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Northern Sky

East Bay Moon Crescent/Photo by Stephan Hoglund

Deane Morrison is a science writer at the University of Minnesota. She authors the Minnesota Starwatch column, and contributes to WTIP bi-weekly on the Monday North Shore Morning program through "Northern Sky," where she shares what's happening with stars, planets and more.


What's On:
Star map March 2019 submitted by D.Morrison

Northern Sky: March 16-29, 2019

NORTHERN SKY – By Deane Morrison  

March 16-29 2019

We’re now deep into spring equinox time, when the sun climbs fastest through the northern sky. The equinox happens at 4:58 p.m. on March 20, and Grand Marais gains three minutes and 28 seconds of daylight per day for two weeks around that date. But Anchorage, Alaska gains five minutes and 44 seconds, while in Trondheim, Norway, they’re gaining six minutes and 19 seconds. Trondheim gets more than an hour of extra daylight just during the 10 days straddling the equinox.
These ultra-rapid changes shouldn’t be too surprising. For example, in Trondheim, the day length goes from about four and a half hours in December to about twenty and a half in June. When the day length has to increase that much in just six months, it’s going to change pretty fast. And it’s fastest in March because that’s when the sun moves northward most rapidly.
At the equinox, neither pole is pointing toward the sun, and the day length is the same, theoretically, all over the planet. We actually get slightly more than 12 hours of daylight on the equinoxes because Earth’s atmosphere is a gigantic lens that allows us to see the sun for a few minutes before it rises and after it sets.
The equinoxes are also times of switchover. During the winter, the farther north you go, the shorter the day length. After the spring equinox, it’s the other way around, and as you go north, the day length increases.
All this is due to Earth orbiting around the sun while being tilted on its axis. That tilt doesn’t change during the course of a year. The North Pole always points to the same spot in the sky, near the North Star, and it’s our orbital motion that makes it point toward or away from the sun, or neither, depending on Earth’s position.
If that’s hard to visualize, get an apple and face a wall. Tilt the apple a little so that the stem—the apple’s north pole—points somewhat upward and toward the wall. Then, without spinning or pivoting the apple in any way, move it counterclockwise in a circle and imagine the sun in the center. Move your arm horizontally, as if stirring a pot, keeping the apple pointed toward that same wall. When it’s closest to you, the apple tilts toward the sun, like Earth at the northern summer solstice. When it’s farthest from you, it tilts away from the sun. That’s the winter solstice. At the midway points it tilts neither toward nor away from the sun, and those are the equinoxes.
Okay. In the sky. Jupiter is well up in the south in the predawn hour, Saturn is much dimmer and off to the lower left of Jupiter, and Venus makes it over the eastern horizon just as the sun’s rays start to wash everything out. 
In the evening, Mars is still up in the west after nightfall. It’s been kind of lonely, but some visitors are on the way. The Pleiades star cluster and the bright star Aldebaran, the eye of Taurus, the bull, are moving closer to Mars every night. Best viewing starts the 22nd of March, at about 8:30 or 9 o’clock, when the sky will be dark but the moon won’t be up yet.
March’s full moon comes right after the equinox, at 8:43 p.m. on the 20th. The moon will be just a day past perigee, its closest approach to Earth in a lunar cycle, and that means we get our third supermoon in a row. This one rises over Grand Marais at 6:52 p.m., less than two hours before fullness, so it’ll come up very round as well as very big.


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Northern Sky: February 16, 2019

