very energetic supernovae that direct most of their energy into a narrow beam, which just happens to be visible from Earth. But most powerful supernovae are due to the collapse of a very large, young star – normally found only inside galaxies. So the detection of a long gamma-ray burst outside of any visible galaxy is rather a surprise. On the other hand, short gamma-ray bursts have been suspected to result from the merger of black holes and/or neurton stars. So another surprise is that the LIGO gravitational wave detector did not register any such event in connection with a recent short gamma-ray burst event.

• Intergalactic 'Shot In The Dark' Shocks Astronomers
• Cosmic explosion detonates in empty space
• A Gamma-Ray Burst Out of Nowhere
• Baffling Cosmic Explosion Comes Out of Nowhere
• Cosmic explosion is shot in the dark
• LIGO Sheds Light on Cosmic Event

Supernova remnants

It has generally been supposed that most elements heavier than hydrogen and helium that are not still locked up inside stars were formed in very massive stars that became supernovae and scattered most of their material into space. But actual traces of such "dust" in the vicinity of known supernova remnants have not been confirmed – until now.

• 10,000 Earths' Worth Of Fresh Dust Found Near Star Explosion
• Litterbugs of the Universe Busted
• Freshly Formed Dust in the Cassiopeia A Supernova Remnant as Revealed by the Spitzer Space Telescope

Very early star formation

Given that interstellar dust contained within galaxies is the result of supernovae explosions of previous generations of massive stars (see above), it is surprising that a galaxy seen as it was only 1.5 billions years after the big bang exhibits a very high rate of star formation (1000 times what now occurs in the Milky Way), and in a very dusty environment besides. But that's exactly what the galaxy GOODS 850-5 seems to show.

• New View of Distant Galaxy Reveals Furious Star Formation
• Galaxy Has 1,000 Times Our Rate of Star Formation
• GOODS 850-5 -- A z>4 Galaxy Discovered in the Submillimeter?

Cosmic inflation

Although the cosmic microwave background (CMB) represents an image of the universe at about 380,000 years after the big bang, some very subtle details of the variation in temperature of the CMB from point to point contain information about the very earliest instants of the universe. (Like time t=10^-35 sec, to be more precise.) It has been expected that a very careful analysis of the data will tell us something about the hypothesized phenomenon of cosmic inflation. The latest analysis claims to rule out the simplest model of inflation. However, it may be that the data obtained in the WMAP mission is insufficiently detailed for a satisfactory resolution of this issue, and we'll have to wait for a more sensitive measurement from the forthcoming Planck mission.

• No Dice for Slow Roll?
• Detection of primordial non-Gaussianity (fNL) in the WMAP 3-year data at above 99.5% confidence
• Detection of primordial non-Gaussianity (fNL) in the WMAP 3-year data at above 99.5% confidence

Mars

Data gathered from many years of surveillance of Mars by satellite missions and landers provides strong indications that Mars was warm and wet early in its history. Yet evidence of the most likely greenhouse gas, CO₂, that could have sustained a warm, wet environment has been conspicuously absent. The evidence now points to a different greenhouse gas, SO₂, instead. But early history aside, it now looks as though Mars could have an active (water ice) glacier at the present time.

• Sulfur dioxide may have helped maintain a warm early Mars
• Fire and Brimstone Helped Form Mars Oceans
• Possible solution to Mars enigma
• Red Planet Still Packs Surprises
• Red Planet Appears to Host Active Glacier

Extrasolar planets

How much technology would be required to learn something about the surface conditions (e. g. continents, oceans, clouds) on extrasolar planets in our neighborhood? New calculations based on plausible strategies for observing such features suggest... not a whole lot more technology than we will soon have. So if there are any civilizations at least as advanced as our own on any of those planets, they probably already have a fair idea of what Earth is like.

• Alien astronomers could discern Earth's features
• To curious aliens, Earth would stand out as living planet
• MIT Asks: How Would Extraterrestrial Astronomers Study Earth?

Sea level rise

A rise in sea levels is one of the most troublesome effects expected from global warming over the next several hundred years, but it has been difficult to make a good estimate of how quickly this would happen. However, about 124,000 years ago the planet was on average about 2° C warmer than it is now – and what it may be in just 100 years. New research claims to show that sea levels then were rising at a rate of 1.5 meters per century – about twice the current "consensus" forecast for our own times.

