A Triple System of Star Corpses

An international team of astronomers has just reported the discovery of one of the weirdest star systems we have ever seen -- a triple system of star corpses (dead stars) whirling around each other in a space smaller than the Earth's orbit around the Sun.

The system of stars is more than 4,000 light years away, in the constellation of Taurus. (But this story is no bull!) The system doesn't have a name, only a catalog number.  It consists of one "neutron star" (which pulses with radio waves) and two "white dwarfs."  Generally, a tiny "neutron star" only forms after a massive star dies by blowing itself to pieces, leaving a very compressed remnant (or "corpse") behind.  So, those three stars, which show evidence of having formed together, had to remain together even when the biggest star of the three exploded.  Later, the two smaller stars died and also became compressed objects (not much bigger than a planet) called "white dwarfs."  (They get that name because they are small and white hot.)

Now the three corpses continue to spiral around each other, in a strange cosmic ballet .  The heaviest corpse, the "neutron star" is really dense -- it is so compressed that to make something like it on Earth, we would have to take all the people in the world and squeeze them into a raindrop!  (Then we would have one rain-drop sized piece of the neutron star.)

Sometimes we see such "neutron stars" giving off spinning magnetic beams of radio waves.  Whenever such a radio beam sweeps over the Earth, we get a pulse of radio waves.  In such cases, we also call these dead stars "pulsars."   Their beams of energy can be timed with great accuracy.

In 1974, my former college advisor, Joseph Taylor (and Russell Hulse,) discovered the first pulsar in a double star system.  Measuring its pulses enabled them to verify important predictions of Einstein's General Theory of Relativity, and earned them the 1993 Nobel Prize in Physics.  At the time, astronomers thought that finding a neutron star/pulsar with a companion was pretty surprising (although today other double systems are known.)

Now suddenly, we have a neutron star/pulsar with TWO companions.  How completely and wonderfully weird!  And this particular neutron star spins hundreds of times per second. Its fast spin and two companions will allow astronomers to measure the predictions of Einstein's theories even more precisely than we have been able to do in the past.

An Old Star for the New Year

Happy next orbit around the Sun, everyone. The center of our beautiful new year photo shows a Hubble image of an old star that is going through a little bit of a crisis in its life (as older stars -- and people -- tend to do.) The star, called RS Puppis, is getting brighter and dimmer on a regular cycle every 41 days. Stars that become changeable like this for a short part of their lives are called "Cepheid Variable Stars."

RS Puppis is one of the brightest known Cepheids, shining on average 15,000 times brighter than the Sun. It contains about 10 times more material than our Sun, and is 200 times larger in extent (an earlier part of its life crisis was swelling up to be much bigger than stars usually are.)

Because this star is surrounded by a cocoon of dust, the changing light from it is seen reflected from the dusty shells around it. (By the way, the cross of light you see coming from the main star and others in the picture is not real -- it is called a "diffraction spike" and is light sneaking around the support structure of one of the mirrors in the Hubble telescope.)

Cepheid variable stars are an important category of stars in astronomy. Their variations allow us to measure their distances and they are a cornerstone of how we know how far away things are in the universe. About 100 years ago, Henrietta Leavitt, a low-paid "computer" working at the Harvard College Observatory found the crucial relationship that allowed Cepheids to be used for this purpose. Even though women were not usually acknowledged for the "behind-the-scenes" work they did at the Observatory, this discovery was so important it was hard to deny her credit.

Playwright Lauren Gunderson has written a play about Henrietta Leavitt called "Silent Sky." It is coming to the Mountain View (CA) Center for the Performing Arts in January and February, for those readers who live in the San Francisco Bay Area. For everyone else, you can see a short excerpt from a previous production at:http://www.youtube.com/watch?v=KiwG6r-9gcw

Happy new year and may your skies be dark and clear in 2014.

P.S. For more on Henrietta Leavitt and contributions by other women to astronomy, see my resource guide: http://www.astrosociety.org/education/astronomy-resource-guides/women-in-astronomy-an-introductory-resource-guide/

45th Anniversary of the Famous Earthrise Photo

It was on Dec. 24, 1968 that astronauts aboard the Apollo 8 mission orbiting the Moon took one of the most famous images in the history of photography. It's become known as "Earthrise on the Moon," and we will soon be celebrating its 45th anniversary.