NORTHERN SKY – Deane Morrison
February 16 – March 1, 2019

In the second half of February, most of the astronomical action is still in the morning sky.
Venus is heading toward the sunrise while Saturn is climbing up away from it. Between the 17th and the 19th, the two planets pass each other. They come closest on the 18th, when Saturn will be one degree, or two moon widths, below Venus, which is by far the brighter planet. For the rest of the month, the distance between them widens, and by March 1 they’ll be 10 degrees apart.
Saturn is following Jupiter, and now these two outer planets are rising earlier every day as they sail westward across the morning sky. Jupiter is brighter than Saturn, but in case you’re not sure which object is which, a fat crescent moon will be right above Jupiter on February 27th. A thinner crescent will be near Saturn on March 1, and Venus on March 2.
What makes the outer planets move westward across the sky—and the stars, too—is Earth’s orbital motion. But the outer planets’ own orbital motion makes them drift eastward with respect to the background of stars. Jupiter drifts eastward faster than Saturn, and now, that motion is carrying it toward Saturn. Late next year, Jupiter will pass Saturn—and very closely, which will be a lot of fun to watch. 
In the evening sky, Mars is still in the west after nightfall. It’s the vlodrdy of the outer planets, and moves the most rapidly eastward against the stars. It is dropping westward, but so slowly that it seems to be holding its own as the stars rush past it. Right now, that’s what the group of bright winter constellations is getting ready to do.
One of those constellations is Gemini, the twins. Its two brightest stars are Castor and Pollux, the heads of the twins. Gemini’s other stars are dimmer, but still, this constellation looks like what it’s supposed to be: two human figures. Pollux is lower and slightly brighter than Castor. Pollux is a large star with at least one large exoplanet, but Castor, not to be outdone, is a system of six stars. It has two main stars that orbit each other.
Each is a little bigger than the sun, and each has a small companion called a red dwarf star. And associated with this system is a pair of red dwarf stars that orbit each other and also appear to orbit the two main stars, albeit very slowly. Multistar systems are common, and needless to say, they can get complicated.
On the 16th, a bright waxing moon will be near the Gemini twins. Two nights later it’ll be near the backward question mark of stars that outlines the head of Leo, the lion. Early the next morning, at 3:03 a.m. on February 19th, the moon reaches perigee, its closest approach to Earth in this lunar cycle. Not quite seven hours later, it becomes full. Because it will be so close to us, this full moon qualifies as another supermoon, so it’ll be especially large and bright.
There’s just one little fly in the ointment, a common one when full moons come in the morning. On that day, the 19th, the moon sets over Grand Marais at 7:18 a.m.—a couple of hours before fullness. So if you want to see a supermoon at its biggest, roundest and brightest, go outside at least half an hour before moonset, which would mean by 6:45 a.m. And you’ll need a clear view of the western horizon. Or, if you’d rather watch a super moonrise, try the one right after full moon, on the evening of the 19th. It will still be pretty big and beautiful.


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Northern Sky: January 19 - February 1, 2019


Deane Morrison         

 As January heads into the home stretch, the morning show, starring Venus and Jupiter, is still going strong. Brilliant Venus has begun a descent into the sunrise, as it does whenever it’s getting ready for another trip behind the sun. Meanwhile, Earth is gaining on Jupiter in the orbital race, and this makes Jupiter climb through the morning sky. On Tuesday, January 22nd, Jupiter slides past Venus on its way up. At the end of the month, Jupiter and Venus will be about nine degrees apart.

 Also on January 31st, you’ll see a waning crescent moon close to Venus. And, if skies are dark, the red star Antares, in Scorpius, off to the right of Jupiter, at about the same distance as Venus. On February 1st, a thinner crescent moon appears below Venus. If you imagine a line from Venus to the moon and extend it down toward the horizon, you may spot Saturn. Earth is catching up to Saturn, too, so the ringed planet is also on its way up in the morning.

But the real show happens in the evening sky on the night of Sunday, January 20, when we get a total eclipse of a supermoon. This full moon deserves that name because it’ll be less than 24 hours from perigee, its closest approach to Earth in a lunar cycle. When the moon rises over Grand Marais—at 4:17 p.m.—you may notice that it’s bigger and brighter than your average full moon. Now, here is a play by play of the eclipse. 

 At 9:34 p.m. the moon’s leading edge makes contact with the Earth’s umbra, or dark inner shadow,  and the shadow starts to spread.

 At 10:41 p.m. totality begins. The moon is now completely engulfed in the umbra. An observer on the moon would see a total solar eclipse, due to Earth blotting out the sun.  The observer may also see a ring of fire around the Earth. The red ring comes from Earth’s atmosphere bending red light from sunsets and sunrises into the umbra, and some of it hits the moon. From our point of view, this light often turns the moon’s face reddish—what we call a blood moon—during a total lunar eclipse.

 At 11:12 p.m. the moon passes closest to the center of the umbra, and it’ll be in deepest shadow.

At 11:43 p.m. totality ends. At this point, the leading edge of the moon breaks out of the umbra.

At 12:51 a.m. on January 21, the moon frees itself from the last vestiges of umbra and the show is over.