• Study suggests future sea-level rises may be even higher than predicted
• Rising seas 'to beat predictions'
• Lessons From an Interglacial Past
• Fast-Rising Sea Levels: An Interview on Research in the Red Seas

Physical sciences news, 12/10/07-12/16/07

Milky Way

Stars occupying regions above and below the disk of a spiral galaxy like the Milky Way are said to be in the galaxy's halo. In our own galaxy it turns out that there are two distinct halo regions, and they are rotating in opposite directions.

• Milky Way's two stellar halos have opposing spins
• Discovery shows Milky Way halo is split in two
• Huge Newfound Part of Milky Way Rotates Backward

Extrasolar planets

Some other solar systems besides ours undoubtedly have rocky planets like Mercury which always show the same face to the host star. A computer simulation shows that there could be a narrow potentially habitable region between the light and dark sides of such a planet.

• 'Twilight zones' on scorched planets could support life

Gliese 581d

Gliese 581d is a rocky planet recently discovered in orbit around the red dwarf star Gliese 581. It has about 8 times the mass of Earth. Two teams have now done simulations of the atmosphere of Gliese 581d and concluded that an atmosphere could exist and have properties considered necessary for Earthlike life to develop.

• Gliese 581: one planet might indeed be habitable
• Gliese 581d: A Habitable World After All?
• Is Gliese 581 Habitable?
• More Evidence that Gliese 581 Has Planets in the Habitable Zone

Haze on HD 189733b

HD 189733b is a gas giant extrasolar planet of the yellow dwarf star HD 189733 A. Although previous observations had suggested the presence of water vapor in the atmosphere, the latest set observations using the Hubble Space Telescope did not find evidence of water, sodium, or potassium in the atmosphere. However, there was an indication that the atmosphere did contain a haze of dust particles of unknown composition about 1 micron in size.

• Hazy red sunset on extrasolar planet
• Dust in a Hot Jupiter's Atmosphere
• First Sunset Outside Our Solar System Glimpsed
• A Red Haze on Distant Exoplanet
• HD 189733b: A 'Murky' Extrasolar Planet

Silica and the possibility of life on Mars

One of NASA's Mars rovers has found what appears to be a a deposit consisting largely of silica (SiO₂) – very fine grained beach sand, essentially. On Earth such deposits are found only in certain hot springs or volcanic fumaroles. Here both such environments support a great deal of microbial life. If life ever existed on Mars, it would likewise probably have thrived in such an environment.

• Clues to a Steamy Martian Past
• Mars Rover Investigates Signs of Steamy Martian Past
• Mars robot unearths microbe clue
• Mars Rover Finding Suggests Once Habitable Environment
• Mars rover finds signs of microbial life
• Spirit's Big Discovery

Organic compounds on Martian meteorite ALH 84001

ALH 84001 is a meteorite whose composition indicates it crystallized from molten rock 4.5 billion years ago on Mars. Over 10 years ago a team of NASA scientists hypothesized that some very small (20-100 nm) structures in the meteorite might be traces of life, but the claim was quite controversial and is no longer widely accepted. However, a recent comparison of the meteorite with terrestrial rocks suggests that simple organic compounds found in ALH 84001 could have formed, as in their terrestrial counterparts, in a chemical process catalyzed by magnetite (Fe₃O₄).

• Building blocks of life formed on Mars
• Building Blocks of Life Formed on Early Mars?
• Life's Building Blocks Found in Mars Rock
• Allan Hills 84001 Analysis Confirms Building Blocks Of Life Also Formed On Mars
• Building Blocks of Life Can Form on Cold, Rocky Planets — Anywhere

Saturn's rings

When Saturn's rings were first examined close-up by the Voyager missions in the 1970s, it was concluded that they had formed relatively recently (like 100 million years ago) when a moon of Saturn was destroyed in a collision with another moon or an asteroid. But the latest evidence from the Cassini mission indicates that Saturn may have had similar rings since the formation of the solar system 4.5 billion years ago. However, it appears that material in the rings is continually accreting into new moonlets, only to be destroyed again in later collisions.

