Astronomy Without A Telescope – SETI 2.0

Allen Telescope Array. Credit: SETI Institute

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Fifty years of eerie silence in the search for extra-terrestrial intelligence has prompted some rethinking about what we should be looking for.

After all, it’s unlikely that many civilizations would invest a lot of time and resources into broadcasting a Yoo-hoo, over here signal, so maybe we have to look for incidental signs of alien activity – anything from atmospheric pollution on an exoplanet to signs of stellar engineering undertaken by an alien civilization working to keep their aging star from turning into a red giant.

We know a spectroscopic analysis of Earth’s atmosphere will indicate free molecular oxygen – a tell tale sign of life. The presence of chlorofluorocarbons would also be highly suggestive of advanced industrial activity. We also know that atomic bomb tests in the fifties produced perturbations to the Van Allen belts that probably persisted for weeks after each blast.

These are planet level signs of a civilization still below the level of a Kardashev Type 1 civilization. We are at level 0.73 apparently. A civilization that has reached the Type 1 level is capable of harnessing all the power available upon a single planet – and might be one that inadvertently signals its presence after thoughtfully disposing of large quantities of nuclear waste in its star. To find them, we should be scanning A and F type stars for spectral signatures of technetium – or perhaps an overabundance of praseodymium and neodymium.

We might also look for signs of stellar engineering indicative of a civilization approaching the Kardashev Type 2 level, which is a civilization able to harness all the power of a star. Here, we might find an alien civilization in the process of star lifting, where an artificial equatorial ring of electric current creates a magnetic field sufficient to both increase and deflect all the star’s stellar wind into two narrow polar jets.

Left image - A proposed model for 'star lifting'. An artificial equatorial ring of electric current (RC) produces a magnetic field which enhances and directs the star's stellar wind though magnetic nozzles (MN) to produce two polar jets (J). Right image (Credit: SETI institute) - Artists impression of the completed Allen Telescope Array for future SETI observations. The lead image for this article is part of the current Allen Array prototype, comprising 42 of the proposed 350 dishes.

These jets could be used for power generation, but might also represent a way to prolong the life of an aging star. Indeed, this may become a vital strategy for us to prolong the solar system’s habitable zone at Earth’s orbit. In less than a billion years, Earth’s oceans are expected to evaporate due to the Sun’s steadily increasing luminosity, but some carefully managed star lifting to modify the Sun’s mass could extend this time limit significantly.

It’s also likely that Type 2 civilizations will play with Hertzsprung–Russell (H-R) parameters to keep their Sun from evolving onto the red giant branch of the H-R diagram – or otherwise from going supernova. Some well placed and appropriately shielded nuclear bombs might be sufficient to stir up stellar material that would delay a star’s shift to core helium fusion – or otherwise to core collapse.

It’s been hypothesized that mysterious giant blue straggler stars, which have not gone supernova like most stars of their type would, may have been tinkered with in this manner (some stress on the word hypothesized there).

As for detecting Type 3 civilizations… tricky. It’s speculated that they might build Dyson nets around supermassive black holes to harvest energy at a galactic level. But indications are that they then just use all that energy to go around annoying the starship captains of Type I civilizations. So, maybe we need to draw a line about who exactly we want to find out there.

Further reading:

Starry Messages: Searching for Signatures of Interstellar Archaeology http://arxiv.org/abs/1001.5455

Detectability of Extraterrestrial Technological Activities http://www.coseti.org/lemarch1.htm

Weekend SkyWatcher’s Forecast – June 18-20, 2010

Greetings, fellow Stargazers! Have you been enjoying the rain? Then keep your eyes open for a “celestial shower” as meteoritic activity picks up over the next few nights, culminating in the peak of the Ophiuchid meteor Saturday night through Sunday morning. While you’re out relaxing, be sure to spare some time for lunacy and take a look some interesting features on the Moon. Need a test of your telescope’s resolving power? Then I “double dare” you to take on Gamma Virginis! Whenever you’re ready, I’ll see you in the back yard….

Friday, June 18, 2010 – Let’s begin the day by recognizing the 1799 birth on this date of William Lassell, telescope maker and discoverer of Triton (a moon of Neptune), and Ariel and Umbriel (satellites of Uranus). As often happens, great astronomers share birth dates, and this time it’s 187 years later for Allan Rex Sandage. A Bruce Medalist, Dr. Sandage is best known for his 1960 optical identification of a quasar, with his junior colleague, Thomas Matthews.

