Two Baby Alien Worlds Show Us How to Cook a Planet
Two new exoplanets have been discovered, and they’re important milestones in our understanding of how alien solar systems behave. That’s because both are very young, both are massive, and both orbit their stars very close in, closer than Mercury orbits the Sun.
First, a quick intro to the problem: When astronomers first started finding planets around other stars in the mid-1990s, they were surprised to find that many were as big and massive as Jupiter but so close to their parent stars that they had orbital periods measured in days. Given that Mercury, the innermost planet in our solar system, is small and takes three months to circle the Sun, these “hot Jupiters” were pretty shocking. How did they get there?
Models of planetary formation show that it’s very unlikely a big planet can form so close to the star. Most likely, they form farther out and somehow migrate in toward the star. One way would be to interact with the disc of debris circling the star from which the planet formed. As it plows into this material, it can drop down to the star. It’s unclear if this happens very early in the life of the planet (like, within a million years or so after it forms) or much later, like right before the debris disk is blown away by the star millions of years later.
Another way would be for it to gravitationally interact with other planets in the system, which can affect their orbits. This method takes a while, though, and is slower in general than the debris disk method. The problem: Most planets found are old, a billion years or more, so it’s hard to know just when the hot Jupiter moved.
These two new planets change that.
One is called K2-33b and was found by the Kepler spacecraft, the one that has discovered so many alien worlds. The star, K2-33, is about 460 light-years away and is a cool red dwarf, only about 0.6 times the mass of the Sun and shining at a feeble 15 percent as bright*. It’s part of a loose cluster of stars called the Scorpius-Centaurus OB Association, which is known to be young. The colors of the star also indicate youth (it’s still very hot from its formation, so it’s bluer than you’d expect), and the smoking gun is the presence of lithium in the star’s atmosphere; that element gets destroyed by a star very quickly, so seeing any at all means the star is very young. All together, this points to an age of no more than 20 million years, and most likely closer to 11 million years.
Our own Sun is 4.56 billion years old, so this star is basically a wee bairn.
K2-33b, the planet (note the “b”) is roughly 60,000 kilometers across, a bit less than five times Earth’s diameter. It has no more than the mass of Jupiter, and likely has less—it’s more like a super-Neptune or a mini-Jupiter. It orbits the star every 5.4 days, so it’s close.
Given its youth, that strongly indicates that massive planets can migrate rapidly toward their star right after they’re born, perhaps even while they’re still forming.
But wait! There’s more! We have the other planet, too.
Before I even get started, let me say that this second planet has not yet been confirmed, but given the circumstances it seems very likely it’s real. I’d be happier with more independent evidence, but the authors indicate the probability of it actually existing is very high.
This one orbits the star V830 Tau, which has a mass almost the same as the Sun, but is twice the radius and about 20 percent more luminous. The planet orbits the star every five days at a distance of just 8.5 million kilometers—that’s very close indeed. Even better, the age of the star appears to be only about 2 million years, which is even younger than K2-33!
So, in both cases, we have a massive planet, which is orbiting very close to its star and is very young. That’s very exciting! They show that planetary migration can happen almost immediately, even as the planet and star are still settling down after their formation.
Mind you, this doesn’t mean planets don’t move later in life. In fact, we have evidence that planetary interactions do happen (some planets orbit their stars backward, in the opposite sense of the star’s rotation, which can happen if the planet has undergone a game of celestial billiards with other planets).
So what we now seem to find is that there’s more than one way to cook a Jupiter, and it can happen right away or it can take a while.
This is amazing. I’ll remind you that until 1995 we didn’t even know if other planets existed around other stars like the Sun. It’s only been 20 years, and we’ve learned so much about them! We have thousands to study, and they come in so many flavors: Big, small, hot, cold, puffy, compact … we see planets like the ones in our solar system, and ones that are entirely alien.
And we’re still just getting started here. We know of something like 3,000 planets right now, but there are likely hundreds of billions in our galaxy alone! With a sample size that vast, even something very unlikely is bound to happen. What other strange new worlds await us?
* Correction, June 21, 2016: I originally wrote that K2-33 has a diameter of 0.6 times the Sun's, but I meant the mass. Weirdly, it's actually about the same size as the Sun, because it's still so hot from formation that it's inflated a bit. It'll shrink as it ages.
Happy Full Moon Solstice!
On Monday at 22:34 UTC (6:34 pm Eastern U.S. time), the Sun will reach its highest declination in the sky, its farthest point north for the year. That is the moment of the June solstice.
This means that, in the Northern hemisphere, we have the longest day of the year, and the shortest night. If you live your life standing on your head in the Southern hemisphere, it means you have the shortest day, and the longest night.
I enjoy writing about the solstices and equinoctes* when they happen, so you can read all about how and why they occur in past articles. I’ll note that Monday is not the date of the earliest sunrise and latest sunset though; that has to do with the Earth’s orbit being slightly elliptical, so I’ll make a special point of linking to this article last year where I explain why that happens. I’ll also note that some people call this the first day of summer (or winter for those in the south), but I disagree; I tend to think of it as actually the midpoint. You can read about that to your brain’s delight as well.