• Saturn's Rings May Be As Old As Solar System
• Saturn's rings 'may live forever'
• Saturn's Rings Older Than First Thought?
• Saturn's Rings Could Be as Old as the Solar System
• Saturn’s Rings More Ancient than First Thought
• Saturn's Rings: Moon Remnants Or As Old As The Solar System?

Greenhouse gases

A new study indicates that human destruction of peat bogs may be responsible for emission of amounts of CO₂ possibly 10% as much as all burning of fossil fuels. Another study proposes a new model, taking into account the role of nitrogen, of how carbon is recycled among plants, soils, and the atmosphere.

• Peatland destruction is releasing vast amounts of CO₂
• New model revises estimates of terrestrial carbon dioxide uptake

Arctic ice

Some scientists who have studied the melting of Arctic ice now believe the ice could melt entirely in summer as soon as 2013, instead of 2040 as previously thought. Even this summer the melting has resulted in sea surface temperatures, in some places, 5° C above average – a level never before recorded. And this summer's melt of the Greenland ice sheet was 10% more than the previous record from 2005.

• 'The Arctic is screaming' — summer sea ice could be gone in five years
• Arctic summers ice-free 'by 2013'
• Without its insulating ice cap, Arctic surface waters warm to as much as 5 C above average
• Greenland melt accelerating, according to CU-Boulder study

Near-record high temperatures

And overall, 2007 figures to be Earth's second-warmest year on record, while the past 10 years have been the warmest decade ever recorded.

• 2007 Brought Near-Record Heat
• 2007 data confirms warming trend
• 1998-2007 warmest decade, UN agency says at climate meet

Physical sciences news, 12/3/07-12/9/07

Active galaxies

Jets of high-energy particles are produced by a variety of astronomical objects. The largest example of this phenomenon has been discovered in the active galaxy CGCG 049-033.

• Intergalactic particle beam is longest yet found

Galaxies in the early universe

The earliest stars in the universe consisted entirely of primordial hydrogen and helium, since heavier elements were formed almost entirely by the demise of these first stars in supernova events. Planets (which are generally considered a necessity for the development of life in any form similar to what we know) require elements heavier than hydrogen and helium. New simulations suggest that the earliest stars, having masses of perhaps 100 Suns, may have formed earlier than previously supposed, meaning that planets (and life) could also have formed earlier.

• Earliest galaxies had building blocks of life

Dark matter stars

Many observations indicate that dark matter in the universe is about 5 times as plentiful (by mass) as "ordinary" baryonic matter. Consequently, the first compact objects to form in the universe may have consisted mostly of dark matter. Although ordinary matter would have been mixed in, the dark matter could have prevented, for a time, ordinary matter from collapsing to a density sufficient to form stars powered by thermonuclear reactions.

• ‘Dark stars’ may have populated early universe
• Drowning in Dark Matter?
• Universe's first stars may have been dark
• First Stars Were Huge and Dark
• Dark matter in newborn universe doused earliest stars

Dark matter in galaxies

Computer simulations of the early universe, until now, have predicted larger amounts of dark matter in the central parts of galaxies than is actually observed. Refined simulations that take into account the supernova explosions of the first generation of stars now indicate that gravitational effects of the supernovae could have driven much of the original dark matter out of the central regions of galaxies.

• Galaxies Are Born Of Violence Between Dark Matter and Interstellar Gas
• Invisible Matter Loses Cosmic Battle

Gas giant planets

Most extrasolar planets that have been detected so far are gas giants located very close to the central star – because this is the configuration most likely to be detected by current technology. Some of these planets are so close to their star that it has been difficult to understand how they have escaped being completely evaporated by the heat. New simulations indicate that positively charged hydrogen ions containing three protons are capable of radiating away enough heat to allow gas giant planets in close proximity to their stars.

• Planets can survive extreme roasting by their stars
• How to Destroy a Giant Planet

Cosmic textures

Phase transitions, such as occur in the freezing of ice and other solids, should also have occurred very early around the hypothesized time of inflation in big bang models of the universe. Such transitions may have led to inhomogeneities called "topological defects", which in principle could lead to observable inhomogeneities in the cosmic microwave background. Theoretical calculations now indicate that particular types of defects called "textures" may account for puzzling features actually observed in the microwave background.