Our telescope lunar challenge tonight will be Hadley Rille. Find Mare Serenitatis and look for the break along its western shoreline that divides the Caucasus and Apennine mountain ranges. South of this break is the bright peak of Mons Hadley, which is of great interest for several reasons, so power up as much as possible.

Impressive Mons Hadley measures about 24 by 48 kilometers at its base and reaches up an incredible 4,572 meters. If volcanic activity had created it, Mons Hadley would be comparable to some of the very highest volcanically formed peaks on Earth, like Mount Shasta and Mount Rainer. South is the secondary peak, Mons Hadley Delta. It is home to the Apollo 15 landing site just a breath north of where it extends into the cove created by Palus Putredinus. Along this ridge line and smooth floor, look for a major fault line, winding its way across 120 kilometers of lunar surface; this is Hadley Rille. In places, the Rille spans 1,500 meters in width and drops to a depth of 300 meters below the surface. Believed to have been formed by volcanic activity 3.3 billion years ago, we can see the impact lower gravity has on this type of formation. Earthly lava channels are usually less than 10 kilometers long, and only around 100 meters wide. During the Apollo 15 mission, Hadley Rille was visited at a point where it was only 1.6 kilometers wide, still a considerable distance. Over a period of time, the Rille’s lava may have continued to flow through this area, yet it remains forever buried beneath years of regolith.

Saturday, June 19, 2010 – Tonight on the Moon we’ll be looking for another challenging feature and the craters that conjoin it—Stofler and Faraday. Located along the terminator to the south, crater Stofler was named for Dutch mathematician and astronomer Johan Stofler.

Consuming lunar landscape with an immense diameter of 126 kilometers, and dropping 2,760 meters below the surface, Stofler is a wonderland of small details in an eroded surrounding. Breaking its wall on the north is Fernelius, but sharing the southeastern boundary is Faraday. Named for English physicist and chemist Michael Faraday, this crater is more complex and deeper (4,090 meters) but far smaller in diameter (70 kilometers). Look for myriad smaller strikes that bind the two together!

When you’re done, let’s have a look at a delightful pair—Gamma Virginis (RA 12 41 41 Dec +01 26 54). Better knownas Porrima , this is one cool binary whose components are of almost equal spectral type and brightness. Discovered by Bradley and Pound in 1718, John Herschel was the first to predict this pair’s orbit in 1833, and stated that one day they would become inseparable to all but the very largest of telescopes—and he was right. In 1920 the A and B stars had reached their maximum separation, and during 2007 they were as close together as they ever can be. Observed as a single star in 1836 by William Herschel, its 171-year orbit puts Porrima in almost the same position now as it was when Sir William saw it!

Sunday, June 20, 2010 – In the predawn hours, we welcome the ‘‘shooting stars’’ as we pass through another portion of the Ophiuchid meteor stream. The radiant for this pass lies nearer Sagittarius, and the fall rate varies from 8 to 20 per hour, but the Ophiuchids can sometimes produce more than expected! Perhaps the sky acknowledges the 1966 passing of Georges Lemaitre on this date? Lemaitre researched cosmic rays and the three-body problem and in 1927 formulated the Big Bang theory using Einstein’s theories.

Are you ready to explore some more history? Then tonight have a look at the Moon and identify Alphonsus; it’s the centermost in a line of rings and looks much like the Theophilus, Cyrillus, and Catharina trio.


Alphonsus is a very old Class V crater, spans 118 kilometers in diameter, drops below the surface to about 2,730 meters, and contains a small central peak. Eugene Shoemaker had studied this partially flooded crater and found dark haloes on the floor. Again, this could be attributed to volcanism. Shoemaker believed they were maar volcanoes, and the haloes were dark ash. Power up and look closely at the central peak, for not only did Ranger 9 hard land just northeast, but this is the only area on the Moon where an astronomer has observed a change and backed up that observation with photographic proof.

On November 2, 1958, Nikolai Kozyrev long and arduous study of Alphonsus was about to be rewarded. Some two years earlier Dinsmore Alter had taken a series of photographs from the Mt. Wilson 60’’ reflector that showed hazy patches in this area that could not be accounted for. Night after night, Kozyrev continued to study at the Crimean Observatory, but with no success. During the process of guiding the scope for a spectrogram, the unbelievable happened—a cloud of gaseous molecules containing carbon had been captured! Selected as the last target for the Ranger series of photographic missions, Ranger 9 delivered 5,814 spectacular high-resolution images of this mysterious region before it crashed nearby. Capture it yourself tonight!