 During the height of a lunar eclipse, if you can see the darkened moon or at least remember where it was with respect to the stars when it disappeared, you can use it to find astronomical objects that otherwise would have been washed out by moonlight. This time, you may find the dim but lovely Beehive star cluster. Look to the lower left of the moon, about 12 moon widths away.

 The Beehive is a feature of Cancer, the crab. It’s between Gemini, one of the winter constellations, and Leo, the quintessential spring constellation. To the naked eye it’s just a fuzzy spot, but with binoculars, you can make out the stars. In 1609 Galileo was the first to observe the Beehive telescopically. He counted 36 stars, but there are actually more like a thousand. The Beehive’s Latin name is Praesepe, or manger. The cluster is framed by two stars called Aselli, which are donkeys feeding at the manger. The Beehive’s stars were all born in the same stellar nursery and have stayed together for the approximately 600 million years of their lifetime.


Northern Sky: January 5-18, 2019

Deane Morrison's "Northern Sky"  -  January 5 - 18, 2019

Early and mid-January are great times for star watching because skies are dark, and the winter constellations are bright. It may get a little nippy, but you don’t have to be outside very early, very late, or very long to see the main features.
The morning sky is especially good right now because the sun is rising about as late as it ever does. In the southeast, Venus and Jupiter are drawing closer every day, getting ready to pass each other on the 22nd. Venus is the brighter and, for now, the higher of the two. And to complete the predawn picture, the bright red star Antares, the heart of Scorpius, is just to the west of Jupiter.
In the evening, the winter constellations are up in the southeast after nightfall. They’re grouped pretty close together, so if you’re not familiar with them, you really should have a star chart to sort them out. But the most recognizable constellation, Orion, is easy to find because of the three stars that form his belt. 
Hanging from Orion’s belt is a line of stars that represent his sword. About halfway down the sword, binoculars will give you a glimpse of the sprawling and colorful Orion Nebula. The Orion Nebula is an immense cloud of gas and dust where new stars are forming. It’s about 1300 light-years away, and an estimated 24 light-years wide. Orion is also home to the famous Horsehead Nebula, which you need a telescope to see. But you can find lots of images of the Horsehead Nebula, and the Orion Nebula, online.
Orion’s left foot is Rigel, a blue-white star. Rigel and Betelgeuse, the red star at Orion’s right shoulder, are the brightest stars in Orion and among the top 10 in the whole sky. Rigel is a multiple star system, and overall, it’s estimated to be 40,000 times brighter than the sun. Betelgeuse is a gigantic star, estimated at 1,000 times the width of the sun. It’s less than 10 million years old—a mere child—but it’s aged rapidly and is now close to the end of its life. It’s expected to die in a spectacular supernova explosion. That may not happen for a million years, or it could blow up tomorrow.
In astronomy news, on New Year’s Day NASA announced that its New Horizons spacecraft, which gained fame by sending back stunning images from Pluto, has just completed what its principal investigator calls “the farthest exploration in the history of humankind.” It performed a flyby of an object in the Kuiper Belt, a doughnut-shaped ring of icy worlds beyond the orbit of Neptune. The object is called Ultima Thule, and it’s 4 billion miles away. The first pictures have just been released, and Ultima Thule looks, in the words of mission scientists, like a reddish snowman, something they’re now sure is the result of two spherical bodies that came together and stuck. Mission headquarters at Johns Hopkins University’s Applied Physics Laboratory says, “the two spheres likely joined as early as 99 percent of the way back to the formation of the solar system, colliding no faster than two cars in a fender bender.”
Ultima Thule is 19 miles long, and its two spheres are 12 and 9 miles wide. Scientists hope this object will clear up some mysteries about how our solar system formed. They want to know, for example, how small objects came together to form larger ones, and how they’ve been bombarded by meteor-like objects, although no impact craters are obvious on Ultima Thule.
Mark your calendars for Sunday, January 20th, when we’ll have a total eclipse of the moon. The show starts at 9:34 p.m., and I’ll have more on that in the next broadcast. 