• Possible Cosmic Defect, Remnant From Big Bang, Discovered
• A Texture in the Sky?
• A Cosmic Microwave Background Feature Consistent with a Cosmic Texture

White dwarfs in globular clusters

Astronomers have been surprised to find that white dwarf stars are unexpectedly scarce in the central regions of some globular clusters. It is hypothesized that the explanation for this may lie in asymmetrical flows of gas out of stars in their red giant phase, just before the star collapses to a white dwarf.

• Sun-like stars get a kick out of death
• Dead Stars Propelled Like Rockets

The solar corona

Observations that have been deduced from data collected by the Japanese Hinode mission may have solved a long-standing mystery of why the Sun's corona is so hot – several million degrees K – even though the solar surface is only about 6000° K. The cause appears to be strong magnetic turbulence in the corona, called "Alfvén waves".

• Mission illuminates solar mysteries
• Roiling magnetic waves explain solar enigma
• Unlocking the riddle of Sun's heat
• Results from Hinode: Sunrise on Coronal Heating
• Are There Alfvén Waves in the Solar Atmosphere?

Slushball Earth

It now appears possible that the Earth's oceans never entirely froze solid, as hypothesized in the "snowball Earth" scenario. Carbon dioxide dissolved in the oceans, coming from carbonate minerals on the ocean floor, may be responsible for a milder freeze that produced only a "slushball".

• Did Carbon Save Earth From a Deep Freeze?
• 'Snowball Earth' was more a slushball

Interruption of the Gulf Stream

About 8200 years ago a huge (100,000 km³, seven times the volume of the present Great Lakes combined) North American glacial lake known as Lake Agassiz had swelled so large that it burst out and mostly flooded into the Atlantic Ocean. There is now evidence that all this cold, dense fresh water was sufficient to disrupt the flow of the Gulf Stream and cause a temporary but severe cooling of the climate.

• Ancient flood brought Gulf Stream to a halt
• Epic Flood Triggered Ancient "Big Chill," Study Says

Spintronics

Scientists have generated, modulated and electrically detected a pure spin current in silicon. This could be a key step in the development of silicon-based "spintronic" devices, which might be used to make denser information-processing devices than can be implemented using present technology based on currenjts of electric charge.

• Scientists generate, modulate, and electrically detect pure spin currents in silicon

Trying some new things

As you may have noticed, new editions of Philosophia Naturalis have not been coming out on a very regular schedule of late.

There are two reasons for this. Firstly, we are getting few volunteers to host this carnival. Hosting is not really that difficult or time-consuming to do, and I could do it myself once a month (say).

But secondly, we are getting too few submissions of suitable blog posts on topics in the physical sciences to include in the carnival. This is a much more serious problem, since without such submissions, there is nothing to include in the carnival (duh). Again, the editor could go out and round up material, but that puts all the burden on one person.

However, I'm not going to give up easily. I have a few ideas of how to encourage more participation. To begin with, you will see another post today entitled "Physical sciences news". This is a list I've put together of what I consider to be the most interesting news in the physical sciences that's come out in (roughly) the past week.

The first post of this kind is heavily weighted towards astronomy and astrophysics. In my experience, this is simply where most of the "action" in the physical sciences is these days, so I would expect this weighting to continue. However, if you happen to know of important news in other areas, such as physics, chemistry, geosciences, or mathematics, by all means feel free to let me know about it. (You'll find the email address here.)

I'll try to do this every weekend. I see two purposes of this. First, it should be a useful resource for anyone interested in the physical sciences who wants to easily keep aware of "significant" news that a non-specialist can appreciate. This in turn will increase traffic here, leading to more blog traffic for you, if you host an edition of the carnival or have an article of yours included in the carnival.

The second purpose is to suggest topics for you to write about on your blog, which articles you can in turn submit to the carnival. As you can see from the news post, there's more than enough happening in just a single week to make up an entire carnival edition. You need not confine yourself to this news, of course. Or if it suggests a topic, you need not write only about the specific news development. You could, for instance, write a review-type article that treats the topic more generally, placing the news in a broader context.

I have other ideas that may be tried, but this seems to me like a good place to start. If enough people are motivated to write and submit articles inspired by something mentioned in the news, perhaps we can evolve this carnival into something more like a useful news service for the community of people who have a serious interest in the physical sciences.

