The Hammer of God by Arthur C. Clarke (Full Text)

In short, The Hammer of God is a disaster novel, telling of  the impending arrival of an asteroid named Kali (the Hindu god of death)  to Earth, threatening apocalyptic destruction.

What makes this  different from other disaster novels, of course, is that this is a novel  told with Clarke’s unique voice. The plot is told in about fifty short  chapters, each rarely more than a couple of pages long. The story is  mainly focussed around Robert Singh, who is the captain of the  expedition to hopefully stop Kali before it reaches Earth. Named  Goliath, the plan is to gently nudge Kali using a pile driver so that it  misses Earth.

If this sounds like another Earth-in-peril story,  well, it is. What makes this a little different is that along the way we  get a story filled with Clarke’s ideas, many of which are unusual,  though suffused with Sir Arthur’s gentle humour. He suggests that in  this future the religions of Christianity and Islam have combined to  create ‘Chrislam’, sharing their central beliefs for the good of all.  Computers are now part of everyday life, although as written from the  perspective of 1993 perhaps not as much as social media would  predominate today. Goliath is partly run by an AI, unsurprisingly called  David, who has developed some quite human mannerisms. David is a much  more personable version of his famous predecessor, HAL 9000.

All in all, it's a nice read for a stormy, rainy day.

The Hammer of God

by Sir Arthur C. Clarke

Published in Dec. 2011 (Issue 19) | 4502 words

It came in vertically, punching a hole ten km wide through the atmosphere, generating temperatures so high that the air itself started to burn. When it hit the ground near the Gulf of Mexico, rock turned to liquid and spread outward in mountainous waves, not freezing until it had formed a crater two hundred km across.

That was only the beginning of disaster: Now the real tragedy began. Nitric oxides rained from the air, turning the sea to acid. Clouds of soot from incinerated forests darkened the sky, hiding the sun for months. Worldwide, the temperature dropped precipitously, killing off most of the plants and animals that had survived the initial cataclysm. Though some species would linger on for millenniums, the reign of the great reptiles was finally over.

The clock of evolution had been reset; the countdown to Man had begun. The date was, very approximately, 65 million B.C.

***

Captain Robert Singh never tired of walking in the forest with his little son Toby. It was, of course, a tamed and gentle forest, guaranteed to be free of dangerous animals, but it made an exciting contrast to the rolling sand dunes of their last environment in the Saudi desert—and the one before that, on Australia’s Great Barrier Reef. But when the Skylift Service had moved the house this time, something had gone wrong with the food-recycling system. Though the electronic menus had fail-safe backups, there had been a curious metallic taste to some of the items coming out of the synthesizer recently.

“What’s that, Daddy?” asked the four-year-old, pointing to a small hairy face peering at them through a screen of leaves.

“Er, some kind of monkey. We’ll ask the Brain when we get home.”

“Can I play with it?”

“I don’t think that’s a good idea. It could bite. And it probably has fleas. Your robotoys are much nicer.”

“But …”

Captain Singh knew what would happen next: He had run this sequence a dozen times. Toby would begin to cry, the monkey would disappear, he would comfort the child as he carried him back to the house …

But that had been twenty years ago and a quarter-billion kilometers away. The playback came to an end; sound, vision, the scent of unknown flowers and the gentle touch of the wind slowly faded. Suddenly, he was back in this cabin aboard the orbital tug Goliath, commanding the 100-person team of Operation ATLAS, the most critical mission in the history of space exploration. Toby, and the stepmothers and stepfathers of his extended family, remained behind on a distant world which Singh could never revisit. Decades in space—and neglect of the mandatory zero-G exercises—had so weakened him that he could now walk only on the Moon and Mars. Gravity had exiled him from the planet of his birth.

“One hour to rendezvous, captain,” said the quiet but insistent voice of David, as Goliath’s central computer had been inevitably named. “Active mode, as requested. Time to come back to the real world.”

Goliath’s human commander felt a wave of sadness sweep over him as the final image from his lost past dissolved into a featureless, simmering mist of white noise. Too swift a transition from one reality to another was a good recipe for schizophrenia, and Captain Singh always eased the shock with the most soothing sound he knew: waves falling gently on a beach, with sea gulls crying in the distance. It was yet another memory of a life he had lost, and of a peaceful past that had now been replaced by a fearful present.

For a few more moments, he delayed facing his awesome responsibility. Then he sighed and removed the neural-input cap that fitted snugly over his skull and had enabled him to call up his distant past. Like all spacers, Captain Singh belonged to the “Bald Is Beautiful” school, if only because wigs were a nuisance in zero gravity. The social historians were still staggered by the fact that one invention, the portable “Brainman,” could make bare heads the norm within a single decade. Not even quick-change skin coloring, or the lens-corrective laser shaping which had abolished eyeglasses, had made such an impact upon style and fashion.

“Captain,” said David. “I know you’re there. Or do you want me to take over?”

It was an old joke, inspired by all the insane computers in the fiction and movies of the early electronic age. David had a surprisingly good sense of humor: He was, after all, a Legal Person (Nonhuman) under the famous Hundredth Amendment, and shared—or surpassed—almost all the attributes of his creators. But there were whole sensory and emotional areas which he could not enter. It had been felt unnecessary to equip him with smell or taste, though it would have been easy to do so. And all his attempts at telling dirty stories were such disastrous failures that he had abandoned the genre.

“All right, David,” replied the captain. “I’m still in charge.” He removed the mask from his eyes, and turned reluctantly toward the viewport. There, hanging in space before him, was Kali.

It looked harmless enough: just another small asteroid, shaped so exactly like a peanut that the resemblance was almost comical. A few large impact craters, and hundreds of tiny ones, were scattered at random over its charcoal-gray surface. There were no visual clues to give any sense of scale, but Singh knew its dimensions by heart: 1,295 m maximum length, 456 m minimum width. Kali would fit easily into many city parks.

No wonder that, even now, most of humankind could still not believe that this modest asteroid was the instrument of doom. Or, as the Chrislamic Fundamentalists were calling it, “the Hammer of God.”

***

The sudden rise of Chrislam had been traumatic equally to Rome and Mecca. Christianity was already reeling from John Paul XXV’s eloquent but belated plea for contraception and the irrefutable proof in the New Dead Sea Scrolls that the Jesus of the Gospels was a composite of at least three persons. Meanwhile the Muslim world had lost much of its economic power when the Cold Fusion breakthrough, after the fiasco of its premature announce­ment, had brought the Oil Age to a sudden end. The time had been ripe for a new religion embodying, as even its severest critics admitted, the best elements of two ancient ones.