No, instead of spending time on that here, I’d prefer to point out something rather special that led to me wandering down a rabbit hole Sunday night as I researched it: Not only is the solstice Monday, but the Moon is full on Monday as well. That moment occurred at 11:02 UTC (07:02 Eastern; I’ll note it’ll look full all day and probably even Tuesday as well).
A full Moon on the same day as the June solstice (or the December one, for that matter) is relatively rare. As I thought about this Sunday night, I wondered just how rare it was. My first thought was that it probably happens once every 30 years or so, since the full Moon can occur on any day, and there are 30 in June.
But then I realized it’s not that simple. Sometimes in astronomy two cycles can beat together in unusual ways, throwing off what you might expect. So I dug into it. I found a list of solstice full Moon dates on the Farmer’s Almanac website, and perusing the numbers it appears that we get a full Moon on the June solstice roughly every 19 years or so … or multiples thereof.
Nineteen years? That sounded familiar. It took me a few minutes, but then it clicked: That’s the Metonic cycle! Let me explain.
The Moon goes through a full phase of cycles (from full to new and full again) in about 29.53 days. That all by itself is interesting, and I talk about that in the episode of Crash Course Astronomy on the phases of the Moon:
One Earth year is, on average, about 365.24 days long. But there’s a funny coincidence here: 19 years is 6,939.56 days, and that is almost a perfect multiple of 29.53! Nineteen years is almost exactly 235 lunar phase cycles. That means that when you have a full Moon on a given date, 19 years later it’ll be on that same date once again. That’s what’s called the Metonic cycle. This fact has been known for about 2,500 years, which is pretty amazing.
But looking at the Farmer’s Almanac, you see it doesn’t seem to happen every 19 years. Why not?
This is where I really started to dig deep. I looked at leap years, and fractional leftovers between the lunar phase month (called the synodic month) and the Earth’s year, and on and on. That can account for some of the reason the full Moon doesn’t always fall on the same calendar date every 19 years.
Then I realized something: time zones.
Astronomical sites list the times of the solstices and full Moons in Coordinated Universal Time (UTC, similar to Greenwich time). That makes it easy for everyone, since you can just look up how far off your time zone is from that (for example, right now the East Coast of the U.S. is on Eastern Daylight Time, UTC – 4 hours).
But that can mess up the full Moon June solstice cycle. Why? Because the exact moment of the solstice changes year to year, and can even occur on different days! It can be on June 20, 21, or sometimes even 22. If the solstice occurs on June 21 at 23:59, and the full Moon two minutes later, technically they’re on different days!
Worse, that’s UTC. In the U.S., where it’s four to seven hours earlier than UTC, both would occur on the same calendar day. So it’s possible (and even likely) that one place in the world would see a full Moon on the same calendar day as the solstice, and another part of the world wouldn’t. What a mess!
Look at Monday’s solstice: It occurs at 22:34 UTC. For someone a couple of time zones east of the U.K., that means it happens on June 21. For them, they don’t get a full Moon on the day of the solstice. The exact moments of the solstice and full Moon are independent of time on Earth (the solstice occurs at the same moment for everyone on the planet, for example), but because we bin time up into days, that can throw off the days on which we say those events happened. Weird.
Going back to the Farmer’s Almanac, you may notice that while the solstice full Moon doesn’t happen every 19 years, it does appear to have a cycle of multiples of 19. For example, there was one in 1796, then the next in 1834, a gap of 38 years, 2 x 19. Other such gaps can be found. The gaps happen because the full Moon missed the calendar day of the solstice by some hours. Not only that, but that table is for the U.S. East Coast, so it doesn’t work for the whole world.
The root of this problem is using calendar days, which are arbitrary to some extent. There’s an overall 19-year cycle, but because of time zones it can get thrown off. A better way to do this would be to ask, “How often does a full Moon occur within a day of the solstice?,” or better yet within 12 hours before to 12 hours after the moment of the solstice.
In that case, I’d expect the 19-year Metonic cycle to be more obvious. However, looking that up using calendars for the full Moon (like this one) and the solstices (like this one) is difficult and tedious. The best way would be to run the calculations specifically looking for that, which I thought of too late to ask anyone to do for Monday’s events. I’ll leave that as an exercise for the reader.
Anyway, my point is … well, I guess I don’t have a point except that numbers are fun to play with and the cycles in the sky are neither always obvious nor simple to grasp.
But they’re there, and if a full Moon falling on the solstice is interesting enough to people that they go outside and take a look for themselves, then I’m all for it.
So happy full Moon June solstice! Enjoy it, because the next one won’t be for a while—June 21, 2062, in fact … if you use UTC.
*Equinoctes is the actual plural for equinox. Some dictionaries say that’s a bit old-fashioned, and equinoxes is now used, which is fine by me. Languages change over time. But I rather like the way equinoctes sounds, and I like using it. So I do.