Physical sciences news, 11/26/07-12/2/07

Climate change

To the surprise of practically nobody except climate change denialists, levels of CO₂ in the atmosphere continued to increase in 2006 to new record levels. And Scientific American comes up with a nice suite of several articles (two listed here), which key off the recent report of the U.N. Intergovernmental Panel on Climate Change.

• U.N.: Greenhouse Gases Hit High in 2006
• Beyond the Worst Case Climate Change Scenario
• 10 Solutions for Climate Change

Venus

Some results are in from the European Space Agency's Venus Express mission, and they paint a picture of Venus as not such a great place for your next summer vacation. Much of the crappy climate is due to a CO₂-induced greenhouse effect. Uh, oh.

• How Earth's twin became so hellishly hot
• NASA Scientist Confirms Light Show on Venus
• Probe likens young Venus to Earth
• Twin Planets Earth and Venus Were "Separated at Birth"
• Signs of Lightning on Venus
• Venus offers Earth climate clues
• Did life once thrive on Evil Twin Venus?

The Milky Way and its neighborhood

Two things here about our galactic neighborhood. We might have another neighbor galaxy that has never actually been seen yet, even though it's almost as close and as large as the Andromeda galaxy. And there's a cluster of very young stars – only 100 light-years from our galactic center – that's moving way too fast.

• Milky Way galaxy may have hidden twin
• Dynamical Constraints on the Local Group from the CMB and 2MRS Dipoles
• Star cluster's extreme speed puzzles astronomers
• The proper motion of the Arches cluster with Keck Laser-Guide Star Adaptive Optics

Early galaxies

Astronomers using Europe's new Very Large Telescope, located in Chile, have observed 27 young "proto-galaxies" as they appeared about 2.5 billion years after the big bang. This provides evidence that larger galaxies like our own may have formed by the amalgamation of a number of such proto-galaxies.

• Faint galaxies spotted in the early universe
• Proto-galaxies tip cold dark matter
• A Long, Hard Look at the Early Universe
• Discovering Teenage Galaxies
• Sighting of 'teenage' galaxies gives scientists
stellar return
• New population of faint protogalaxies discovered
• A Population of Faint Extended Line Emitters and the Host Galaxies of Optically Thick QSO Absorption Systems

Formation of planetary systems

Astronomers think they have found the two youngest solar systems ever detected, about 450 light-years from Earth. Elsewhere, one bright, massive young star in the Trapezium of the Orion Nebula is pumping out hot gas at a temperature of about 2 million degrees C, and this probably affects the formation of planetary systems around other nearby young stars.

• Planet Formation is Child's Play
• Of Young Stars and Ancient Planets
• Huge Stars Seen as Source of Glowing Gas
• Million-Degree Plasma Pervading the Extended Orion Nebula

Preon nuggets

Preons are hypothetical particles that have been proposed to make up quarks. Although there is as yet no experimental evidence for preons, if they ever existed in the universe soon after the big bang, a few preon clumps might still survive as objects a few centimeters in size but with as much mass as the Moon.

• Nuggets of New Physics
• The observational legacy of preon stars - probing new physics beyond the LHC

Quasistars

Large clumps of hydrogen and helium in the early universe may have condensed into star-like objects initially 1000 times as massive as the Sun. Although the core would collapse into a black hole, the resulting "quasistar" might be massive enough to avoid destruction, and continue to accrete matter, evolving into a supermassive black hole such as seems to exist in the center of most galaxies.

• Biggest black holes may grow inside 'quasistars'
• Quasistars: Accreting black holes inside massive envelopes

Philosophia Naturalis #15 has been published

Sam Wise at Sorting Out Science has put together a great collection of posts. It's a wonderful look at a number of different viewpoints on a lot of recent news in the physical sciences. Thanks, Sam.

Philosophia Naturalis #14 has been published

It's now up at Dynamics of Cats, and what a herd it is.

Thanks, Steinn.

Philosophia Naturalis #14 is coming

After a slightly extended hiatus it will be back on Thursday, October 4 – a date to remember – at the Dynamics of Cats.

Although time is short, if you have a blog post you especially like that relates to the physical sciences or technology, submit it for the carnival – you won't want to miss this special day.