Moon chronicler Andrew Chaikin has worked with NASA to make a short video of the complete story of how this image came to be taken, and wrote me about recently. I thought I would share it with all of you -- whether you are an old geezer like me (and were alive in 1968) or whether you are newer to life on Earth and saw the picture later. You can find the video at:http://www.youtube.com/watch?v=dE-vOscpiNc

I love the image and its portrayal of a small, fragile planet Earth isolated in space above the airless surface of the Moon. But since this is the AstroProf's page, I have to add, like a good teacher should, that the name creates a bit of a misimpression.

When we talk about sunrise on Earth, we mean that as the Earth turns, we can see the Sun rise above the eastern horizon. As the day goes on, we see the Sun move through our skies, until, in the evening, it sets below the western horizon. What we see as the rising and setting of the Sun is just the effect of the 24-hour rotation of our planet. The spinning of the Earth causes the whole sky to go around us in a day.

The Moon's spin is much slower than Earth's! It takes the Moon 27.3 Earth days to spin once. And in exactly the same 27.3 days, the Moon also orbits once around the Earth. This "tidal locking" of the two motions, the Moon's spin and its revolution around us, means that the Moon always keeps the same face to the Earth.

If you don't believe or see this, try the experiment with your little brother. Put him in the middle of an empty space, face him, and then go around him in the exact same time as you turn your shoulders in a circle. If you take the same time to go around him as to go around yourself, your little brother will always see the front side of your body and never the back side.

For the same reason, if you stand on the Moon, you will either see the Earth in your sky (if you are on the near side of the Moon) or you will not (if you are on the far side). But the Earth will not rise or set in the Moon's sky the way the Sun or Moon rise and set in our sky.

In the famous picture, the Earth only seemed to be "rising" to the astronauts because the Apollo spacecraft was orbiting the Moon.

But if future visitors to the Moon's surface really want to see an Earthrise, it is possible. The Moon wobbles back and forth just a bit (we call it "lunar libration") and so, if you stand in just the right place on the Moon, you could see the Earth dip very slowly below the horizon and then come up again. (Google lunar libration if you want the technical details.)

For everyone else, just enjoy the image and the video. In these times of strife and mistrust everywhere, it's good to remember that -- in the larger picture -- we are all passengers aboard spaceship Earth, sharing its limited area and limited resources.

A Beautiful New Image from the Hubble Telescope

Here is a gorgeous picture of a spiral galaxy, which is part of the Coma Cluster of galaxies, roughly 300 million light years away. This galaxy (of billions of stars), like our own, is shaped like a frisbee -- and we are looking at the disk of the frisbee face-on. Its name is just a catalog number: NGC 4921. You can see its huge encircling "arms" of countless stars, blending their light together. And notice a number of clusters of young stars glowing blue, a little distance out from the center.

But what is amazing about this image, if you look at it for a while, is how many OTHER galaxies are visible through and around NGC 4921! All those structures around the galaxy that are not precise pinpoints of light are other great islands of stars -- each containing billions of stars and planets. The cluster of galaxies which NGC 4921 is part of contains more than a thousand galaxies. And there are more galaxies beyond that cluster. Pictures like this help us remember that our problems and disagreements on Earth are such minor issues when seen from the perspective of the universe.

This image, by the way, was assembled from a number of Hubble Space Telescope images and processed by Roberto Colombari, an Italian astronomical photographer working in Brazil.

Comet ISON Ready for its Thanksgiving Date with Destiny

When it was discovered in 2012 as a new comet coming from deep space, some observers predicted Comet ISON would become so bright in our skies it would be the "Comet of the Century." Wiser heads knew, as comet hunter David Levy likes to say, "Comets are like cats. They have tails and they do precisely what they want!"

For a while, the comet seemed disappointing. But this week, on its way in to a close encounter with the Sun, Comet ISON started putting on a somewhat better show (as you can see in the image, taken by the skillful UK astro-photographer Damian Peach.) The comet now has two nice tails, one made of dust, the other of gas, pointing in the direction away from the Sun.

The comet is currently visible in the pre-dawn sky, but only barely and only when it's really dark. It's better with binoculars or telescopes. The excitement, however, is just beginning. Comet ISON is what astronomers call a "sungrazer" -- a comet that comes indecently close to our Sun. It just so happens, the closest encounter -- only about 3/4 of a million miles from the Sun's surface -- will be on Thanksgiving Day 2013.