The Prophet Fatima Magdalene (née Ruby Goldenburg) had attracted almost 100 million adherents before her spectacular—and, some maintained, self-contrived—martyrdom. Thanks to the brilliant use of neural programming to give previews of Paradise during its ceremonies, Chrislam had grown explosively, though it was still far outnumbered by its parent religions.

Inevitably, after the Prophet’s death the movement split into rival factions, each upholding the True Faith. The most fanatical was a fundamentalist group calling itself “the Reborn,” which claimed to be in direct contact with God (or at least Her Archangels) via the listening post they had established in the silent zone on the far side of the Moon, shielded from the radio racket of Earth by 3,000 km of solid rock.

***

Now Kali filled the main viewscreen. No magnification was needed, for Goliath was hovering only 200 m above its ancient, battered surface. Two crew members had already landed, with the traditional “One small step for a man”—even though walking was impossible on this almost zero-gravity worldlet.

“Deploying radio beacon. We’ve got it anchored securely. Now Kali won’t be able to hide from us.”

It was a feeble joke, not meriting the laughter it aroused from the dozen officers on the bridge. Ever since rendezvous, there had been a subtle change in the crew’s morale, with unpredictable swings between gloom and juvenile humor. The ship’s physician had already prescribed tranquilizers for one mild case of manic-depressive symptoms. It would grow worse in the long weeks ahead, when there would be little to do but wait.

The first waiting period had already begun. Back on Earth, giant radio telescopes were tuned to receive the pulses from the beacon. Although Kali’s orbit had already been calculated with the greatest possible accuracy, there was still a slim chance that the asteroid might pass harmlessly by. The radio measuring rod would settle the matter, for better or worse.

It was a long two hours before the verdict came, and David relayed it to the crew.

“Spaceguard reports that the probability of impact on Earth is 99.9%. Operation ATLAS will begin immediately.”

The task of the mythological Atlas was to hold up the heavens and prevent them from crashing down upon Earth. The ATLAS booster that Goliath carried as an external payload had a more modest goal: keeping at bay only a small piece of the sky.

***

It was the size of a small house, weighed 9,000 tons and was moving at 50,000 km/ h. As it passed over the Grand Teton National Park, one alert tourist photographed the incandescent fireball and its long vapor trail. In less than two minutes, it had sliced through the Earth’s atmosphere and returned to space.

The slightest change of orbit during the billions of years it had been circling the sun might have sent the asteroid crashing upon any of the world’s great cities with an explosive force five times that of the bomb that destroyed Hiroshima.

The date was Aug. 10, 1972.

***

Spaceguard had been one of the last projects of the legendary NASA, at the close of the 20th century. Its initial objective had been modest enough: to make as complete a survey as possible of the asteroids and comets that crossed the orbit of Earth—and to determine if any were a potential threat.

With a total budget seldom exceeding $10 million a year, a worldwide network of telescopes, most of them operated by skilled amateurs, had been established by the year 2000. Sixty-one years later, the spectacular return of Halley’s Comet encouraged more funding, and the great 2079 fireball, luckily impacting in mid-Atlantic, gave Spaceguard additional prestige. By the end of the century, it had located more than one million asteroids, and the survey was believed to be 90% complete. However, it would have to be continued indefinitely: There was always a chance that some intruder might come rush­ing in from the uncharted outer reaches of the solar system.

As had Kali, which had been detected in late 2212 as it fell sunward past the orbit of Jupiter. Fortunately humankind had not been wholly unprepared, thanks to the fact that Senator George Ledstone (Independent, West America) had chaired an influential finance committee almost a generation earlier.

The Senator had one public eccentricity and, he cheerfully admitted, one secret vice. He always wore massive horn-rimmed eyeglasses (nonfunctional, of course) because they had an intimidating effect on uncooperative witnesses, few of whom had ever encountered such a novelty. His “secret vice,” perfectly well known to everyone, was rifle shooting on a standard Olympic range, set up in the tunnels of a long-abandoned missile silo near Mount Cheyenne. Ever since the demilitarization of Planet Earth (much accelerated by the famous slogan “Guns Are the Crutches of the Impotent”), such activities had been frowned upon, though not actively discouraged.

There was no doubt that Senator Ledstone was an original; it seemed to run in the family. His grandmother had been a colonel in the dreaded Beverly Hills Militia, whose skirmishes with the L.A. Irregulars had spawned endless psychodramas in every medium, from old-fashioned ballet to direct brain stimulation. And his grandfather had been one of the most notorious bootleg­gers of the 21st century. Before he was killed in a shoot-out with the Canadian Medicops during an ingenious attempt to smuggle a kiloton of tobacco up Niagara Falls, it was estimated that “Smokey” had been responsible for at least 20 million deaths.

Ledstone was quite unrepentant about his grandfather, whose sensational demise had triggered the repeal of the late U.S.’s third, and most disastrous, attempt at Prohibition. He argued that responsible adults should be allowed to commit suicide in any way they pleased—by alcohol, cocaine or even tobacco—as long as they did not kill innocent bystanders during the process.

When the proposed budget for Spaceguard Phase 2 was first presented to him, Senator Ledstone had been outraged by the idea of throwing billions of dollars into space. It was true that the global economy was in good shape; since the almost simultaneous collapse of communism and capitalism, the skillful application of chaos theory by World Bank mathematicians had broken the old cycle of booms and busts and averted (so far) the Final Depression predicted by many pessimists. Nonetheless, the Senator argued that the money could be much better spent on Earth—especially on his favorite project, reconstructing what was left of California after the Su­perquake.

When Ledstone had twice vetoed Spaceguard Phase 2, everyone agreed that no one on Earth would make him change his mind. They had reckoned without someone from Mars.

The Red Planet was no longer quite so red, though the process of greening it had barely begun. Concentrating on the problems of survival, the colonists (they hated the word and were already saying proudly “we Martians”) had little energy left over for art or science. But the lightning flash of genius strikes where it will, and the greatest theoretical physicist of the century was born under the bubble domes of Port Lowell.

Like Einstein, to whom he was often compared, Carlos Mendoza was an excellent musician; he owned the only saxophone on Mars and was a skilled performer on that antique instrument. He could have received his Nobel Prize on Mars, as everyone expected, but he loved surprises and practical jokes. Thus he appeared in Stockholm looking like a knight in high-tech armor, wearing one of the powered exoskeletons developed for paraplegics. With this mechanical assistance, he could function almost unhandicapped in an environment that would otherwise have quickly killed him.

