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52768 (1998 OR2)
On Wednesday morning at 5:56 a.m. (New York Time), the world will receive a reminder that things could always be a lot worse when a 2 kilometer (1.2 mile) asteroid zips by Earth at 31319 kilometers per hour (19,461 miles per hour). The great boulder goes by the not-very-lovely name 52768 (1998 OR2). It was discovered in 1998 by NASA’s Center for Near-Earth Object Studies, a program established to protect the denizens of Earth from possible space collisions (although our current terrestrial troubles suggest we may need to get our act together a bit better if we ever hope to, you know, actually do anything if one of these things comes straight towards us).
“But I voted to make dinosaurs great again!”
Fortunately during this pass-by, the asteroid will be a comfortable 6.3 million kilometers (3.9 million miles) away. That sounds disturbingly close, but it is really 16 times farther than the moon. Astronomers are carefully measuring the fly-by though, in order to learn what they can about asteroids, and because 52768 (1998 OR2) will be back…and next time it will be much closer. In 2079 it will probably be 3.5 times closer than it is this time, so mark your calendars for that: it might be a bit more exciting than this time around.
I have been trying to spruce up my online presence by building some new web pages (more about that soon) and by fixing the site I already have which everybody loves [crickets], um, which is to say Ferrebeekeeper! Unfortunately trying new things doesn’t always work…so kindly forgive me if yesterday’s post looks a bit peculiar. We will work with the web guru to get it all taken care of. In the mean time, speaking of experimenting with new things, let’s check back in on JAXA spaceship Hayabusa2.
Artist’s conception of Hayabusa2 touching down on Ryugu
When last we checked in with Hayabusa2, the Japanese spaceprobe had entered orbit around Asteroid Ryugu (a carbonaceous near-Earth asteroid, which is believed to be composed of pristine materials left over from the dawn of the solar system). Hayabusa2 was deploying tiny 1.1 kilograms (2.4 pounds) hopping droids to jump around the ancient ball of rock and snow and learn whatever they could. These robots would be followed by a larger robot probe, Mascot, which would study the asteroid in depth before Hayabusa2’s glorious showstopping signature move–a descent to the surface in order to fire a projectile into the asteroid (in order to collect an asteroid sample). That’s right: while Americans have been utterly transfixed by the bloviations of our felonious leader, the Japanese have dispatched a spacefaring robot to drop hopping mechanized lice on a primeval space snowball and then to pop a cap in it! Respect to the Land of the Rising Sun!
The probe arrived in perfect condition back in September of 2018, but the next phase of the mission got off to a rocky start…literally! JAXA expected Ryugu to be covered with fine powder, but it was covered with jagged rocks. The tiny hopping bots MINERVA-II1 A and B were really meant to test the conditions for MASCOT, a shoebox like robot-probe with real scientific instruments. On a prior mission these hopping probes were too enthusiastic and, after a single touchdown, they hopped magnificently but suicidally into the infinite void (presumably yelling inaudible robot slogans of honor). Although conditions on Ryugu were not as expected, the second generation Minervabots did a better job this time: they delivered the necessary telemetry, astrionics, and surface conditions to bring the mission to the next phase. Mascot was duly dispatched back in October and it operated faultlessly for 17 hours before its battery ran out and the active phase of its mission ended. [As an aside, I am finding it challenging to describe all of the things happening on a planetoid inhabited entirely by various sorts of robots]
Animation of Mascot probe hopping around Ryugu…such balletic grace!
On February 22nd 2019, the Hayabusa2 spacecraft descended to the surface of the asteroid and physically collected a substantial sample of the regolith by shooting the asteroid with a small projectile. You can watch the video of the brief encounter here. There are a lot of pebbles and shards flying around, but apparently the craft was fine and is now back in orbit while the ground crew looks for a final site to sample in April.
The Surface of Ryugu as imaged by a robot probe (JAXA)
This mission is super exciting, but the precious samples aren’t home yet. We will keep you updated here on Ferrebeekeeper (and we will keep working on our own tech project of building a better site).
Congratulations to the Japanese Space Agency! On Friday morning (EST) the Japanese space probe Hayabusa2 dropped two adorable little hopping rover bots (“hoppers”? “hop-overs”? “hop-bots”? um, we’ll work on it…) onto the surface of Asteroid Ryugu. The spacecraft arrived at the near-Earth asteroid back in June when the sort-of-octahedral space rock was passing near to our home planet. The twin “MinervaII” probes (“Micro Nano Experimental Robot Vehicle for Asteroid”) are 18 centimeter (7 inch) disks which weigh 1.1 kilograms (2.4 pounds) each. Making use of the asteroid’s exceedingly low gravity, the tiny robots will hop to their location and deliver readings about the composition of the ancient icy rock, which will hopefully provide insight into the formation of the solar system. Additionally, more stirring action is on the way in October when Hayabusa II will deliver a larger lander (named Mascot!) and then a third Minerva lander. This flurry of activity is in preparation to collect asteroid material which will be returned to Earth!