Until next time? Ask for the Moon… But keep on reaching for the stars!

This week’s awesome images are (in order of appearance): Dr. Alan Sandage courtesy of Dr. Sandage, Hadley Rille, courtesy of Wes Higgins, Stoffler and Faraday courtesy of Wes Higgins, Porrima – Palomar Observatory courtesy of Caltech, Georges Lemaitre and Albert Einstein (historical image), Ranger 9 Image of Alphonsus taken 3 minutes before impact courtesy of NASA, Alphonsus’ central peak taken 54 seconds before Ranger 9 impact courtesy of NASA. We thank you so much!

Astronomers Witness Star Birth

Astronomers caught a glimpse of a future star just as it is being born out of the surrounding gas and dust, in a star-forming region similar to the one pictured above. (Spitzer Space Telescope image of DR21 in Infrared) Credit: A. Marston (ESTEC/ESA) et al., JPL, Caltech, NASA

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Astronomers have glimpsed into the birth of a star, and have seen what could be the youngest known star at the very moment it is being born. “It’s very difficult to detect objects in this phase of star formation, because they are very short-lived and they emit very little light,” said Xuepeng Chen, from Yale University and lead author of a new paper. Not yet fully developed into a true star, the object is in the earliest stages of star formation and has just begun pulling in matter from a surrounding envelope of gas and dust. The team detected the faint light emitted by the nearby dust.

Using the Submillimeter Array in Hawaii and the Spitzer Space Telescope, the astronomers studied L1448-IRS2E, located in the Perseus star-forming region, about 800 light years away within our Milky Way galaxy.

Stars form out of large, cold, dense regions of gas and dust called molecular clouds, which exist throughout the galaxy. Astronomers think L1448-IRS2E is in between the prestellar phase, when a particularly dense region of a molecular cloud first begins to clump together, and the protostar phase, when gravity has pulled enough material together to form a dense, hot core out of the surrounding envelope.

Most protostars are between one to 10 times as luminous as the Sun, with large dust envelopes that glow at infrared wavelengths. Because L1448-IRS2E is less than one tenth as luminous as the Sun, the team believes the object is too dim to be considered a true protostar. Yet they also discovered that the object is ejecting streams of high-velocity gas from its center, confirming that some sort of preliminary mass has already formed and the object has developed beyond the prestellar phase. This kind of outflow is seen in protostars (as a result of the magnetic field surrounding the forming star), but has not been seen at such an early stage until now.

The team hopes to use the new Herchel space telescope, launched last May, to look for more of these objects caught between the earliest stages of star formation so they can better understand how stars grow and evolve. “Stars are defined by their mass, but we still don’t know at what stage of the formation process a star acquires most of its mass,” said Héctor Arce, also from Yale. “This is one of the big questions driving our work.”

Other authors of the paper include Qizhou Zhang and Tyler Bourke of the Harvard-Smithsonian Center for Astrophysics; and Ralf Launhardt, Markus Schmalzl and Thomas Henning of the Max Planck Institute for Astronomy.

The new study appears in the current issue of the Astrophysical Journal.

Read the team’s paper here.

Source: Yale University

Astronomy Cast Ep. 188: The Future of Astronomy

Artist impression of the OWL Telescope concept

We spent 5 episodes telling the story of astronomy so far, how we got from the work of the Babylonians to the modern discoveries made in the last decade. But now we want to look forward, studying the current space missions and experiments to uncover the mysteries that astronomers hope to solve.

Click here to download the episode.

Or subscribe to: astronomycast.com/podcast.xml with your podcatching software.

The Future of Astronomy shownotes and transcript

Zoom into a New VISTA of the Sculptor Galaxy

VISTA’s infrared view of the Sculptor Galaxy (NGC 253). Credit: ESO

The new VISTA telescope at the Paranal Observatory in Chile (the Visible and Infrared Survey Telescope for Astronomy) has captured a great new image of the Sculptor Galaxy (NGC 253), and this video allows you to zoom in for a closer look. The sequence starts with a wide view of the southern sky far from the Milky Way. Only a few stars are visible, but then VISTA brings us in closer where the view shifts to the very detailed new infrared image of NGC 253 provided by the new telescope at Paranal. By observing in infrared light VISTA’s view is less affected by dust and reveals a myriad of cooler stars as well as a prominent bar of stars across the central region. The VISTA image provides much new information on the history and development of the galaxy. See the still image below.