Needless to say, when the ceremony was over, Carlos was bombarded with invitations to scientific and social functions. Among the few he was able to accept was an appearance before the World Budget Committee, where Sena­tor Ledstone closely questioned him about his opinion of Project Spaceguard.

“I live on a world which still bears the scars of a thousand meteor impacts, some of them hundreds of kilometers across,” said Professor Mendoza. “Once they were equally common on Earth, but wind and rain—something we don’t have yet on Mars, though we’re working on it!—have worn them away.”

Senator Ledstone: “The Spaceguarders are always pointing to signs of asteroid impacts on Earth. How seriously should we take their warnings?”

Professor Mendoza: “Very seriously, Mr. Chairman. Sooner or later, there’s bound to be another major impact.”

Senator Ledstone was impressed, and indeed charmed, by the young scientist, but not yet convinced. What changed his mind was not a matter of logic but of emotion. On his way to London, Carlos Mendoza was killed in a bizarre accident when the control system of his exoskeleton malfunctioned. Deeply moved, Ledstone immediately dropped his opposition to Spaceguard, approving construction of two powerful orbiting tugs, Goliath and Titan, to be kept permanently patrolling on opposite sides of the sun. And when he was a very old man, he said to one of his aides, “They tell me we’ll soon be able to take Mendoza’s brain out of that tank of liquid nitrogen, and talk to it through a computer interface. I wonder what he’s been thinking about, all these years …”

***

Assembled on Phobos, the inner satellite of Mars, ATLAS was little more than a set of rocket engines attached to propellant tanks holding 100,000 tons of hydrogen. Though its fusion drive could generate far less thrust than the primitive missile that had carried Yuri Gagarin into space, it could run continuously not merely for minutes but for weeks. Even so, the effect on the asteroid would be trivial, a velocity change of a few centimeters per second. Yet that might be sufficient to deflect Kali from its fatal orbit during the months while it was still falling earthward.

***

Now that ATLAS’s propellant tanks, control systems and thrusters had been securely mounted on Kali, it looked as if some lunatic had built an oil refinery on an asteroid. Captain Singh was exhausted, as were all the crew members, after days of assembly and checking. Yet he felt a warm glow of achievement: They had done everything that was expected of them, the countdown was going smoothly, and the rest was up to ATLAS.

He would have been far less relaxed had he known of the ABSOLUTE PRIORITY message racing toward him by tight infrared beam from ASTROPOL headquarters in Geneva. It would not reach Goliath for another 30 minutes. And by then it would be much too late.

***

At about T minus 30 minutes, Goliath had drawn away from Kali to stand well clear of the jet with which ATLAS would try to nudge it from its present course. “Like a mouse pushing an elephant,” one media person had described the operation. But in the frictionless vacuum of space, where momentum could never be lost, even one mousepower would be enough if applied early and over a sufficient length of time.

The group of officers waiting quietly on the bridge did not expect to see anything spectacular: The plasma jet of the ATLAS drive would be far too hot to produce much visible radiation. Only the telemetry would confirm that ignition had started and that Kali was no longer an implacable juggernaut, wholly beyond the control of humanity.

There was a brief round of cheering and a gentle patter of applause as the string of zeros on the accelerometer display began to change. The feeling on the bridge was one of relief rather than exultation. Though Kali was stirring, it would be days and weeks before victory was assured.

And then, unbelievably, the numbers dropped back to zero. Seconds later, three simultaneous audio alarms sounded. All eyes were suddenly fixed on Kali and the ATLAS booster which should be nudging it from its present course. The sight was heartbreaking: The great propellant tanks were opening up like flowers in a time-lapse movie, spilling out the thousands of tons of reaction mass that might have saved the Earth. Wisps of vapor drifted across the face of the asteroid, veiling its cratered surface with an evanescent atmosphere.

Then Kali continued along its path, heading inexorably toward a fiery collision with the Earth.

***

Captain Singh was alone in the large, well-appointed cabin that had been his home for longer than any other place in the solar system. He was still dazed but was trying to make his peace with the universe.

He had lost, finally and forever, all that he loved on Earth. With the decline of the nuclear family, he had known many deep attachments, and it had been hard to decide who should be the mothers of the two children he was permitted. A phrase from an old American novel (he had forgotten the author) kept coming into his mind: “Remember them as they were—and write them off.” The fact that he himself was perfectly safe somehow made him feel worse; Goliath was in no danger whatsoever, and still had all the propellant it needed to rejoin the shaken survivors of humanity on the Moon or Mars.

Well, he had many friendships—and one that was much more than that—on Mars; this was where his future must lie. He was only 102, with decades of active life ahead of him. But some of the crew had loved ones on the Moon; he would have to put Goliath’s destination to the vote.

Ship’s Orders had never covered a situation like this.

***

“I still don’t understand,” said the chief engineer, “why that explosive cord wasn’t detected on the preflight check-out.”

“Because that Reborn fanatic could have hidden it easily—and no one would have dreamed of looking for such a thing. Pity ASTROPOL didn’t catch him while he was still on Phobos.”

“But why did they do it? I can’t believe that even Chrislamic crazies would want to destroy the Earth.”

“You can’t argue with their logic—if you accept their premises. God, Allah, is testing us, and we mustn’t interfere. If Kali misses, fine. If it doesn’t, well, that’s part of Her bigger plan. Maybe we’ve messed up Earth so badly that it’s time to start over. Remember that old saying of Tsiolkovski’s: ‘Earth is the cradle of humankind, but you cannot live in the cradle forever.’ Kali could be a sign that it’s time to leave.”

The captain held up his hand for silence.

“The only important question now is, Moon or Mars? They’ll both need us. I don’t want to influence you” (that was hardly true; everyone knew where he wanted to go), “so I’d like your views first.”

The first ballot was Mars 6, Moon 6, Don’t know 1, captain abstaining.

Each side was trying to convert the single “Don’t know” when David spoke.

“There is an alternative.”

“What do you mean?” Captain Singh demanded, rather brusquely.

“It seems obvious. Even though ATLAS is destroyed, we still have a chance of saving the Earth. According to my calculations, Goliath has just enough propellant to deflect Kali—if we start thrusting against it immediately. But the longer we wait, the less the probability of success.”

There was a moment of stunned silence on the bridge as everyone asked the question, “Why didn’t I think of that?” and quickly arrived at the answer.