March … I Mean April… I Mean May 2016 Is the Sixth … I Mean Seventh… I Mean Eighth Temperature Record-Breaking Month in a Row
October. November. December. January. February. March. April. And now May.
sixth seventh eighth month in a row, we’ve had a month that has broken the global high temperature record. And not just broken it, but shattered it, blasting through it like the previous record wasn’t even there.
According to NASA’s Goddard Institute for Space Studies,
March April May 2016 was the hottest March April May on record, going back 136 years. It was a staggering 1.28°C 1.11°C 0.93° C above average across the planet.* The previous March April May record, from 2010 2014, was 0.92° 0.87° 0.86° above average. This year took a huge jump over that.
Welcome to the new normal, and our new world.
As you can see from the map above, much of this incredible heat spike is located in the extreme northern latitudes. That is not good; it’s this region that’s most fragile to heating. Temperatures soaring to 7° or more above normal means more ice melting, a longer melting season, loss of thinner ice, loss of longer-term ice, and most alarmingly the dumping of billions of tons of fresh water into the saltier ocean which can and will disrupt the Earth’s ability to move that heat around.
What’s going on? El Niño might be the obvious culprit, but in fact it’s only contributing a small amount of overall warming to the globe, probably around 0.1° C or so. That’s not nearly enough to account for this. It’s almost certain that even without El Niño we’d be experiencing record heat.†
Most likely there is a confluence of events going on to produce this huge spike in temperature—latent heat in the Pacific waters, wind patterns distributing it, and more.
And underlying it all, stoking the fire, is us. Humans. Climate scientists—experts who have devoted their lives to studying and understanding how this all works—agree to an extraordinary degree that humans are responsible for the heating of our planet.
That’s why we’re seeing so many records lately; El Niño might produce a spike, but that spike is sitting on top of an upward trend, the physical manifestation of human induced global warming, driven mostly by our dumping 40 billion tons of carbon dioxide into the air every year.
Until our politicians recognize that this is a threat, and a very serious one, things are unlikely to change much. And the way I see it, the only way to get our politicians to recognize that is to change the politicians we have in office.
That’s a new world we need, and one I sincerely hope we make happen.
*GISS uses the temperatures from 1951–1980 to calculate the average. The Japanese Meteorological Agency uses 1981–2010, which gives different anomaly numbers, but the trend remains the same. Realistically, the range GISS uses is better; by 1981 global warming was already causing average temperatures to rise.
† You may have noticed that the actual temperature anomaly for each month over March through May appears to be dropping; 1.28 to 1.11 to 0.93. That may be due to El Niño weakening, but it’s hard to know over such a short time period. Even if the trend continues, I’d bet 2016 will be the hottest year on record.
ExoMars Sees Mars
When you spend a lot of time and effort to send a spacecraft to another planet, it’s a nice benchmark when that spacecraft first spots it.
The image above is Mars, as seen by the Trace Gas Orbiter, part of the European Space Agency’s two-pronged ExoMars program (the first mission is the TGO plus Schiaparelli, a lander that will test technologies for future missions, including the 2020 ExoMars rover). TGO and Schiaparelli were launched on March 14 and were about 41 million kilometers from its destination when this shot was taken.
Mars is only about 6,800 kilometers in diameter, so from that distance it was only a dozen or so pixels across in the camera of the Trace Gas Orbiter. That’s pretty small, which is why it’s hard to see much here. But it shows the camera works! To make the picture a little clearer, here’s a slightly (3 pixel Gaussian) blurred version of it:
The image release notes that the Tharsis region of Mars was facing the camera when the shot was taken. Tharsis is a huge area of Mars known for its four massive volcanoes, including Olympus Mons, the largest such beast in the solar system. I poked around and found a Mars picture by Hubble that more or less matches the ExoMars shot:
That was taken in 2003 and isn’t an exact match, but it’s close. Olympus Mons is the big splotch at the top center, and the dark southern region below it is called Terra Sirenum. Out of curiosity I shrank it to roughly the same size as the ExoMars picture, rotated it, and blurred it a bit to compare them:
Not bad. Not exact, but you can see the similarities. This first ExoMars mission will reach Mars in October, and once in orbit the camera (called CaSSIS) will be able to spot objects on the surface as small as 10 meters across—the size of a small house. So expect far more interesting picture than this coming this winter!
Blue Origin to Test Rocket Parachute Failure Sunday Morning
Update, June 19, 2016, at 13:00 UTC: The launch was a success! The peak altitude reached was more than 101 kilometers, passing above the Kármán line and into space. The crew capsule deployment looked good, with the two main parachutes slowing the capsule adequately (we’ll know more when the data are analyzed) and the capsule touching down about 10 minutes 30 seconds after launch. One note:The capsule appeared to land too soon, and I'm not sure the retrothrust system activated. We'll know more soon. The rocket itself landed vertically right on target, too.