Besides that, it would be nice to see a little more interest in this carnival, so it will be worthwhile to continue. And if you have a blog that deals with some aspect of physical science or technology, please consider volunteering to host the carnival, so we can keep the ball rolling.

Philosophia Naturalis #13 has been published

And it's another great one – at Cocktail Party Physics. Thanks, Jennifer.

Philosophia Naturalis #12 has been published

And as previously announced, it's at a geocentric view. (And it even appeared on time this month, unlike this notice.) Definitely worth your time to read a bit.

Thanks to mollishka for doing and hosting this month's edition.

Philosophia Naturalis #12 call for submissions

Mollishka at a geocentric view will be hosting the next edition of the carnival on Thursday, July 19. The announcement is here.

Submissions should be made by Tuesday night, July 17. An email address for submissions is in the announcement, or you can use this handy form. The editor's area of expertise is astronomy, so I'm sure submissions in that area will be welcome, but so will those in other traditional physical sciences (physics, math, earth science, chemistry, etc.)

Let's make this another great collection of physical science writing.

Philosophia Naturalis #11 has been published

And it may be the best one yet. If you blog about the physical sciences and you haven't submitted some of your writing for Philosophia Naturalis... well, what's holding you back? You could be in some pretty fine company.

Anyhow, for the latest edition, you'll find it here at Highly Allochthonous, courtesy of Chris Rowan. The layout and presentation is especially clever. Great job, Chris!

Philosophia Naturalis #11 delayed a week

By mutual agreement of the carnival manager (me) and the editor of the 11^th edition of the carnival (Chris Rowan at Highly Allocthonous) the appearance of the next edition will be delayed a week, until Thursday, June 28. You can read Chris' comments here.

We both regret the delay, but expect the result will be much better. And just think – now you have (almost) another whole week to suggest that great physical science blog article you were meaning to submit all along...

Philosophia Naturalis #10 has been published

By Stuart Coleman at Daily Irreverence. It's full of quantum goodness and other delights. Thanks, Stuart!

And if that whets your appetite for more, be prepared to come back in four weeks for the next edition, which will be hosted June 21 by Chris Rowan at Highly Allochthonous.

Philosophia Naturalis #10 is coming May 24

And it will be at Daily Irreverence, courtesy of Stuart Coleman. Check out the details here.

And please send in your suggestions for good blog articles in the physical sciences. (See the announcement for instructions, or look here.)

Philosophia Naturalis #9 has been published

Whew, finally. News about your next vacation destination (a few centuries in the future) and quantum mechanics too. Go have a look.

Philosophia Naturalis #8 is (finally) up

And you can find it right here.

We apologize for the delay, but there's some really, really good stuff in this edition. Thanks, Sujit.

Philosophia Naturalis #8 call for submissions

Philosophia Naturalis #8 will be hosted at Sujit Datta's blog metadatta on Thursday, March 29.

If you've recently written or read a noteworthy blog article on physics, math, astrophysics, chemistry, Earth science, advanced technology, or any other physical science topic, read the call for submissions for details of how to submit it for inclusion in the carnival.

Sujit needs the submissions a little early – by March 23 – so don't delay. Send something in now.

Posterity will thank you.

Philosophia Naturalis #7 - tabloid journalism at its best!

The truly amazing and astounding thing about this edition of Philosophia Naturalis is that it does not contain anything about flying saucers and space aliens!

How could such a government scandal have been hidden so long? But now the truth is finally coming out: UFO science key to halting climate change: former Canadian defense minister

A former Canadian defense minister is demanding governments worldwide disclose and use secret alien technologies obtained in alleged UFO crashes to stem climate change, a local paper said Wednesday.

But wait! There's even more tabloid goodness to this story. You see, it must be Bill Clinton's fault! In fact, Limbaugh says this is all a Liberal scam! Just like global warming itself!

Whatever. After you've digested that little bit of news, head on over to Lorne's place at Geek Counterpoint to read other incredible facts!

Philosophia Naturalis #7 is coming up soon

It will be up Thursday, March 1, to be more precise, at Geek Counterpoint. But you don't have a lot of time to get your suggestions in – they need to be in to the editor by Monday, February 26. You can send them to the editor as described here, or email them to carnival AT scienceandreason.net.

Do it now. You'll be glad you did.