Hopefully….the MinervaII probes are (unsurprisingly) the second in a line of Minerva probes. The first Minerva hopping robot met an inglorious fate during the first Hayabusa mission to the asteroid Itokawa in 2005. That (smaller) Minerva rover was deployed a bit early and hopped ignominiously into the void of space. Sadly I don’t have pictures, but imagine a hockey puck falling into infinite blackness.
I will follow up with more news about this mission as it becomes available, but for now let us celebrate!
Oumuamua is an asteroid which came from beyond the solar system. Perhaps it was ejected from a star system in the Carina–Columba association (which is not an Italian fraternal organization but rather a vast nebula by Eta Carinae about 100 parsecs) around 50 to 100 million years ago, but its age and point of origin are unknown. It is whipping past the sun and then back into the vast darkness between the stars at a prodigious velocity (apparently it was traveling through interstellar space at something like 26 kilometers per second (58,000 miles per hour). The object, which measures between 100 and 800 meters (300 to 2500 feet), was initially classified as a comet, but its speed, its orbital eccentricity, and its bizarre shape–which is like an icicle or a shard–caused astronomers to realize it was deeply strange interloper from beyond.
The object has been closely observed by many of the Earth’s great observatories and it is apparently a dark red—which is caused by cosmic radiation striking it for 100s of millions of years (Kuiper belt objects have similar coloration). It is traveling far too fast for any existing human craft too reach (although we may be able to build such crafts in the near future), however scientists are assessing it for traces of life or civilization by means of radio telescopy. It will be out by Jupiter next year and far beyond are kin soon after that, but scientists have learned a great deal from the visit. Additionally they speculate that other such objects come through the solar system at the rate of one or two per year (which does not seem like a lot considering how large the solar system is). We are lucky to have spotted this shard, but its catastrophic shape makes one speculate that there is a lot about planetary formation (and destruction) which we don’t know yet.
M-type asteroids are high albedo (i.e shiny) asteroids made partially or mostly of metal. Of all of M-type asteroids currently known in the solar system, 16 Psyche is the most massive. It is a hunk of iron and nickel (and other heavy metals?) which has a diameter of 250 kilometers. Psyche orbits the sun between Mars and Jupiter and is believed to be the exposed core of a planet approximately the size of Mars which was obliterated by a catastrophic impact. The asteroid is named after the intrepid mortal who found love and ultimately apotheosis in an “Eyes Wide Shut” type Greek myth of great suspense, horror, and beauty.
Are you curious to know more about 16 Psyche based on this description? I certainly hope you are, because NASA has just announced future missions for the 2020s and 16 Psyche is on the list. As currently conceived, the Psyche exploration mission will send a robot probe powered by solar electric propulsion out to the obliterated core to examine the planetoid. The probe will be equipped with a magnetometer and a gamma-ray spectrometer to find out more about the composition and history of the enigmatic relic.
Of course other long term aspects of the mission are of interest as well. Although we have not yet mastered nuclear fusion, safe comprehensive control of such boundless energy is probably only 20 years or so away [winky icon]. What if humankind had sophisticated manufacturing robots and near infinite energy? In such circumstances 8 million cubic kilometers of steel might come in very handy indeed. So far the good news keeps rolling in for 2017. This Psyche mission can’t happen fast enough for my taste.
Today (June 30th) is asteroid day. For this auspicious (yet anxious-making) holiday, I have been saving two asteroid-related miniature stories ripped from the headlines.
First, we return to the dwarf planet Ceres, the largest object in the asteroid belt. We need to revisit the bright spots upon the dwarf planet’s surface. Ever since the New Horizons spacecraft began to approach the little world, these glistening spots have fascinated the astronomy community. Initially scientists thought that the spots were composed of hydrated magnesium sulfate (a substance quite similar to the Epsom salts sold for bathing and foot-soaking), however it now seems like the shiny patches are made of something else entirely. According to astronomers, the particular chemical in these glistening patches actually turns out to be sodium carbonate–a salt formed from carbon. On Earth, this chemical usually forms in evaporitic conditions–when water evaporates from a lake, sea, or hot springs. This seems to indicate that the geology of Ceres is more complicated than initially thought—instead of a big ice crystal which has always been the same, the miniature planet has undergone changes: surface water evaporated to leave these mysterious chemical deposits. Hopefully finding out about Ceres’ past can teach us more about how planets form (or don’t form).