On Sunday, at approximately 14:15 UTC (10:15 a.m. Eastern time), the private rocket company Blue Origin plans to launch its New Shepard rocket for the fourth time. As with the three previous tests, it’ll launch straight up, deploy the crew capsule, and then come back down vertically. The crew capsule will come back much more slowly, using parachutes to descend gently (and a retrothrust system to make sure the landing isn’t too rough).
Except this time, the company has rigged it so that only two of the three parachutes will open.
This test is being done on purpose to make sure they can still safely land in the event of single parachute failure. As Blue Origin CEO Jeff Bezos said, “Works on paper, and this test is designed to validate that.”
This should be an exciting test. In a very different move for the company, it has announced that it will be streaming the event live on its website (it starts at 13:45 UTC, a half hour before the launch). I find that very interesting; in general the company has not done that; they release video after the flights, and rarely even announce when the launch tests will be. I wouldn’t say they’re secretive, but they tend not to actively seek publicity.
I have to wonder if the live coverage of SpaceX launches is behind this decision. Obviously, SpaceX has captured the lion’s share of the public’s attention when it comes to rocket launches. SpaceX has carefully cultivated an excellent public outreach effort, and the result is that its launches are watched live by a lot of folks. I imagine Blue Origin wants a piece of that.
They deserve it. New Shepard (named after astronaut Alan Shepard, the first American in space) has launched successfully three times, and each flight has tested different aspects of the process, including a quick restart of the engine only a kilometer above the ground before landing. It’s actually pretty amazing.
What SpaceX is doing and what Blue Origin is doing are, at the moment, very different. SpaceX is launching a very large rocket into orbit, meaning it has to go sideways (usually to the east) very rapidly to go around the Earth. Blue Origin’s flights are suborbital; the rocket goes essentially straight up, past the arbitrary but generally agreed-upon 100-kilometer altitude marking the beginning of space (at that height, there’s almost no air and no drag on the rocket). That’s far easier than going into orbit.
But not easy. Going up that high, releasing a capsule, having that land safely, and landing the rocket itself back down vertically on its tail is incredibly hard. Blue Origin has shown they’re getting the hang of it, though.
And while there’s a good market for suborbital flights (even a few minutes of free fall can be very useful scientifically), the plan is to use the knowledge gained to create a more powerful rocket capable of orbital flight. This is how SpaceX did it with the Falcon 1 rocket that led to the Falcon 9, and Blue Origin has similar ideas. Its BE-4 engine, currently being tested, should have enough oomph to do this. United Launch Alliance, which makes the Atlas and Delta rockets, has partnered with Blue Origin to develop this engine for use with their next generation Vulcan rocket. That’s being created as a competitor for SpaceX’s Falcon series, and I’ll be very interested indeed to see how this goes.
I’ll be getting up early Sunday morning to watch this fourth New Shepard test flight, and live tweeting it, too. Rocket launches are fun and exciting, and these tests are the first steps toward a bigger and better arena for commercial spaceflight. I have a lot of hope for this new chapter in space exploration. A lot, and I think it’s been earned.
There’s an (apocryphal) curse: “May you live in exciting times.” I don’t think it’s a curse. I think it’s the best time to be alive.
Another Moon for Earth? Well, Not Really, but It Depends on Your Point of View.
The Earth has one satellite, right? That fact is so solid, we just call it the Moon with a capital M.
But due to a trick of gravity and timing, there are other objects out in space that aren’t really moons but do travel along with Earth through space. I guess “companions” would be a better name.
One of them was just discovered recently by astronomers: the asteroid 2016 HO3. It’s small, probably 40–100 meters in size, and let me be clear: It orbits the Sun, not the Earth, so I wouldn’t call it a moon. But its orbit is such that it always sticks near the Earth, and from our point of view even seems to go around us!
Here’s how that works. The asteroid was first seen in April 2016 in observations of the sky taken by the Pan-STARRS observatory, designed to look for asteroids and comets that get close to Earth. That’s recent enough that a really good orbit for it is hard to determine, but it turns out it was seen in older observations (those can be found by tracing the orbit backward and checking if any observations of it were archived), providing a much longer baseline and therefore a better orbit.
What they found is really interesting: The orbit of HO3 is very Earth-like! It’s very slightly elliptical, and tilted by about 8° with respect to Earth’s, but the average distance of the asteroid from the Sun is just a hair more than Earth’s, and it takes 365.93 days to orbit the Sun. That’s just 16.6 hours longer than Earth’s 365.24 daylong year!
Because it’s moving on a tilted and elliptical orbit, sometimes it’s a wee bit closer to the Sun and moving a bit faster than Earth, and sometimes it’s a wee bit farther out and moving a bit more slowly. But it never gets closer than about 14 million kilometers from Earth or farther than about 40 million kilometers.