Philosophia Naturalis #6 has been published

Charles Daney at Science and Reason has posted the 6^th edition of Philosophia Naturalis. It's really fair-to-middling good this month.

Announcement of Philosophia Naturalis #6

Philosophia Naturalis #6 will be published on Thursday, February 1 by Charles Daney at Science and Reason.

Don't miss this literally once-in-a-lifetime opportunity to have your favorite article included in Philosophia Naturalis #6. Remember, Philosophia Naturalis is the blogosphere's best blog carnival covering all of physical science and technology.

More information on suggesting articles is here.

Philosophia Naturalis #5 has been published

Chris Rowan at Highly Allocthonous has posted the 5^th edition of Philosophia Naturalis. It's in the form of a great essay about the functions of science blogging. Don't miss it!

Hosting Philosophia Naturalis

We're looking for a few good bloggers to host future editions of the carnival. It's not a lot of work (a little, but not that much), it is fun, and it draws attention to the hard work you do for your own blog.

There are just a few guidelines:

• Your blog should have some focus on the natural sciences and/or technology, even if mixed in with other things. This will be interpreted liberally, but you know what we mean. Please respect our readers and be candid about your purpose in hosting an edition of the carnival.
  
• To volunteer for hosting, just get in touch with the carnival organizer. (See contact information in the organizer's profile.) If your offer is accepted, the organizer will schedule you for the next available date, or some later date if necessary.
  
• Within two to four weeks before the date you are scheduled to host the carnival, place a call for submission of article recommendations on your blog. Mainly this should state the deadline for submissions and an email address to which submissions should be sent. Also include a link to this blog so that readers can see what the carnival is about and read past editions. Be sure that you let the carnival organizer know when you do this, and a note of the call for submissions will be posted here.
  
• It's not necessary to be elaborate and creative in composing your edition of the carnival. Although creativity will make your effort more memorable, it's enough to name the author of each article and briefly describe what it's about. Read some of the past editions of the carnival to see what other editors have done.
  
• If you want to select high-quality articles for inclusion on your own, by all means do so, especially if you haven't received many recommendations by a week before the edition is due to be published. The carnival organizer will be happy to help out if you ask for assistance.
  
• After the edition has been published, send a brief email to authors of included articles, to thank them, to announce the carnival, and to allow authors to make a mention of it on their own blogs, if they wish. It's not a bad idea, either, to acknowledge contributions when you receive them, if you have time. The carnival organizer will help publicizing your edition if you have other specific suggestions.
  
• Have fun.
  
  

Announcement of Philosophia Naturalis #5

Philosophia Naturalis #5 will be published on Thursday, January 4 by Chris Rowan at Highly Allochthonous. Preliminary information is here.

You can suggest an article for the carnival at any time before January 4 – even right now.

Philosophia Naturalis #4 has been published

Daniel Collins at Down to Earth has posted the 4^th edition of Philosophia Naturalis. It's your gateway to interesting science reading, right here.

Announcement of Philosophia Naturalis #4

Philosophia Naturalis #4 will be published on Thursday, December 7 by Daniel Collins at Down to Earth. The full details are here.

You can suggest an article for the carnival at any time before December 7 – even right now. Don't delay – you know how hectic things can get at that time of year.

Philosophia Naturalis #3 has been published

And you can find it right now, at geek counterpoint. Don't miss it – it's really good.

Thanks, Lorne, for a fine job.

Announcement of Philosophia Naturalis #3

Philosophia Naturalis #3 will be published on Thursday, November 9 at Geek Counterpoint. The full details are here.

You can suggest an article for the carnival at any time before November 9 -- even right now. Do it now, and avoid the rush at the last minute.

Philosophia Naturalis #2 is published

The second edition of Philosophia Naturalis is now up at Nonoscience. Happy reading!

And thanks to Arunn for putting it all together.

Announcement of Philosophia Naturalis #2

Philosophia Naturalis #2 will be published on Thursday, October 12 at Nonoscience -- check there for any further information.

Make it easy on yourself -- don't put off sending your suggestions till the last minute. Submitting an article to the carnival takes very little time (assuming it's already written!) So do it now, and then you won't have to keep thinking about it.