David had kept his head, if one could use so inappropriate a phrase, while all the humans around him were in a state of shock. There were some compensations in being a Legal Person (Nonhuman). Though David could not know love, neither could he know fear. He would continue to think logically, even to the edge of doom.

***

With any luck, thought Captain Singh, this is my last broadcast to Earth. I’m tired of being a hero, and a slightly premature one at that. Many things could still go wrong, as indeed they already have …

“This is Captain Singh, space tug Goliath. First of all, let me say how glad we are that the Elders of Chrislam have identified the saboteurs and handed them over to ASTROPOL.

“We are now fifty days from Earth, and we have a slight problem. This one, I hasten to add, will not affect our new attempt to deflect Kali into a safe orbit. I note that the news media are calling this deflection Operation Deliverance. We like the name, and hope to live up to it, but we still cannot be absolutely certain of success. David, who appreciates all the goodwill messages he has received, estimates that the probability of Kali impacting Earth is still 10% …

“We had intended to keep just enough propellant reserve to leave Kali shortly before encounter and go into a safer orbit, where our sister ship Titan could rendezvous with us. But that option is now closed. While Goliath was pushing against Kali at maximum drive, we broke through a weak point in the crust. The ship wasn’t damaged, but we’re stuck! All attempts to break away have failed.

“We’re not worried, and it may even be a blessing in disguise. Now we’ll use the whole of our remaining propellant to give one final nudge. Perhaps that will be the last drop that’s needed to do the job.

“So we’ll ride Kali past Earth, and wave to you from a comfortable distance, in just fifty days.”

It would be the longest fifty days in the history of the world.

***

Now the huge crescent of the moon spanned the sky, the jagged mountain peaks along the terminator burning with the fierce light of the lunar dawn. But the dusty plains still untouched by the sun were not completely dark; they were glowing faintly in the light reflected from Earth’s clouds and continents. And scattered here and there across that once dead landscape were the glowing fireflies that marked the first permanent settlements hu­mankind had built beyond the home planet. Captain Singh could easily locate Clavius Base, Port Armstrong, Plato City. He could even see the necklace of faint lights along the Translunar Railroad, bringing its precious cargo of water from the ice mines at the South Pole.

Earth was now only five hours away.

***

Kali entered Earth’s atmosphere soon after local midnight, 200 km above Hawaii. Instantly, the gigantic fireball brought a false dawn to the Pacific, awakening the wildlife on its myriad islands. But few humans had been asleep this night of nights, except those who had sought the oblivion of drugs.

Over New Zealand, the heat of the orbiting furnace ignited forests and melted the snow on mountaintops, triggering avalanches into the valleys beneath. But the human race had been very, very lucky: The main thermal impact as Kali passed the Earth was on the Antarctic, the continent that could best absorb it. Even Kali could not strip away all the kilometers of polar ice, but it set in motion the Great Thaw that would change coastlines all around the world.

No one who survived hearing it could ever describe the sound of Kali’s passage; none of the recordings were more than feeble echoes. The video coverage, of course, was superb, and would be watched in awe for generations to come. But nothing could ever compare with the fearsome reality.

Two minutes after it had sliced into the atmosphere, Kali reentered space. Its closest approach to Earth had been 60 km. In that two minutes, it took 100,000 lives and did $1 trillion worth of damage.

***

Goliath had been protected from the fireball by the massive shield of Kali itself; the sheets of incandescent plasma streamed harmlessly overhead. But when the asteroid smashed into Earth’s blanket of air at more than one hundred times the speed of sound, the colossal drag forces mounted swiftly to five, ten, twenty gravities—and peaked at a level far beyond anything that machines or flesh could withstand.

Now indeed Kali’s orbit had been drastically changed; never again would it come near Earth. On its next return to the inner solar system, the swifter spacecraft of a later age would visit the crumpled wreckage of Goliath and bear reverently homeward the bodies of those who had saved the world.

Until the next encounter.

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The real reason why NASA sent a probe to land on the 433 Eros Asteroid

The decision to land a probe on the asteroid 433 Eros, and place a spacecraft in orbit around it was not by random chance. No particular scientist looked at a tabulated list of the thousands of asteroids and picked it out randomly. There was a real good reason. And that reason, boys and girls, is because MAJestic (through NASA) wanted a close look at the extraterrestrial facility there.

What the public is told…

The Near Earth Asteroid Rendezvous (NEAR)

The Near Earth Asteroid Rendezvous (NEAR) was designed to study the near Earth asteroid 433 Eros from close orbit. It was designed to operate for over a period of a year. It was designed quickly (for a NASA program) and was successfully launched in February 1996. It traveled for four years until it was able to enter orbit around the asteroid in February 2000.

The Near Earth Asteroid Rendezvous (NEAR) spacecraft took 4 years from launch until it became the first spacecraft to orbit an asteroid in February 2000. 

A month later, the spacecraft was re-named "NEAR Shoemaker" to honor the late Eugene Shoemaker. 

To save launch costs, the mission used a special 2-year-period trajectory with an Earth gravity assist. On the way, the spacecraft imaged the asteroid 253 Mathilde. 

On 20 December 1998, NEAR’s large engine misfired, failing to brake it for entry into orbit about 433 Eros. Another attempt 2 weeks later succeeded, but the spacecraft was almost a million kilometers away and took over a year to reach the asteroid. 

The mission was recovered thanks to a generous fuel supply and robust contingency planning. 

The implementation of the spacecraft’s daring orbital maneuvers is described, including those used to land on Eros’ surface in February 2001.

-NEAR Mission Design

In 1991, a “Discovery” Near Earth Asteroid Rendezvous (NEAR) mission was proposed, and competitive proposals for it were prepared by APL and by the Jet Propulsion Laboratory (JPL).

The APL proposal was selected and system definition studies were carried out in 1992–1993.

The studies first concentrated on direct flight paths to small near-Earth asteroids that lay on the Ecliptic plan. The initial plan was with a mission to (4660) Nereus that would launch in January 1998.

Jan 01, 2000 · The Apollo type asteroid (4660) Nereus (1982DB) is recognized as one of the most accessible asteroid, and it is a candidate for the target of MUSES-C project, i.e. the first asteroid sample return mission by the Institute of Space and Astronautical Science (ISAS).

-Photometric observation of (4660)Nereus - ScienceDirect

Strangely, some vocal but un-named scientists were concerned that an intensive orbital survey of such a small asteroid might not be very productive. They INSISTED that the entire mission be re-scoped to a completely different asteroid.

So these un-named scientists had the program target changed.