That’s hard to picture, so I made an animation using the JPL Small Body Database Browser. It shows the inner solar system and keeps Earth centered as it and 2016 HO3 orbit the Sun (HO3’s orbit is blue; light blue for when it’s north of (“above”) the Earth’s orbit, and dark blue when it’s south (“below”). As time moves forward, you can see HO3 moving faster and ahead of the Earth, then slowing and lagging behind, but never getting very far away:
So as you can see it’s clearly orbiting the Sun, but never straying far from Earth. If you map its motion relative to Earth, it actually appears to go around us, like a moon! That’s shown in the diagram at the top of this article.
But it gets weirder. Because the orbit is slightly longer than Earth’s, you’d expect it to drift away over many years, lagging behind Earth more and more every year. But that’s not the case! Earth’s gravity tugs on HO3, changing the orbit slightly every time they pass. That keeps HO3’s orbit in line with Earth’s, so it never gets too close or too far away. It’ll be our companion for at least the next few centuries.
If you’re wondering how we’ve missed it all this time, I’ll remind you it’s small and still pretty far away in terms of actual kilometerage. Even at closest approach it’s at about 21st magnitude, or just one-millionth as bright as the faintest star you can see with your unaided eye. It takes a decent telescope to see it at all.
I find things like this delightful. The Universe is so surprising! Due to the law of gravity our solar system is in many ways like a clock, each object like a gear ticking away in time with the others.
But there’s more than fanciful analogies to be had here: Because of its similar orbit, HO3 is moving relatively slowly compared with Earth’s motion through space. That makes it a rather tempting target for a space mission, where how much fuel you need to get from point A to point B depends on their relative motion. HO3 is moving just a few kilometers per second relative to Earth in some parts of it orbit, making it much easier to send a probe there. Or maybe, someday, humans.
How about that? One of the best targets we could hope for, and we just discovered it a few weeks ago. The Universe really is surprising.
LIGO Bags Another Binary Black Hole Burst
About 1.4 billion light-years from Earth, two black holes were on a dance of death. One was about 14 times the mass of the Sun; the other eight. For a long time their orbits had been decaying, approaching each other ever more rapidly. And then, finally, so close they were whipping each other around at very nearly the speed of light, they merged. The event was catastrophic, sending out a blast of energy that literally shook the very fabric of the Universe itself.
Eons later, that death cry was seen by astronomers here on Earth. By the time it got here it was vanishingly feeble, but strong enough to shake the sensors in LIGO, the Laser Interferometer Gravitational-Wave Observatory. Two facilities comprise the observatory, one in Livingston, Louisiana, and the other in Hanford, Washington. Each one uses a system of lasers to measure the distance between a set of mirrors, and when the ripples in space-time emanating from the black hole merger passed through the Earth, they changed the distance between mirrors ever so slightly.
Perhaps I’d better explain. In fact, I already have, when the first event was announced in February 2016:
One of the outcomes of Einstein’s General Relativity theory is that space and time are two facets of the same thing, which we call space-time. There are lots of analogies for it, but you can think of it as the fabric of space, a four-dimensional tapestry (three of space and one of time) in which we are all embedded. Remember, it’s not literally like this; we’re using an analogy. But it’ll help you picture it …
… if a massive object is accelerated, it will cause ripples, waves, to move away from itself as it moves. These are actually ripples in the fabric of space-time itself! Space-time expands and contracts in complicated ways as a wave passes, a bit like how ripples will move out from a rock dropped into a pond, distorting the surface of the water.
In other words, when a massive object accelerates, it emits what’s called a gravitational wave that quite literally stretches and shrinks space. The more massive the object and the higher the acceleration, the more powerful the gravitational wave is, and the more space gets distorted. Most objects in the Universe are way too placid to do this, but when two black holes merge, the masses are high and the acceleration fierce.
Even then, by the time the waves get here (moving at the speed of light across the Universe), the ripples are incredibly tiny. The ripples from this new event, called GW 151226 (for the gravitational wave source detected on Dec. 26, 2015), stretched space by only a factor of about 10-22 by the time they reached Earth. That’s so small it’s hard to imagine, so let me put it this way: If you had a ruler a kilometer long, as a ripple passed through, it would change its length by less than the width of a proton!
Still, that’s measurable! Barely. As I described in my earlier article, LIGO is designed to see incredibly small strains in the fabric of space-time. The biggest problem is noise; in this case the detectors are so sensitive that they can detect molecules of air hitting the mirrors!
It’s taken many years, but last year LIGO was finally made sensitive enough to detect the more powerful gravitational waves passing through it. The first detection, made on Sep. 14, 2015, was from two pretty beefy black holes, roughly 36 and 29 times the mass of the Sun. The event lasted two-tenths of a second.
In this second case, the entire detected event lasted about a full second. As the black holes fell in those last few kilometers, their fierce gravity swung them around faster and faster, causing the gravitational waves to increase in frequency and strength. When sound waves do this, you get a sharp, short “chirp,” and that’s what astronomers call this event, too.
The detection itself is pretty amazing. Automated software checks the signal from the LIGO setup and was the first to notice something was up. It alerted astronomers, who checked to make sure the signal was real. Part of that was looking at the signal from both facilities in Washington and Louisiana, and they both saw it (it was first seen in Louisiana, then in Washington 1.1 milliseconds later; that has to do with the speed of light and the angle to the merging black holes).