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The Sculptor Galaxy (NGC 253) lies in the constellation of the same name and is one of the brightest galaxies in the sky. It is prominent enough to be seen with good binoculars and was discovered by Caroline Herschel from England in 1783. NGC 253 is a spiral galaxy that lies about 13 million light-years away. It is the brightest member of a small collection of galaxies called the Sculptor Group, one of the closest such groupings to our own Local Group of galaxies. Part of its visual prominence comes from its status as a starburst galaxy, one in the throes of rapid star formation. NGC 253 is also very dusty, which obscures the view of many parts of the galaxy. Seen from Earth, the galaxy is almost edge on, with the spiral arms clearly visible in the outer parts, along with a bright core at its center.

Learn more about this image and the VISTA telescope at the ESO website.

How Many Miles Around the Earth?

Planet Earth, as seen from Apollo 17 mission. Credit: NASA/)PL

Planet Earth, which we humans and all currently-known forms of life call home, is the third planet from the Sun, and the largest of the terrestrial planets. With a mean radius of 6,371 km (3,958.8 miles), it is slightly larger than Venus (which has a radius of approx. 6,050 km), almost twice the size of Mars (~3,390 km), and almost three times the size of Mercury (~2,440 km).

Basically, Earth is a pretty big world. But just how big if one were to measure it from end to end? If one were to just start walking, how many kilometers (and/or miles) would they have to go before they got back to where they started. Well, the short answer is just over 40,075 km (or just over 24,901 miles). But as always, things get a little more complicated when you look closer.

Continue reading “How Many Miles Around the Earth?”

Fully Functional Pan-STARRS is now Panning for Stars, Asteroids and Comets

Pan-STARRS PS1 Observatory. Image courtesy of Rob Ratkowski Photography and the Haleakala Amateur Astronomers.

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There’s a new eye on the skies on the lookout for ‘killer’ asteroids and comets. The first Pan-STARRS (Panoramic Survey Telescope & Rapid Response System) telescope, PS1, is fully operational, ready to map large portions of the sky nightly. It will be sleuthing not just for potential incoming space rocks, but also supernovae and other variable objects.

“Pan-STARRS is an all-purpose machine,” said Harvard astronomer Edo Berger. “Having a dedicated telescope repeatedly surveying large areas opens up a lot of new opportunities.”

“PS1 has been taking science-quality data for six months, but now we are doing it dusk-to-dawn every night,” says Dr. Nick Kaiser, the principal investigator of the Pan-STARRS project.

Pan-STARRS PS1 Observatory just before sunrise on Haleakala, Maui. Credit: Harvard-Smithsonian Center for Astrophyiscs

Pan-STARRS will map one-sixth of the sky every month and basically be on the lookout for any objects that move over time. Frequent follow-up observations will allow astronomers to track those objects and calculate their orbits, identifying any potential threats to Earth. PS1 also will spot many small, faint bodies in the outer solar system that hid from previous surveys.

“PS1 will discover an unprecedented variety of Centaurs [minor planets between Jupiter and Neptune], trans-Neptunian objects, and comets. The system has the capability to detect planet-size bodies on the outer fringes of our solar system,” said Smithsonian astronomer Matthew Holman.

Pan-STARRS features the world’s largest digital camera — a 1,400-megapixel (1.4 gigapixel) monster. With it, astronomers can photograph an area of the sky as large as 36 full moons in a single exposure. In comparison, a picture from the Hubble Space Telescope’s WFC3 camera spans an area only one-hundredth the size of the full moon (albeit at very high resolution).

This sensitive digital camera was rated as one of the “20 marvels of modern engineering” by Gizmo Watch in 2008. Inventor Dr. John Tonry (IfA) said, “We played as close to the bleeding edge of technology as you can without getting cut!”

Each image, if printed out as a 300-dpi photograph, would cover half a basketball court, and PS1 takes an image every 30 seconds. The amount of data PS1 produces every night would fill 1,000 DVDs.

Another view of Pan STARRS PS1 Observatory. Image courtesy of Rob Ratkowski Photography and the Haleakala Amateur Astronomers.

“As soon as Pan-STARRS turned on, we felt like we were drinking from a fire hose!” said Berger. He added that they are finding several hundred transient objects a month, which would have taken a couple of years with previous facilities.

Located atop the dormant volcano Haleakala (that’s Holy Haleakala to you, Bad Astronomer) Pan-STARRS exploits the unique combination of superb observing sites and technical and scientific expertise available in Hawaii.