Deane is a science writer at the University of Minnesota.
She authors the Minnesota Starwatch column which can be found on the University of Minnesota website at


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Northern Sky: November 24 - December 7 2018

Northern Sky by Deane Morrison
November 24 - December 7, 2018

Deane Morrison is a science writer at the University of Minnesota.        
She authors the Minnesota Starwatch column, and in this feature
she shares what there is to see in the night sky in our region.
Deane's column “Minnesota Starwatch” can be
found on the University of Minnesota website at 


November Sky Map

Northern Sky: November 10 - 23, 2018

NORTHERN SKY – Deane Morrison
November 10 – 23, 2018
Now that we’re back on standard time, the stars come out earlier. That’s good for watching the evening sky. But the morning sun also comes up earlier than it did on daylight time. It rose over Grand Marais at 7:49 a.m. right before the switchover, and it won’t rise that late again till the second half of December. So for now, everybody will have to get out earlier to see the morning show.
The star of that show is our old friend Venus. It’s climbing over the eastern horizon as it emerges from a trip between Earth and the sun, and so it’s relatively close and very bright. It starts out as a thin crescent, and through a small telescope or even a pair of very strong and steady binoculars, you can see the crescent getting thicker as the days go by. The star above Venus is Spica, in Virgo. If you go out on only one day, try the 14th, when the planet and the star will be at their minimum distance, just over two moon widths apart. Look about an hour before sunrise.
Jupiter will join Venus next month, but right now it's in the process of falling out of the evening sky and getting lost in the sunset. And Saturn is right behind it. In both cases, Earth is going around the sun, leaving those planets behind. In the east, the bright winter constellations are making their annual entrance. However, only a few, like the Pleiades star cluster and Taurus, the bull, are up right after nightfall. If you’re out at that time and looking for something new, you may want to see if you can find some double stars that are up in early evening. Binoculars are highly recommended here.
The first double star is easy: it’s at the bend of the Big Dipper's handle. The Big Dipper is now sitting pretty much upright, just above the northern horizon. The double star in the handle is well known, and you can see it without binoculars if your vision is good. While you’re there, you can use the Big Dipper to find Polaris, the north star. The two stars on the bowl of the Big Dipper that are farthest from the handle point toward the north star. Also, try to find the whole Little Dipper. Polaris is at the free end of its handle, and keep in mind that the two "bowl" stars nearest the handle are pretty dim. The second double star is in Taurus. To recap, it's in the east after nightfall. Find the face of the bull, with a star chart if you need one. You'll see the bright star Aldebaran next to the Hyades star cluster, which is shaped like a V. Follow the line of stars from Aldebaran toward the point of the V, and you'll see the double star. Binoculars will help. Use them again on the Pleiades, which appear to the naked eye as a fuzzy patch above Aldebaran. The third double star is the most challenging. Find Vega, a brilliant star in the west, and look just above it for a tight doublet of stars. You’ll definitely need binoculars for that one. And you may want to postpone your search for double stars until after full moon because a waxing or full moon can wash out the dimmer stars in the early-evening sky.
Our full moon arrives at 11:39 p.m. on the 22nd, which is Thanksgiving Day. It rises over Grand Marais at 4:28 that afternoon, and for my money, that's when it will be most beautiful. At nightfall, it will be between and just west of Aldebaran and the Hyades, below, and the Pleiades above. 



Northern Sky: Oct 13 - 28, 2018

Northern Sky - by Deane Morrison
October 13 - 28, 2018

Deane Morrison is a science writer at the University of Minnesota.        
She authors the Minnesota Starwatch column, and in this feature, she shares what there is to see in the night sky in our region.

Deane Morrison’s column “Minnesota Starwatch” can be found on the University of Minnesota website at 