Note that in the plot above, a pair of up and down cycles is one orbit of the black holes around each other. These objects combined are 20 times the mass of our entire star, but they were whipping around each other hundreds of times per second before the end.
The exact shape of that signal is predicted by Einstein’s Theory of General Relativity. Using computers, the astronomers then generated literally millions of theoretical signals, comparing them to the observed one. They change the masses of the black holes, as well as many other parameters, giving them a range of values for their masses and distances. In the end, the masses found were 14.2 ± 8.3/3.7 (so as much as 8.3 more and 3.7 less) and 7.5 ± 2.3/2.3 times the mass of the Sun, and the distance roughly 1.4 billion light-years.
This means the black holes were probably created in the usual way. A long time ago, two very massive, hot stars were in orbit around each other. One blew up, expelling its outer layers, and its core collapsed to form a black hole. Sometime after that the second one blew, creating the other black hole. They would have orbited each other stably forever, but Einstein has something to say about that: As they moved, they emitted those gravitational waves. The emission was very weak at first, but it removed energy from the system, and the black holes spiraled every so slightly closer together. As they got closer they moved faster, were accelerated more, and emitted more waves. This was a positive feedback loop, and when they got close enough together, BLOOP! They merged.
The 14 and eight solar mass black holes combined to form a single black hole with 21 times the mass of the Sun.
Of course, 14 + 8 = 22. What happened to the missing mass? That mass was converted into the energy of gravitational waves.
I’m not going to lie to you: Just writing that gave me a chill down the back of neck.
That amount of energy is beyond staggering: It’s equivalent of all the energy the Sun emits over a period of about 15 trillion years. That’s a thousand times the lifetime of the Sun! Or, if you prefer, it’s about the same amount of energy emitted by a billion galaxies like ours over the same time interval as the merger.
And now you can see why astronomers are so excited by this. These are among the most energetic events in the Universe, and until last year we were completely blind to them.
The first event showed we could do it. This second event shows that the age of gravitational wave astronomy is truly here. Mind you, both events were detected just a few months after LIGO became sensitive enough to detect them; many more will be seen, and soon. As data are gathered, we’ll learn more about this entirely new field of astronomy, one completely divorced from the usual detection of electromagnetic waves—light. Certainly, conventional telescopes will help; it’s suspected there may be a brief flash of light accompanying the release of gravitational waves, but it’s not certain. And just on their own, gravitational waves yield a treasure of information.
This is an amazing event. Predicted by esoteric physics a century ago, detected by physics even older than that, we finally have the technology that allows us to hear the faint whispers the results from these deafening roars. And it will allow us understand the universe in a whole new way.
A Dying Star Metamorphoses Into a Butterfly
When a star dies, it can be lovely.
When a star dies with another nearby, it can be amazing.
The image above shows Hubble 12 (also called HB 12 for short), what astronomers call a planetary nebula, the gas and dust thrown off by a star as it ends its life. When the star runs out of fuel in its core needed to generate the energy it uses to sustain itself, the outer layers of the star can be thrown off in a series of winds, like a solar wind on steroids.
But HB 12 has an extra ingredient or two. One of them is that the star in the center isn’t one star, but two. They orbit each other pretty close together, their orbital velocities high. This can help shape the wind blown out by the one star that’s dying; it adds a component of centrifugal force. Most of the material flung out goes out along the orbital plane of the two stars, forming a disk. Other stuff hits this disk and flows up and away, forming the hourglass figure.
Another ingredient is the fact that HB 12 sits in a region of the galaxy thick with interstellar gas and dust. Some observations indicate there’s quite a bit of it surrounding the stars, and the wind is plowing into that material, which confines it. That may be why the edges of the shapes you see in the image are so well defined. It also makes the nebula denser, and therefore brighter; HB 12 has one of the highest “surface brightnesses” of any nebula—that means any given piece of it is pretty bright compared with the same size section of another nebula.
But there’s a lot more going on here. If you look at the inner nebula, the part that looks like a butterfly, you can see brighter rings going around the cone-shaped “wings” (reminding me of the old Rocketdyne F-1 engines used on the Saturn V rocket). Each one of these may have been due to a gust of wind from the star, an episodic hiccup that temporarily increased the amount of material blown out. Given the spacing in the rings, they probably occur every 50 years or so. So twice a century the star went through some sort of event that increased its outflow. It’s not clear what that event might be.
Those outer structures, though! What a mess. But if you look carefully, you see symmetry. For every U-shaped structure you see, there’s an upside-down U to match it. That’s because every time the star blows out material, it does so in both directions, up and down. That might be more clear in a grayscale version of the image:
The exact cause of all these structures has me scratching my head, though. The eye-shaped oval in particular is weird. I’d expect that to be an ellipse, a circle of expanding material seen at an angle (like looking at a water glass from an angle makes the circular opening appear like an ellipse). However, in this case it has sharper cusps on the left and right. That might simply be due to a weird perspective; the gas here is thin, and you can see through it, so you’re seeing the front and back side of the nebula on top of each other.