The solid "nucleus" of this comet -- a chunk of frozen ices and rock -- is now estimated to be somewhere between 1/4 and 3/4 of a mile across. The Sun's heat could vaporize much of its ice and rock and the Sun's gravity could tear it apart into smaller chunks. Past sungrazing comets have had one or both of these things happen. So it could emerge from its date with the Sun one smaller but strongly evaporating comet, or as several comets spread out over a wider area, or as nothing more than a subtle trail of gas and dust.

If Comet ISON survives Thanksgiving, it will swing away from the Sun and emerge into our dark skies going northward from the plane of our solar system. Should there be enough of it left to make a show, that show will be visible to us in December and January. Around January 8th, for example, it will be near the north star, remaining in our view all night long. (But by then it will likely be much fainter.)

As we say on the radio, "Stay Tuned!" I will give you more updates on this interesting new visitor to our cosmic neighborhood in future posts.

If your want bulletins on Comet ISON between my posts, or need more technical information, see the "Current Status" page at NASA’s Comet ISON Campaign: http://isoncampaign.org/Present and then look around on that site.

[If you search the web for Comet ISON information, beware of the nutty websites predicting a collision with Earth or some other reason for the end of the world. The closest the comet will get to Earth is about 40 million miles on Dec. 26th. That's far enough that we can all sleep soundly at night.]

Billions of Earth-like Planets

This week, the University of California, Berkeley and NASA's Kepler Telescope project jointly announced that the ongoing discovery of planets around other stars had yielded some exciting statistics: It now appears that one out of five Sun-like stars has an Earth-like planet!

One out of five! This means there are likely to be BILLIONS of earth-sized planets orbiting at comfortable distances from BILLIONS of stars in our Milky Way Galaxy. All of us involved with SETI -- the Search for Extra-Terrestrial Intelligence -- are, of course, thrilled to hear this news. Our hope is that among all those planets, there are some where intelligent creatures with an interest in astronomy have developed and perhaps enjoy their own blogs with astronomy news like we do.

The latest stats about known planets around other stars are also record-breaking.  As of early November 2013, we have found 1039 planets around 787 stars beyond our solar system! (There are 173 stars so far where we have discovered more than one planet in the same system.)  In addition, the Kepler mission (which is searching for such planets from space) already has over 3000 candidate planets which are still being checked out!  And they still have a whole year's worth of data to go through.

I was interviewed on KQED, the San Francisco Bay Area public radio station, by Michael Krasny, the host of the Forum program, about all this -- and we were joined by the Berkeley graduate student who had done the basic work of making the estimates. If you want to hear the interview, it is available at:
http://www.kqed.org/a/forum/R201311060930 

Earth-like Planet Discovered in a Ridiculous Orbit

 Astronomers from two continents made a startling announcement last week. They had found a world similar in size and composition to the Earth that orbited its star in only eight and a half hours.... Just think about that for a minute. Our planet takes 365 and a quarter days to complete its orbit. The innermost planet in our system, Mercury, takes 88 days to circle the Sun. The new planet, designated Kepler 78b, takes only about a third of one of our days to orbit its star. In other words, a year on Kepler 78b is only 8.5 hours long -- a two-Earth-year-old toddler on this alien world would already be 2,063 years old in local time!

The planet is a bit larger in size than our Earth, but made of dense rock like our inner planets (and not gas and liquid, like our outer planets.) Since it circles so close to its star, it must be torridly hot, so we imagine its surface is molten rock and not solid like our own crust.  Some are calling it a lava planet.

How can astronomers know so much about a distant world like Kepler 78b? As its name implies, the planet was discovered around a faint star in the constellation of Orion by the Kepler telescope in space. Kepler's camera measures the size of a planet when the planet is seen going across the face of its star and diminishing the star's light briefly. But that can only tell us how big the planet is across, and not what kind of material it's made of.

But once Kepler found the planet, astronomers in the U.S. and Europe used giant telescopes on the ground to find the tiny wiggle the pull of the planet causes in the motion of its star. This "wiggle method" tells us how much pull (gravity or mass) the planet has.

When astronomer combine the size of the planet from Kepler and the mass of the planet from the wiggle method, they can calculate the planet's "density" (mass per unit volume). In this case, all the measurements made it clear this was a dense world, made of rock, just like our Earth.

The mystery is: how did an Earth get SO outrageously close to its star. If it was falling in, what made it stop? We know it couldn't have been born so close to the star, because the star was larger when it was young, and the planet would have been inside the star, where no planet can exist. Kepler 78b is part of a group of strange planets Kepler has been discovering -- all of them too close to their stars for their own good and for our peace of mind.