They argued that the 433 Eros asteroid would be a much better target since it has dimensions of about 14 x 14 x 33 km, about 400 times the area and over 6000 times the volume of 4660 Nereus. It was much, much, larger.

  • 4660 Nereus. The initial size estimate for Nereus came from an optical R-band study (Ishibashi et al., 2000a, 2000b) which concluded that it is an elongated object with diameter between 1.1–1.3 km
  • 433 Eros. Much larger at 33 x 13 x 13 km.

Unfortunately, problem was that 433 Eros was way, way out of the way. It was not on nor lay closely upon the Ecliptic Plane as all the other asteroids that were being considered. It was “in the boondocks”, and way out of the way. Making a trip to visit is outrageously difficult.

Eros’ orbit is inclined 11° to the ecliptic (Earth’s orbit plane), requiring, for direct transfers, high declination of launch asymptotes and launch energies that are too high for a reasonably sized spacecraft with the Discovery-baselined Delta-class launch vehicle. 

This problem was solved by using a 2-year delta V-Earth Gravity Assist (delta VEGA) trajectory. 

The spacecraft would be launched into an orbit with an approximately 2-year period in the ecliptic plane 23 months before the latest minimum-launch energy departure date on 22 or 23 January 1998. 

Near aphelion of this orbit, a delta V maneuver would be performed to target an Earth swing-by at the optimum date. At the Earth return, the spacecraft’s velocity relative to the planet would be increased considerably, allowing a swing-by low over the Northern Hemisphere that would bend the trajectory into Eros’ orbit plane with its 11° inclination to the ecliptic.

-NEAR Mission Design

In mid-1993, the delta VEGA trajectory to Eros was adopted as the baseline for the NEAR mission. At aphelion in early 1997, the space-craft would be behind the Sun as seen from the Earth, so the deep space delta V was moved to early March, several days after the NEAR spacecraft (re-christened NEAR Shoemaker in March 2000 to honor the late Eugene Shoe-maker) left the solar exclusion zone within 3° of the Sun, where communications with the spacecraft would be difficult or impossible.

Trajectory for the NEAR spacecraft to visit 433 Eros.
Trajectory for the NEAR spacecraft to visit 433 Eros.

After a four year travel, the NEAR spacecraft approached the asteroid and started to make it’s approach. This approach involved a lot of fuel, but unusually good planning on the part of NASA made sure that the spacecraft would be able to get into a fine parking orbit around the asteroid.

The table below, lists several parameters for each of the propulsive maneuvers performed by the NEAR Shoemaker spacecraft. In the last column, under “Mode,” the table

The table below, lists several parameters for each of the propulsive maneuvers (changing trajectory planes) performed by the NEAR Shoemaker spacecraft. In the last column, under “Mode,” the table indicates the basic strategy for orienting the spacecraft according to the options available (and described elsewhere).

It’s all very interesting (to me at least), but let’s not get too bogged down on all the interesting details. In short, the spacecraft needed to maneuver to get into orbit. This took generous amounts of fuel and energy. And, as specified earlier, this is simply because the spacecraft was moving to a difficult to visit, and difficult to go into orbit about, asteroid.

Here’s a summary of the orbital and trajectory firings, if you don’t believe me…

Orbital firings of the engines for the NEAR spacecraft.

Objectives

The primary scientific objectives of NEAR were to return data on the bulk properties, composition, mineralogy, morphology, internal mass distribution and magnetic field of 433 Eros. Secondary objectives include studies of asteroid regolith properties (loosely consolidated surface material), interactions with the solar wind, possible current activity as indicated by dust or gas and the asteroid spin state.

NASA’s NEAR Shoemaker spacecraft, met all its scientific goals in orbiting the asteroid Eros and successfully accomplished a controlled descent to the surface of the asteroid on 12 February 2001. The chief goal of the controlled descent to the surface was to gather close-up pictures of the boulder-strewn surface of 433 Eros, more than 196 million miles from Earth.

DESIGN

The NEAR spacecraft design is mechanically simple and geared toward a short development and test time. Except for the initial deployment of the solar panels and protective instrument covers, the spacecraft has only one moveable mechanism. Its distributed architecture allows parallel development and test of each subsystem, yielding an unusually short spacecraft integration and test period.

Several innovative features of the NEAR design include the first use of an x-band solid-state power amplifier for an interplanetary mission, the first use of a hemispherical resonator gyroscope in space and extremely high-accuracy, high voltage power supply control.

Equipment layout of the NEAR spacecraft.
Equipment layout of the NEAR Spacecraft.

The spacecraft has the shape of an octagonal prism, approximately 1.7m on each side. It has four fixed gallium arsenide solar panels in a windmill arrangement, a fixed 1.5m X-band high-gain radio antenna with a magnetometer mounted on the antenna feed and an X-ray solar monitor on one end (the forward deck). The other instruments are fixed on the opposite end (the aft deck). Most electronics are mounted on the inside of the decks. The propulsion module is contained in the interior.

PROPULSION

The craft is three-axis stabilized and uses a single bipropellant (hydrazine/nitrogen tetroxide) 450 Newton (N) main thruster and four 21N and seven 3.5N hydrazine thrusters for propulsion, for a total delta-V potential of 1,450m/s. Attitude control is achieved using the hydrazine thrusters and four reaction wheels. The propulsion system carried 209kg of hydrazine and 109kg of NTO oxidizer in two oxidizer and three fuel tanks.

NEAR Spacecraft showing deployment of the solar panels.
NEAR Spacecraft showing deployment of the solar panels.

Power was provided by four 1.8m x 1.2m gallium arsenide solar panels that can produce 400W at 2.2AU (NEAR’s maximum distance from the Sun) and 1,800W at 1AU. Power was stored in a 9A/hr, 22-cell rechargeable super nickel-cadmium battery.

INSTRUMENTATION

The spacecraft also featured Multi-Spectral Imager (MSI) for imaging Eros in multiple spectral bands to determine its shape and surface features and to map mineral distributions. It had a NEAR Infrared Spectrometer (NIS) for measuring the near-infrared spectrum to determine the distribution and abundance of surface minerals and a NEAR Laser Rangefinder (NLR). This is a laser altimeter that measures the range to the surface to build up high-resolution topographic profiles (giving a global shape model of Eros).

It also has an X-ray/Gamma-Ray Spectrometer (XGRS) detecting X-ray fluorescence from elements on the asteroid surface. Some of the emissions are excited by cosmic rays and some are from natural radioactivity in the asteroid. There is also a Magnetometer (MAG) that searches for and maps any intrinsic magnetic field around Eros and a Radio Science, which is a coherent X-band transponder measuring radial velocities of the spacecraft relative to Earth, helping to map the gravitational field of Eros.