So that wide open structure on the outside is probably much like the inner, bright butterfly structure. Perhaps it’s just older and has had more time to spread out. If that’s the case, I see at least three such structures here, which hints that the dying star has had a lot of increased activity over the years.
And this I find particularly interesting: Just outside the central bright point marking the star’s position, you can see two parallel circular features, one just above and one just below the star. That reminds me very strongly of NGC 1514, another planetary nebula:
As I wrote then, such features aren’t well-understood. What shapes them, why are they on opposite sides of the star like that, why are they so bright? It’s not clear.
Actually, there’s a lot that’s not well known about this object. We’re not even sure of its distance! Various methods to measure that yield wildly different results; everything from 7,500 light-years to more than 25,000 light-years! I suspect it’s probably on the closer end of that range, but who knows?
Here’s another interesting thing: This nebula is young. Measuring the speed of the expansion of the features and then tracing that back,* the age of the nebula is probably more than 1,000 years. That’s consistent with what we know about such objects; the gas is thrown out pretty quickly, and the planetary nebula stage of a dying star lasts millennia at most. The expanding gas becomes too thin and too distant for the star to light up, and the nebula fades.
I love planetary nebulae; I studied them both for my master’s degree and Ph.D. Very little was known about them before the advent of digital cameras, they’re pretty faint and small. But now we have extremely sensitive detectors and telescopes like Hubble, capable of imaging their fantastic structures.
And one last thing: The images you see here of HB 12 were processed and constructed by Judy Schmidt, who likes to reprocess data from the Hubble Space Telescope and create beautiful images. Her work has been featured here on the blog many times, and you can also see her creations on her website and on her Flickr page. Follow her on Twitter to get the latest updates, too. We had a fun conversation about this nebula, and I hope she tackles more such objects in the future.
*It’s a bit like knowing how far you’ve driven knowing your speed and how long you’ve been on the road. If you know the size of the nebula and how quickly it’s expanding, working the math backwards gives you the age.
Will SpaceX Be on Its Way to Mars by 2018? Maybe. But That’s Not the Point.
In May, Elon Musk announced that SpaceX would be sending a Dragon capsule on its way to Mars by the end of 2018.
That’s pretty ambitious. After all, 2018 is soon.
But is it too soon? I wrote an article about Musk’s plan to go to Mars, and I still think SpaceX can do it. But can do it isn’t the same thing as will do it. The problems are essentially twofold: The hardware they’ll use to go to Mars (mostly the Falcon Heavy rocket and the upgraded Dragon capsule) is still untested, and the fact that, to coin a phrase, stuff happens. By that I mean the winds of chance: a launch delay, a wonky part that refuses to be diagnosed, a lawmaker who has a NASA rocket facility in their district and doesn’t want the competition … these can all add weeks or months to the countdown.
So when Taylor Quimby of the New Hampshire Public Radio show Word of Mouth called me to talk about it and settle a bet he had with his colleague Sam Evans-Brown, I tried to explain this all carefully.
In the end, the distinction I’m trying to make is that yes, SpaceX can get to Mars, and possibly even launch the mission before Dec. 31, 2018. But it seems to me, given the reality of the situation, it’s quite likely it’ll happen in 2019 or later.
Ask me again after the Falcon Heavy goes on its first voyage, and the upgraded Dragon is built and tested, too. Once SpaceX gets those up and running, well, the sky’s no longer the limit.
As I said in the interview, the real question is: Who will put humans on Mars first, NASA or SpaceX?
NASA’s plans to go to Mars are a bit vague but rely on the Space Launch System to do it (full disclosure: I’m not a big fan of SLS). Like the Falcon Heavy, SLS has not yet launched, and the first flight is planned for late 2018 (barring delays, of course). NASA doesn’t plan to have humans on board an SLS flight until at least 2023, with a Mars flight perhaps sometime “in the 2030s.” Musk recently announced he wants to put humans on Mars by 2024, another ambitious but potentially doable deadline. Even if delayed several years, SpaceX would have an edge over NASA.
The situation with SLS and Falcon Heavy is complex, and more than I want to dive into here; a longer, more thorough post will come where I lay out my current thoughts on it. But in the meantime, to be clear: The deadlines Musk has laid are ambitious but achievable, and even if they aren’t met, the ability of SpaceX to go to Mars and eventually put humans there should not be discounted.
It’s the way to bet.
Orlando: What Can You Do in the Face of Another Senseless Gun Tragedy?
On Sunday, the country woke up to another horrific crime: a mass shooting in Orlando, Florida. A man who legally purchased guns just days before walked into a gay night club and shot more than 100 people, killing 49.*
By now you’ve heard the story, read the articles, perhaps even listened to the president, sounding tired and at a loss after having to make a variant of this speech more than a dozen times since talking office.