Northern Sky: Sept 15 - 28

Norther Sky – by Deane Morrison  -  Sept. 15-28 2018

During the last two weeks of September, we have bright planets in the evening and a couple of regularly scheduled astronomical events.
If you face south 40 to 45 minutes after sunset, you’ll see Mars fairly low and still quite bright. Turning a bit westward, you’ll see the Teapot of Sagittarius, with Saturn above it. Next, even lower than Mars, there’s Antares, the red heart of Scorpius. Finally, low in the southwest, we have Jupiter. You probably won’t see Venus, though, especially later in the month, because it’s dropping into the sunset on its next trip between Earth and the sun. That trip also takes it, officially, from the evening to the morning sky.
As for stars, the Summer Triangle of bright stars is high in the south after nightfall. And in the west, the brilliant star Arcturus is still pulling its kite-shaped constellation, Bootes the herdsman, down toward the horizon. You might want to compare Arcturus with Vega, the brightest star in the Triangle and see if you can tell that Arcturus is ever so slightly brighter.
Now, about those scheduled events. First is the fall equinox. It arrives at 8:54 p.m. on Saturday the 22nd. At that point an observer from space would see the sun poised over the equator and Earth lighted from pole to pole. The equinox is also a crossover time of sorts. In spring and summer, the Northern Hemisphere tilts toward the sun, and the farther north you go, the longer the day length. But after the fall equinox, it tilts away from the sun and the days get shorter as you go north.
And, this is the time of year when the Northern Hemisphere is most rapidly shifting its tilt away from the sun. Which brings us to the second scheduled event: the harvest moon. Some say the harvest moon is the full moon closest to the fall equinox, others say it’s the first full moon after the equinox. This one qualifies on both counts. The full harvest moon, on Monday, September 24, rises over Grand Marais at 7:12 p.m., which is just two hours and 40 minutes before perfect fullness, so it’ll be nice and round.
But the harvest moon is more than just a name. Here’s how it goes. The full moon occupies a position on the other side of Earth from the sun—so it’s opposite the sun in the sky. Therefore, when we’re tilting most rapidly away from the sun, making it move south and rise later each day, we’re tilting most rapidly toward the full and nearly full moons and making them move north and rise relatively sooner each day.
Note that’s relatively sooner. The moon’s orbit makes it rise later from one day to the next; on average, around 50 minutes later. But around the time of the fall equinox, that interval gets slashed because of the moon’s rapid movement up through the northern sky. This year, for a few days centered on September 24, moonrise comes only 24 minutes later each night. That’s the harvest moon effect.
It’s fortunate for farmers, because it means that near full moon time, farmers harvesting crops don’t have to wait as long for a bright moon to come up and light their fields.
Finally, the rapid change in Earth’s tilt is sapping the day length faster than ever at this time of year, which I’m sure comes as no surprise. We’re losing around three minutes of daylight every day. But, I keep reminding myself, people in places like Alaska and Iceland have to put up with losses of six minutes a day.




Northern Sky: Sept 1 - 14, 2018

Deane Morrison is a science writer at the University of Minnesota.
She authors the Minnesota Starwatch column which can be found on the University of Minnesota website at

She tells us what to look for in the night sky in our region.

NORTHERN SKY – by Deane Morrison                      September 1-14 2018
Now that September’s here, the skies are getting seriously dark. Venus is still in the west, but it’s sinking fast. It’s also coming toward us, on the way to zipping between Earth and the sun. If you have a small telescope, you can watch it go through phases. Venus appears as a fat crescent now, but the crescent gets longer and thinner as September goes by. 
Somewhat high in the west, we have the brilliant star Arcturus. At this time of year, I like to watch Arcturus slowly fall through the sky from night to night. Arcturus is the brightest star in Bootes, the herdsman, a kite-shaped constellation, and it’s right where the tail of the kite would attach to the sail. So as Arcturus and Bootes drop down toward the horizon, it always seems as if this heavy star is dragging the kite down with it.
Actually, Arcturus is falling on a grander scale. It doesn’t orbit horizontally around in the disk of the Milky Way like the sun. Instead, its orbit slices right through the galactic disk. But Arcturus isn’t plunging through the disk by itself; it has more than four dozen stellar companions. Together the group is called the Arcturus stream. One caution: Don’t confuse Arcturus with Jupiter, which is bright but rather low in the southwest after nightfall.
Mars and Saturn come out low in the south. Mars is east of Saturn; it’s also brighter and, of course, redder than Saturn. Between the two planets is the Teapot of Sagittarius. Above all this, we have the large Summer Triangle of bright stars. The lowest is Altair, in Aquila, the eagle. It’s pretty much right above Mars. Looking up and a little west of Altair, you’ll see the brightest star in the Triangle. That’s Vega, in Lyra, the lyre of Orpheus. Note the parallelogram of stars below Vega; they outline the lyre and they make a really beautiful sight through binoculars. East of Vega is the third star, Deneb, in Cygnus the swan. Deneb also marks the head of the Northern Cross, a notable feature of Cygnus.
The Summer Triangle is a rich area of sky to explore, with both the naked eye and binoculars. And a star chart, if it’s your first time. Look above Altair—again, that’s the lowest star in the Triangle—and try to make out a short and skinny constellation called Sagitta, the arrow. Then try immediately northwest of Sagitta’s feathers and see if you can find the dim but astonishingly realistic Coathanger hanging upside-down. You’ll need those binoculars to make it out. Finally, look to the east-northeast of Altair for Delphinus, the dolphin, which seems to be happily leaping into a dark sea.
The moon is new on September 9.  For a couple days before then, there’s a thin old crescent moon in the east before dawn. On Saturday, the 8th, the moon rises close to Regulus, the brightest star in Leo. Then comes Mercury, and the sun right behind it. Look about 40 minutes before sunrise, and good luck seeing all three of the other objects when the sun is so close.
And, starting on the 8th, try looking for the elusive zodiacal light in the east, just before the sky starts to get light. The zodiacal light appears as a broad but faint glow along the sun’s path and it comes from sunlight reflecting off the dust that extends far out into space in the plane of the solar system. If you don’t find the zodiacal light on the 8th, the following two weeks will also be good times to look, and the moon won’t interfere with your view of the morning sky. 