Second, we turn our eyes back closer to Earth to take in the newly discovered “second moon” a tiny asteroid about the size of the great pyramid of Giza which seems to be orbiting Earth. This new asteroid, called 2016 HO3, is not really a true moon but a quasi-satellite: it sometimes loops around our planet because Earth and the little rock both orbit the sun on a similar circuit. The asteroid orbits the sun in 365.93 days (just slightly longer than Earth’s orbit of 365.24 days). Thus, for the next few hundred years it will act like a true moon as our orbits converge. The rock is about 40 meters (130 feet) across by 100 meters (328 feet) wide. It is a bit strange to think about it up there hidden in the darkness, but it is a fairly comforting asteroid day story. 2016 HO3 is never destined to hit Earth. The really bad asteroids seem to be the ones we don’t know about (so it is time to keep our eyes on the skies and learn more).
216 Kleopatra
It’s time for Ferrebeekeeper to get back out to space. This grotesque gray hambone-looking thing is a metallic asteroid approximately the size of New Jersey known as 216 Kleopatra. The asteroid was discovered in 1880 by Austrian astronomer Johann Palisa when he was director of the Austrian naval observatory at the great Austrian naval port of Pula (!). The asteroid is 217 kilometers long by 94 kilometers deep by 81 kilometers long (135 miles by 58 miles by 50 miles). It is composed of slurry of metal, dust, and…nothing: between 30 to 50% of the asteroid’s volume is empty space (which makes it sound a lot like the consumer goods for sale in American stores).
216 Kleopatra has been the subject of a fair amount of human scrutiny. In 2008, a team of astronomers working from Hawaii’s Keck observatory (at the summit of Mauna Kea in Hawaii discovered two tiny moons orbiting the asteroid. These moons have diameters of about 5 km and 3 km respectively and they are named Alexhelios and Cleoselene for Cleopatra’s children.
An obvious question is what knocked this doughty asteroid into a strangely shaped cloud of weird slurry and little moons. The most obvious answer is an oblique impact, which astronomers estimate occurred about a hundred million years ago. I wonder what other secrets this giant rubble pile in space is hiding.
Also…it rotates, as seen in this stunning animation.
A gray-tufted monkey traveled to the edge of space according to Iranian media
Today’s post concerns various contemporary news items regarding outer space. At first this list may seem like a bit of a mash-up, but it all comes together as a very specific polemical point.
This year has already featured a lot of space news, but, sadly, most of it seems like it could have come from the 1950s. Iran launched a monkey to the edge of outer space. South Korea placed its first satellite in orbit (which seems like a response to North Korea doing the same thing last year).
South Korea’s rocket lifts off from its launch pad at the Naro Space Center in Goheung, South Korea
In US space news, the 27th anniversary of the Challenger disaster came and went (that was an epically bad day in 6th grade–which was hardly a picnic anyway). Additionally, America announced that its biggest space plans for the near future include landing a redundant lander on Mars which was not exactly what NASA wanted but it fit the budget and was politically expedient. Our not-very-exciting work on our not-very-exciting next generation rockets continues slowly.
Finally, in other space-related news, paleontologists discovered that a massive space event apparently bombarded the Earth with Gamma rays in the 8th century. Astronomers speculate that two neutron stars might have collided! Also on February 15th a 50 meter asteroid will narrowly miss the Earth (flying by closer than many of our communication satellites).
All of this paints a rather alarming picture of a turbulent and dangerous universe where catastrophic events can occur with little notice. Meanwhile on Earth dangerous rogue nations (not you, South Korea, we like your style) are venturing into strategically important low Earth orbit. NASA’s current large-scale projects are lackluster (although its robotic exploration of the solar system continues to be exemplary). Are we discarding our leadership position in space because of debt, political paralysis, and complacency? It certainly seems like it…
An Aerial View of Lochnagar Crater in Summer of 2009
On July 1st 1916 at 7:28 AM, the British Army detonated the Lochnagar mine–two underground charges of a high explosive compound called ammonal (respectively 24,000lb and 30,000lb) thereby entirely vaporizing a large section of trenches filled with German infantryman. This was only one of 17 giant mines which the British exploded in Northern France that morning. In fact there were an original total of 21 buried explosive charges—but, because of various exigencies, two of these were not exploded until much later on July 1st (one of the remaining charges was detonated by lightning many years after the war, and another was never found).