Source: CfA

What Type of Planet is Mars?

The Grand Canyon of Mars
The Grand Canyon of Mars

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“What type of planet is Mars?” is a question that many readers ask. Mars is one of the four terrestrial planets. Mercury, Venus, and Earth are the other three. All of the terrestrial planets are made up of rock and metals. The remaining planets are classified as the outer gas giants.

All of the terrestrial planets have the same basic structure: core, mantle, crust; although each layer differs in thickness depending on the planet. Mercury has an average density of 5.43 g/cm3. Earth is the only planet more dense than Mercury. Mercury most likely has a liquid core that is mostly an iron-nickel alloy. The core accounts for as much as three-fourths of the planet’s radius. There are no numbers available for how thick the mantle and core are. Venus has a crust that extends 10-30 km below the surface. After that, the mantle reaches to a depth of some 3,000 km. The planetary core is a liquid iron-nickel alloy. Average planet density is 5.240 g/cm3.

Even though we live on Earth, not everyone is aware of its density and the depth of the various layers of our home world. The crust thickness averages 30 km for land masses and 5 kilometers for seabeds. The mantle extends on to an additional depth of 2,900 km. The core begins at a depth of around 5,100 km and is in two distinct parts: the outer core of liquid iron-nickel alloy and the inner core which is a solid alloy of iron-nickel. Average planet density is 5.520 g/cm3. The final terrestrial planet is Mars. Mars is roughly one-half the diameter of Earth, which leads scientists to speculate that the core has cooled and solidified. The depth of the crust and mantle are not known for sure, but the average planet density is 3.930 g/cm3. While there are only four terrestrial planets in our Solar System, here is a report on how NASA is trying to find more in other star systems.

Since we are talking specifically about Mars, we will talk about the composition of the planet’s surface material. There are hundreds of volcanoes on the surface of Mars. Several are regarded as the tallest mountains in the Solar System. Without plate tectonics, these volcanoes erupted for millions of years. Those massive eruptions explain why the entire surface is covered in basalt that is high in iron content. The iron content in the basalt has interacted with the Martian atmosphere and oxidized. The iron oxide explains why the entire Martian surface is coated in a reddish dust.

Answering ”what type of planet is Mars” took us on a little bit of a tangent. Hopefully, it is a tangent that will inspire you to find out more about the Red Planet.

We have written many articles about Mars for Universe Today. Here’s an article about the gravity on Mars, and here’s an article about the size of Mars.

If you’d like more info on Mars, check out Hubblesite’s News Releases about Mars, and here’s a link to the NASA Mars Exploration home page.

We’ve also recorded an episode of Astronomy Cast all about Mars. Listen here, Episode 52: Mars.

Source:
NASA

What Type of Planet is Venus?

Venus Cloud Tops Viewed by Hubble
Venus Cloud Tops Viewed by Hubble

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Venus is the second planet from the Sun, and a virtual twin of our own planet Earth in many ways. But what type of planet is Venus? There are two major classifications of planets in the Solar System. There are the inner, rocky terrestrial planets and then the outer gas giants. Venus is a terrestrial planet.

The terrestrial planets are the 4 inner rocky worlds in the Solar System: Mercury, Venus, Earth and Mars. The word terrestrial comes from the root term “terra”, which is Latin for Earth. So the terrestrial planets are “Earth like” worlds.

And Venus is the most Earth-like planet in the Solar System. It has almost the exact same size, mass and density. Its composition is probably very similar to Earth, with a metallic core surrounded by a rocky mantle and a thin crust. The main difference between Earth and Venus is the incredibly thick carbon dioxide atmosphere, which raises temperatures on the surface of Venus to the point that it’s hot enough to melt lead.

But compare a terrestrial world like Venus to the gas giants like Saturn and Jupiter. The mean density of Venus is 5.204 g/cm3. While the density of Saturn is only 0.687 g/cm3. The density of Saturn is less than water, and it would float if you could find a pool large enough.

We’ve written many articles about Venus for Universe Today. Here’s an article about pictures of planet Venus, and here’s an article about how to find Venus in the sky.

If you’d like more info on Venus, check out Hubblesite’s News Releases about Venus, and here’s a link to NASA’s Solar System Exploration Guide to Venus. Finally, here’s a link to ESA’s Venus Express spacecraft.

We have also recorded an entire episode of Astronomy Cast all about Venus. Listen here, Episode 50: Venus.