The Landing of a probe onto the asteroid

NEAR-Shoemaker became the first spacecraft to land on an asteroid and send signals back from its surface.

NEAR spacecraft trajectory and crash site.
NEAR spacecraft trajectory and crash site.

Since the robot spacecraft was not designed for such activity, the success of the landing on asteroid 433 Eros was not assured. In short, after the orbital mapping was completed, the NASA team crashed the spacecraft into the asteroid. They tried to do it gingerly, but they pretty much smashed it onto the surface.

The last picture taken by the NEAR-Shoemaker spacecraft prior to impact.

Shown above is the last picture taken by NEAR-Shoemaker before its touchdown.

The streaking on the lower part of the image was caused by the loss of telemetry as the satellite impacted the surface.

The image was taken 130 meters above the surface and spans 6 meters across. Rocks as small as a human hand are visible.

The Official Narrative…

Feb. 12, 2001 — After an apparently gentle descent, the first spacecraft ever to land on an asteroid touched down today shortly after 3 p.m. ET.

The 1,100-pound craft settled on a saddle-shaped depression of the asteroid, Eros, and then continued transmitting signals to Earth, suggesting it was not damaged as it struck the asteroid’s rock-strewn surface.

Asteriod Landing Animation “I am happy to report that the NEAR has touched down,” said Robert Farquhar, the NEAR mission director, just after the craft transmitted its zero altitude location. “We are still getting signals!”

Not only was the dicey landing the first successful touchdown on an asteroid, it was also the most faraway landing ever attempted — at a distance of 196 million miles from Earth. The NEAR Shoemaker robot craft has no legs or landing gear and was never designed to land. To ensure a successful landing, controllers managed to slow the craft from about 20 to about 3 miles per hour.

First, controllers at The Johns Hopkins University Applied Physics Laboratory in Laurel, Md., triggered the craft to thrust its engines so the compact car-sized probe was knocked from its orbit and aimed for the asteroid. Then the team used a series of four rocket firings to slow the craft as it drifted toward the asteroid.

“We’re right on the money,” said NEAR Mission Operations Manager Robert Nelson as the NEAR probe drifted toward Eros. By just before 3 p.m. ET, the probe was less than a mile from the asteroid and approaching slowly. During its final descent scientists snapped about two photos of the asteroid every minute.

At one point controllers believed the craft had landed and then bounced away from the asteroid, but soon they received data suggesting it was resting on the rocky celestial outpost. The craft landed nearly on time, touching down on a 6-mile-wide, saddle-shaped depression at Eros’ side at 3:07 p.m.

“It’s an exciting area geologically because we’re on the edge of this large depression — which is probably a very large impact crater — and we’ll be getting images of its interior as well as of the heavily cratered terrain on the outside,” says NEAR imaging team member Mark Robinson of Northwestern University.

Now that it has managed a gentle landing, the tin-can shaped probe is expected to provide unprecedented up-close images and data from the asteroid for up to three months…

NEAR landing site on Eros.
(NEAR landing site on Eros)
Take a look at these high-quality, close-up images of Asteroid 433 Eros that NEAR Shoemaker spacecraft transmitted as it floated to a historic landing on the rocky surface nearly 200 million miles (322 million kilometers) from Earth on Monday, February 12, 2001.

Science Fiction Landings

As far as I know, the first story about landing a craft on an asteroid was written by Edward Drax in 1931. In The Travel Tales of Mr. Joseph Jorkens, minor navigation problems result in a landing on an asteroid:

"I had not seen it as soon as I had seen Mars, on account of its being so near to the line of the Sun... I couldn't make out anything, as most of the orb was in darkness... 

I got into the darkness at last and switched on my engines, and flew till I came to the very first edge of twilight that gave light enough for me to land... 

And that was how I came to make a bad landing, with my wheels deep down in a marsh..."

A more technical approach to landing on an asteroid was completed by Robert Heinlein. In his 1939 short story Misfit, young men without a trade were given another chance in the Cosmic Construction Corps. One job was to make a livable space habitat on selected asteroids.

He walked over by the lookouts at stereoscopes and radar tanks and peered up at the star-flecked blackness. Three cigarettes later the lookout nearest him called out.

"Light ho!"

"Where away?"

His mate read the exterior dials of the stereoscope. "Plus point two, abaft one point three, slight drift astern." He shifted to radar and added, "Range seven nine oh four three."

"Does that check?"

"Could be, Captain. What is her disk?" came the Navigator's muffled voice from under the hood.

The first lookout hurriedly twisted the knobs of his instrument, but the Captain nudged him aside. "I'll do this, son." He fitted his face to the double eye guards and surveyed a little silvery sphere, a tiny moon. Carefully he brought two illuminated cross-hairs up until they were exactly tangent to the upper and lower limbs of the disk. "Mark!"

The reading was noted and passed to the Navigator, who shortly ducked out from under the hood.

"That's our baby, Captain"

...McCoy forced them to lie down throughout the ensuing two hours. Short shocks of rocket blasts alternated with nauseating weightlessness. Then the blowers stopped and check valves clicked into their seats. The ship dropped free for a few moments -- a final quick blast -- five seconds of falling, and a short, light, grinding bump. A single bugle note came over the announcer, and the blowers took up their hum.

Public Discoveries

Of course, the entire data pool from the NEAR spacecraft is available for “armchair” and regular scientists to study. Of course, NASA has to “clean up” the data before releasing it. Don’t you know. There were things that might not be easy to explain or might be confusing to “Joe and Suzy Average”.

The photos of the asteroid have been very nice.

 It belongs to the Amor group.
Eros was one of the first asteroids to be visited by a spacecraft, and the first to be orbited and soft-landed on. NASA spacecraft NEAR Shoemaker entered orbit around Eros in 2000, and came to rest on its surface in 2001.
433 Eros is an S-type near-Earth asteroid approximately 34.4×11.2×11.2 kilometers (21.4×7.0×7.0 mi) in size, the second-largest near-Earth asteroid after 1036 Ganymed. It was discovered in 1898 and was the first near-Earth asteroid discovered. It was the first asteroid orbited by an Earth probe (in 2000). It belongs to the Amor group.
Eros was one of the first asteroids to be visited by a spacecraft, and the first to be orbited and soft-landed on. NASA spacecraft NEAR Shoemaker entered orbit around Eros in 2000, and came to rest on its surface in 2001.

Well, the public will never know what was really discovered or found out.