Northern Sky: August 18 - 31, 2018

NORTHERN SKY – Deane Morrison       Aug. 18-31 2018

At this time of year, the stars and planets have started coming out noticeably earlier. Venus is sinking, but still bright, in the west after sunset. The bright star Spica, in Virgo, is off to the left--our left--of Venus in midmonth. Spica is also dropping toward the western horizon, and it crosses paths with Venus on Friday the 31st. That evening, If you catch them when the sky's dark enough but they haven’t set yet, you’ll see Spica about two and a half moon widths above Venus.
Moving east, we have Jupiter, always bright. East of Jupiter and low in the sky is Scorpius, with Antares, the gigantic red star at the heart of the scorpion. Moving east again, we have the lovely Teapot of Sagittarius with Saturn shining above it, and finally Mars. Mars, Venus and Jupiter outshine all the stars, and Mars still outshines Jupiter. But Mars is fading as Earth leaves it behind in the orbital race, and soon Jupiter will reclaim its mantle as the brightest of the outer planets.
August's full moon arrives at 6:56 a.m. on Sunday, the 26th. However, the moon sets at 6:07 a.m. that day, so to see it you could go out around 5:30 a.m., or look for it the night before or the night after.
In astronomy news, you may have heard that on Sunday, August 12, NASA launched the Parker Solar Probe, an ambitious mission to the one star we can study up close. Parker will fly through the sun’s corona—its outer atmosphere—passing closer to the sun than any previous mission, and University of Minnesota space physicists play an essential role in it. Here’s the scoop.
It’s been known for decades that when subatomic particles escape from the sun’s surface their temperature is about 10,000 degrees Fahrenheit. But when they pass through the corona, they get heated to a few million degrees.
Scientists have debated how the corona heats these particles so intensely. And also, how the corona accelerates them and spews them out in a torrent of particles that barrels through space at up to a million miles per hour. This stream of particles bathes the solar system and is known as the solar wind.
Earth’s magnetic field intercepts the solar wind and shields us against it. When it collides with Earth’s magnetic bubble, it can lead to spectacular auroras. But when it’s fierce, the solar wind can knock out power grids, as it did in Quebec in 1989.
Whatever in the corona is heating and accelerating these particles has to be electric and magnetic fields, because that’s all there is. The debate is about the details. The Parker spacecraft carries an instrument, designed by U of M researchers, to study the corona’s electric and magnetic fields and particles. This data will help settle the debate and make it easier to predict the heaviest gusts of the solar wind and take precautions to protect power grids.
How close will Parker get to the sun? If Earth and the sun were at opposite goal lines on a football field, the closest any spacecraft has come is the sun’s 29-yard line. But Parker will zip inside the 4-yard line, less than four million miles from the sun. NASA has dreamed of such a mission for 50 years, but the technology took time to develop. For example, engineers had to design a heat shield that’s capable of deflecting temperatures high enough to melt steel. Also, the Parker Solar Probe must, by itself, adjust its orientation to keep its heat shield between the spacecraft and the sun as it hurtles through its tightest loop around the sun at more than 400,000 miles per hour.