How to suggest an article for Philosophia Naturalis

You may suggest either an article you have written, or an article that you consider especially worthwhile written by someone else. Articles should be publicly accessible -- i. e., not available only by paid subscription.

The content of the article should be reasonably related to science in general or to the physical sciences -- such as physics, mathematics, astronomy, cosmology, computer science, chemistry, or Earth science -- or to advanced technology -- such as nanotechnology, robotics, artificial intelligence, alternative energy, or quantum computing.

The level of expertise assumed by the article you recommend may range from beginner to advanced. But in the latter case, the article should have at least something of value for non-experts.

Please do not "spam" the carnival by suggesting articles whose main purpose is to promote a commercial product or service.

In your suggestion, don't forget to include the URL, and add a brief comment about the article.

Suggestions may be sent by email to the address: carnival@scienceandreason.net. Please put "Philosophia Naturalis" somewhere in the subject line. You may also send the information using the form at Blog Carnival. Editors of particular editions may also provide an alternate email address for submissions, which will be noted in the announcement of the forthcoming edition.

For more information about Philosophia Naturalis, including the publishing schedule, see our profile at Blog Carnival.

Philosophia Naturalis #1 published

The first edition of Philosophia Naturalis was published on September 14, 2006 at Science and Reason.

About Philosophia Naturalis

In this edition of the Tangled Bank I raised the issue of a blog carnival focused on the physical sciences and technology. Since the response was encouraging, I have started such a carnival. It has been named Philosophia Naturalis, and the first edition has already been published here.

The name is Latin for Natural Philosophy, which Wikipedia describes as "a term applied to the objective study of nature and the physical universe that was regnant before the development of modern science." The name is also a reference to Isaac Newton's 1687 Philosophiae Naturalis Principia Mathematica (although Newton didn't originate the term).

Just as the Tangled Bank focuses its attention on the life sciences and medicine, Philosophia Naturalis will take the physical sciences and technology as its focus. That doesn't mean just "physics". The physical sciences include physics, astronomy, cosmology, chemistry, mathematics, computer science, and Earth sciences. And just as medicine is applied life science, technology is applied physical science, including such topics as nanotechnology, robotics, artificial intelligence, alternative energy, and quantum computing.

The blog named Philosophia Naturalis is the "home page" for the carnival. Here you will find announcements (such as what you're reading now) related to the carnival, notification of upcoming publication dates, announcements of the publication of new editions when they occur, messages about carnival policies and procedures, and any other messages pertinent to the carnival.

The actual editions of the carnival will be hosted at other sites -- generally a site belonging to the editor of each edition. The locations will be identified in announcements here. Since these announcements will be archived here, you can always locate older editions (unless the host site deletes the edition or completely disappears -- which we hope seldom happens!)

If you want to keep informed about what's going on with the carnival, and especially about when new editions are published, all you have to do is add the RSS feed for this blog to your favorite feed reader/aggregator.

Why another carnival? Surprisingly, there seem to be no carnivals out there now having this focus. There needs to be a way for people interested in any of the physical sciences and advanced technology to easily read new articles in these fields -- articles that have been judged to be especially noteworthy. There also needs to be a way for people who write about these topics to bring their work to the attention of a wider audience.

You can become involved in this project right now. It needs you to submit suggestions for articles to be included. This may be your own writing. However, since only links and brief quotations will be published in editions of the carnival, anyone other than the copyright owner can also send in suggestions of especially good articles they've found.

We're looking for the best articles published on the Web within the past few months that fall within the topic focus. Articles may range from introductory tutorials for a wide audience to more specialized pieces that still may be interesting to educated people with an active curiosity. These need not be blog articles. They could also be any good, short science writing that first appeared in a print publication and has been posted on the Web by its copyright holder for general access.

To submit an article, all you have to do is send a short email message to carnival@scienceandreason.net, with a link to the article and a few words why you're recommending it. Please put "Philosophia Naturalis" somewhere in the subject line.

Of course, we also need volunteer editors. If you have a blog which deals with the physical sciences and technology, even a little bit, you are eligible to edit and host a future edition of the carnival. Simply send your request to the same email address noted above. Editing is actually a lot of fun, and not all that much work -- and your blog will benefit from a great deal of attention and traffic when your edition appears.

Tags: blog carnival, Philosophia Naturalis