Instead we get to see nice pictures of dust, rocks and dirt.

This view of asteroid 433 Eros is part of an image mosaic taken in the early hours of October 26, 2000, during NEAR Shoemaker's low-altitude flyover of Eros. Taken while the spacecraft's digital camera was looking at a spot 8 kilometers (5 miles) away, the image covers a region about 800 meters (2600 feet) across. Rocks of all sizes and shapes are set on a gently rolling, cratered surface. Locally, fine debris or regolith buries the rocks. The large boulder at the center of the scene is about 25 meters (82 feet) across.
This view of asteroid 433 Eros is part of an image mosaic taken in the early hours of October 26, 2000, during NEAR Shoemaker’s low-altitude flyover of Eros. Taken while the spacecraft’s digital camera was looking at a spot 8 kilometers (5 miles) away, the image covers a region about 800 meters (2600 feet) across. Rocks of all sizes and shapes are set on a gently rolling, cratered surface. Locally, fine debris or regolith buries the rocks. The large boulder at the center of the scene is about 25 meters (82 feet) across.

What we are told instead is the geology of the asteroid itself. And while this is very interesting, most people wouldn’t really care about it at all. They just don’t.

433 Eros had a past full of impacts and the resulting craters.

Eros is 20 miles (33 kilometers) long and about 8 miles (13 kilometers) wide. It is the most well studied asteroid. NEAR-Shoemaker mapped Eros in detail back in 2000-2001 before officials executed a controlled and dramatic crash landing, the first-ever touchdown on an asteroid.

433 Eros.

Like any asteroid, Eros been banging around the solar system in some form for about 4.5 billion years.

In the early days of the solar system, when things were more crowded, collisions were frequent. Some large asteroids become smaller. Some small rocks stuck together and grew. Many were scooped up by the fledgling Earth and the other planets.

Two examples of evidence for a joint and fracture structure underlying the regolith layer on 433 Eros, imaged by the NEAR-Shoemaker spacecraft, in the form of: (A) several structurally controlled, `square' impact craters (MET 132151598, 218.91 W, 16.64 S, 5.57 m/pixel); and (B) a network of criss-crossing ridges and grooves, with a few, small, structurally controlled craters (MET 136266921, 218.72 W, 42.00 N, 4.58 m/pixel).
Two examples of evidence for a joint and fracture structure underlying the regolith layer on 433 Eros, imaged by the NEAR-Shoemaker spacecraft, in the form of: (A) several structurally controlled, `square’ impact craters (MET 132151598, 218.91 W, 16.64 S, 5.57 m/pixel); and (B) a network of criss-crossing ridges and grooves, with a few, small, structurally controlled craters (MET 136266921, 218.72 W, 42.00 N, 4.58 m/pixel).

The asteroids that remain, confined mostly to a belt between Mars and Jupiter, harbor a tale of the solar system’s formation. But first scientists have to figure out how to read their language, with an alphabet of craters and cracks and a grammar based largely on mineral composition and density.

Another great view of 433 Eros.

Among Eros’ most striking features is an impact crater 4.7 miles (7.6 kilometers) wide that scientists have determined was carved fairly recently. Another curious aspect to Eros is that across nearly 40 percent of its surface, all craters up to about a third of a mile (0.5 kilometers) wide have been erased.

Smooth surface.

The smooth surface has puzzled scientists since the NEAR landing.

A great view of 433 Eros.

The new study, led by Cornell University researcher Peter Thomas, nixed one theory by determining that the vanished craters could not have been covered by material ejected in the recent large impact. Further, the locations of the erased craters suggests they were jiggled out of existence by the internal vibrations caused in the impact.

Two examples of ponded deposits on 433 Eros, imaged by the NEAR-Shoemaker spacecraft. Note the marked difference in morphology between these ponds and the degraded craters shown Fig. 1(D) and Fig. 15, indicative of different formation processes. The ponds shown here are located on the low surface-gravity (2.5-3.0 mm sec^-2) 'nose' of the asteroid, which also spends a longer than average amount of time near the terminator (light/dark boundary). (A) A beautiful 100 m diameter ponded deposit containing an embedded 25 m boulder. Note the extremely flat surface containing a tiny (few-meter diameter) impact crater (MET 155888598, 179.04 W, 2.42 S, 0.55 m/pixel). (B) A smaller 75 m diameter ponded deposit. Note the difference between the smooth, fine-grained pond surface and the coarse, boulder strewn terrain surrounding the deposit (MET 155888731, 183.88 W, 3.21 S, 0.63 m/pixel).
Two examples of ponded deposits on 433 Eros, imaged by the NEAR-Shoemaker spacecraft. Note the marked difference in morphology between these ponds and the degraded craters shown Fig. 1(D) and Fig. 15, indicative of different formation processes. The ponds shown here are located on the low surface-gravity (2.5-3.0 mm sec^-2) ‘nose’ of the asteroid, which also spends a longer than average amount of time near the terminator (light/dark boundary). (A) A beautiful 100 m diameter ponded deposit containing an embedded 25 m boulder. Note the extremely flat surface containing a tiny (few-meter diameter) impact crater (MET 155888598, 179.04 W, 2.42 S, 0.55 m/pixel). (B) A smaller 75 m diameter ponded deposit. Note the difference between the smooth, fine-grained pond surface and the coarse, boulder strewn terrain surrounding the deposit (MET 155888731, 183.88 W, 3.21 S, 0.63 m/pixel).

The hypothesis, if right, can be used to glean an idea of how the asteroid is constructed. Scientists have long wondered if asteroids were solid rocks or, as is likely in at least some cases, loose piles of rubble that have undergone many collisions and managed to hang together.

"Our observations indicate that the interior of Eros is sufficiently cohesive to transmit seismic energy over many kilometers, and the outer several tens of meters [yards] of the asteroid must be composed of relatively non-cohesive material," 

-Thomas and his colleague, Mark Robinson of Northwestern University, write in the July 21 issue of the journal Nature.

That outer non-cohesive stuff would be regolith, which on Earth is called dirt and on our nearest natural satellite is known as Moon dust.

"For the first time, the authors provide convincing evidence that makes this conclusion more than just reasonable conjecture," 

- Erik Asphaug, a scientist at the University of California, Santa Cruz who was not involved in the study.

The non-public discoveries

Famous Taiwanese ufologist Scott Waring, studying NASA official images, regularly publishes his findings and shares his opinions. And, this time, he studied the surface of the near-Earth asteroid Eros from a photograph taken by NASA, and found something interesting on it.