There have been a lot of updates since that morning, and there will be more to come. Twitter was its usual self, both an excellent and abhorrent example of the good and the awful in humanity.
I don’t usually comment very much in social media about such things, mostly because it tends to erase subtlety and flatten layers of meaning. But like so many others, I couldn’t stand by, silent. So I composed a series of thoughts and laid them out on Twitter and Facebook.
Waking up to another mass shooting, another mass murder, in my country.— Phil Plait (@BadAstronomer) June 12, 2016
More than 50 gay people dead, their crime being who they were.— Phil Plait (@BadAstronomer) June 12, 2016
Appalled. Saddened. Sickened. Angry. But not shocked.— Phil Plait (@BadAstronomer) June 12, 2016
When fear, loathing, and disgust against entire groups of people are officially sponsored by the State, how can we be shocked?— Phil Plait (@BadAstronomer) June 12, 2016
The gay community has made some huge strides in the past few years, with love mostly winning out over bigotry ... in the legal system. But that undercurrent of homophobia, especially in state governments, is still there. And we've seen this ugliness still bubbling up to the surface ...
"It's too soon to politicize a tragedy". Bull. It's too late. It's always too late. People are dying because this has always been political.— Phil Plait (@BadAstronomer) June 12, 2016
Senseless anti-LGBTQ laws have been cynically used this whole election cycle for one reason: Promote fear.— Phil Plait (@BadAstronomer) June 12, 2016
By this I mean the ridiculous transgender bathroom laws that are getting so much airtime (and which, incidentally, are unconstitutional). Given that there's never been a recorded case of a transgender person attacking a child in a public restroom, the purpose behind these laws, so heavily promoted by state-level GOP politicians, is obvious: scare people, and get them to the voting booths come November.
And many politicians send their "thoughts and prayers", but refuse to even discuss any action on guns.— Phil Plait (@BadAstronomer) June 12, 2016
Of course people want to send their thoughts and express their grief; that's natural and very human. But it's cynically hypocritical when politicians do it and nothing else. Congress made it extremely difficult for the Centers for Disease Control and Prevention to even study the effects of gun violence. Seeing all the NRA-funded lawmakers tweeting their "thoughts and prayers" was particularly galling.
I know there's no easy answer to this. But I also know *no* answer will found by doing nothing, allowing no research, taking no action.— Phil Plait (@BadAstronomer) June 12, 2016
20 children were killed in a school and no action was taken. A US Representative was shot in the head and no action was taken.— Phil Plait (@BadAstronomer) June 12, 2016
We have an election coming up soon. I'm asking you to take action. Vote.— Phil Plait (@BadAstronomer) June 12, 2016
And contact your state and federal officials. Tell them how you feel: https://t.co/yMxq16DgDe— Phil Plait (@BadAstronomer) June 12, 2016
Take special note of how politicians reacted after the shooting. Watch President Obama's calm speech again. Note how he calls this event a shooting and specifically mentions the LGBTQ community.
Contrast that with Donald Trump's response, who made a series of appalling tweets about the event, then released an unhinged statement about "radical Islam," saying Obama should step down, and then gave an interview on Fox strongly implying conspiracy ideations about the president.
Contrast that with Hillary Clinton's response, which was far more measured and reality-based. She understood that information was (and is) still lacking, and going off like tainted batch of fireworks not only is the wrong thing to do, but it actually makes things worse. As my Slate colleague William Saletan wrote in the link above, hate against Muslims is what ISIS wants. And also note that, like the president but unlike Trump, Clinton didn't hesitate to talk about guns in her reaction. She addressed the actual situation, not some fantasy spun out of conspiracies and hatred.
Who sounded more presidential?
Speaking of action, if you're in Orlando here's how you can help: https://t.co/caWK9HmF5k— Phil Plait (@BadAstronomer) June 12, 2016
Also, if you want to donate money to help, Equality Florida, the state's (LGBTQ) civil rights organization, has set up donation page on GoFundMe. They also have information there about other ways to help.
And remember: Individuals can be awful. But humans, as a whole, are good. https://t.co/yBZgzrCtO0— Phil Plait (@BadAstronomer) June 12, 2016
Not long after I posted those tweets, my friends at STARtorialist posted the image of a heart I used at the top of this article, and it really struck me, so I retweeted it.
This is lovely. The colors of the Sun shine on all of us. https://t.co/DuzCdUVhN7— Phil Plait (@BadAstronomer) June 12, 2016
Inside the heart is the spectrum of the Sun, composed of light from all of its constituents inside it and mixed together, shining down on Earth. If there’s a metaphor there, feel free to ponder it.
So, to reiterate, how to help:
- Donate money
- Donate blood
- Contact your representatives at the state and federal level and talk to them about rational gun control measures
*Update, June 13, 2016: This post has been updated to more accurately reflect the death toll from Sunday's shooting. Earlier reports of 50 victims included the shooter, but it’s standard practice not to list the perpetrator as a victim in these situations.