One of the Other 17 Mined Explosions that Morning (Hawthorne Ridge)
The explosions followed 16 days of heavy artillery fire and immediately preceded a general infantry charge which began the Battle of the Somme. It was an appropriately apocalyptic beginning of the worst day ever for the British armed forces—by midnight there were 57,470 British casualties (19,240 of whom died of their injuries). The battle of the Somme itself ground on until 18 November, 1916 by which point it had claimed over 1,200,000 casualties from both sides. More than three hundred thousand people were killed during the course of the battle.
Lochnagar Crater after the Battle of the Somme
Today the huge scars from that morning have been filled in by farmland—with the notable exception of Lochnagar crater, which was privately purchased and left as a monument to the futility and destruction of World War I. Erosion is taking its toll on the crater, yet, even after nearly a century, the great hole still has a diameter of approximately 91 meters (300 feet) and a depth of 21 meters (70 feet). Lochnagar crater is said to be the largest extant crater created by human artifice during war (obviously pit mines and nuclear test sites are much larger). It still possesses a unique horror—a round void in the placid farmlands of Picardy. To this day the grain fields around it yield rusted rifles, dented helmets, and skeletons in addition to wheat.
I am writing about this disquieting pockmark as preparation for writing about Armistice Day later this week, when we can reflect on World War I — surely one of the most comprehensive disasters to befall humankind. I am also writing about the largest wartime crater on earth, as an opportunity to note how feebly small it is in comparison to even modest meteor impact craters such as Lake Lonar or Kaali Craters, both of which happened in the remote past–to say nothing of giants like the Manicouagan Crater in Quebec which has a diameter of 70 kilometers (even after 225 million years of erosion).
A High Altitude Photo of Manicouagan Crater
Of course all of this should really be cause to reflect on how lucky we are—not only have we missed the Great War (except for you, Florence Green, if you’re reading this), but we have also missed all sorts of other unfortunate events. Today at 6:28 PM EST, an asteroid passed by the Earth. At its closest point it was nearer to us than the moon. The space rock (unsentimentally named “2005 YU55”) was about the size of an aircraft carrier and was traveling faster than 13 km (8 miles) a second. An amateur astrophysicist on the web estimates that it would have created a crater more than 5 kilometers in diameter if it had struck a limestone region of Earth.
Asteroid 2005 YU55
Ceres (optimized image from the Hubble Space telescope)
Today’s post topic is located in the depths of space far far away from the bats, pumpkins, and haunted deserts I have been writing about for October. The dwarf planet Ceres is located in the midst of the asteroid belt between Jupiter and Mars. The only dwarf planet in the inner solar system, Ceres is only 950 km (590 miles) in diameter, but it is sufficiently large to have become spherical from its own gravity (and it is by far the largest asteroid). Named after Ceres (Demeter), the mythological goddess of growing things whose daughter was abducted by Hades and who gave the secrets of agriculture to humankind through the farmer Triptolemus, the dwarf planet was discovered in 1801 by Italian astronomer Giuseppe Piazzi, a Roman Catholic priest of the Theatine order. Ceres was the first asteroid to be discovered and it comprises a third of the asteroid belt’s total mass.
A comparison of the sizes of the Earth, Moon, and Ceres
The nebular hypothesis proposes that the solar system formed as a great cloud of space dust and gas coalesced into a disk which then further coagulated into small clumps, then into planetesimals, then into moon-sized planetary embryos, and finally into planets. Ceres is one of the few (or maybe the only) planetary embryos which formed four and a half billion years ago but somehow did not get smushed together with other like bodies to form a planet or hurled off into deep space. The dwarf planet probably consists of a rocky core surrounded with an icy mantle of frozen water. Ceres is believed to contains 200 million cubic kilometers of water–more fresh water than in all the lakes, rivers, clouds, swamps, ponds (and everything else) on Earth. The Hubble telescope has photographed several mysterious surface features on Ceres including a dark spot believed to be a crater (now informally named after Piazzi) and several bright spots, the nature of which is unknown.
Image of the bright spots on Ceres (taken by the Hubble Space telescope)
Astronomers are profoundly curious about Ceres and hope to better understand the history of the solar system by examining this surviving planetary embryo. Additionally, the chemical makeup of Ceres is similar to that of Earth. Scientists seeking extraterrestrial life have concentrated on Europa and Mars, but Ceres is next on their short list.
Astronomers will soon have some of their answers about Ceres. The asteroid probe Dawn is currently orbiting the asteroid Vesta–but its mission there is scheduled to end in July of 2012. At that point Dawn will power up its ion thrusters and fly to Ceres. In February of 2015 Dawn will enter permanent orbit around the little planet and we will finally have some of our answers.