According to the ufologist, on the surface of the asteroid Eros clearly visible unnatural structure, which has a rectangular shape.

NASA has reported that there is a large rectangular shaped object that rests upon 433 Eros.
NASA has reported that there is a large rectangular shaped object that rests upon 433 Eros.

The ufologist found it very funny that NASA noticed this structure, but the space agency’s explanations turned out to be very predictable and primitive.

According to NASA scientists, this is a “large rectangular object that measures 45 meters (148 feet) across“. There are no further explanations for this finding. (Ah. They know what is going on, and they know that they cannot comment on it.)

It is possible that this object is a mining station that was used by an advanced alien civilization to extract valuable metals.
It is possible that this object is a mining station that was used by an advanced alien civilization to extract valuable metals.

No further information regarding this feature has been made available.

NASA has nothing further to say about this matter.

What is this thing?

So anyone who looks at this photograph can conclude that this object looks to be of some kind of artificial construction. Why?

  • The shape is rectangular.
  • In the exact center of this object is another rectangular object.
  • The light reflecting off this object is different is type and magnitude from the surrounding terrain.
  • The shadow of this object shows a rectangular cross section.
  • The shadow indicates that the front protrusion hangs out and over the terrain, like a gantry crane or some kind of access tube.

Because of the above, those that study this matter believe that this object is not of natural construction.

One thing is clear. The object in the picture is NOT the NEAR Shoemaker probe from NASA.  It is something altogether different. 

The probe did not “fire” or launch any objects into the asteroid.  This is a photo from the NEAR spacecraft as it orbited the asteroid.  In so doing it caught a picture of this rectangular object resting on the surface of the asteroid. Then it was ordered to crash into the asteroid.

This object does not appear to be of natural construction.
Non-human probe discovered on 433 Eros.
This is a photo of the NASA raw feed for the NEAR Shoemaker Probe as it orbited the 433 EROS asteroid. It shows an object that appears to be a series of interconnected rectangular boxes and containers.  There are those that state that these are suggestive of mining operations, but what their true purpose is remains unknown.

Debunkers have their say…

Well, there is no way that this can be “swamp gas”, can it?

Debunkers offer alternative solutions to the observed anomaly. They postulate that [1] it is a Photoshop fraud, or that [2] it is a NASA photo from the Hubble Space Telescope that imaged a photo of the NEAR spacecraft itself on the surface of the asteroid. (If so, then it doesn’t look anything like the spacecraft.) They also postulate that [3] it is merely debris that was ejected from the NEAR spacecraft that happened to land on the asteroid in the fashion shown, and finally [4] it is just a pixilation error caused by a gamma-ray burst that caused an erroneous image pattern.

Interesting stretches of imagination.

But I can personally assure the readership that as of 2004 the MAJestic organization formally considered this object to be an extraterrestrial probe or structure of unknown purpose. That I can tell you all.

Conclusions

In the image of the asteroid Eros made by the NEAR Shoemaker spacecraft on May 1, 2000, when it was at an orbital altitude of 53 km (33 miles), it is visible, a large rectangular object, 45 meters in diameter.
In the image of the asteroid Eros made by the NEAR Shoemaker spacecraft on May 1, 2000, when it was at an orbital altitude of 53 km (33 miles), it is visible, a large rectangular object, 45 meters in diameter.

In the image of the asteroid Eros made by the NEAR Shoemaker spacecraft on May 1, 2000, when it was at an orbital altitude of 53 km (33 miles), it is visible, a large rectangular object, 45 meters in diameter.

The size of four (40′ GP) shipping containers laid end to end.

Considering the fact that data from the spacecraft collected on Eros in December 1998 suggest that it can contain 20,000 billion kilograms of aluminum and a similar amount of other metals that are rare on Earth, such as gold and platinum.

The weight of Eros is 6.69 · 1015 kilograms, which is a bit even for an asteroid. However, if we take into account the size of the asteroid – 34.4 km in diameter in the widest place – it turns out that Eros is quite dense, about 2.67 g / cm³. The same density would have an aluminum monolith of similar dimensions. Similar characteristics have the crust. By the way, even with its small size, Eros is the second largest among near-Earth asteroids.

The shape of Eros is irregular, elongated and often compared with peanuts. Because of this, the center of gravity shifts, which creates extremely interesting effects. Moving in its orbit, Eros does not rotate, like spherical bodies – and somersaults, like a boulder rolling from the hill. This also leads to differences in gravitational force. However, it is very easy to overcome it. A man would be able to leave Eros with the help of a foot thrust.

It is possible that this object is a mining station that was used by an advanced alien civilization to extract valuable metals.

The asteroids converging with the Earth are a group of small celestial bodies whose orbit has a chance in future to cross with our planet. The asteroid Eros – is among the most studied asteroids in the solar system.

Eros belongs to the class of asteroids S – the so-called stone asteroids, the material of which consists of silicon and metals.

Orbital characteristics of Eros – its main attraction. Around the Sun, he turns for 1.7 of the Earth year, around his own axis – for 5 and a half hours. But the real feature of Eros is that it belongs to the group of Cupids – asteroids, whose orbit is similar to the terrestrial, but lies further from the Sun. So, none of the Cupids can approach the Sun closer than 1.017 “standard” distance from the Sun to Earth – an astronomical unit. By the way, the Earth itself can move away from the Sun at such a distance – when reaches aphelion, the maximum distance from the luminary. This happens in the middle of summer, between 3 and 7 July.

Due to this they are quite bright – the largest objects of the S-class can be seen in a regular binocular.

Such asteroids also contain a large amount of minerals. After analyzing the composition of Eros, the scientists once again started talking seriously about the industrial development of outer space.

The object found in place on 433 Eros.
The object found in place on 433 Eros.

This is an interesting object.

If I were a betting man, I would guess that this object is either a robotic mining droid or a monitoring station of some sort.

But I do not know.

As of 2004, neither did MAJestic.

Anyways…

When someone tries to tell you that sooner or later the US Government is going to release “findings” and conduct “studies” on the “UFO issue”, you can laugh in their face. MAJestic has known for years about the population of our solar system by extraterrestrials. It’s just that there are limits to how we can go about in the discovery of these entities and their technologies.

Anyways, enjoy the few precious snippets that you can find on the internet now. The suppression of NASA related images is now “tighter than a drum”. You won’t find much more in the future moving forward.

And this object…

It’s either a robot, a probe, a station, a mining vehicle, or some other mechanism that was not made by humans. It rests upon the asteroid 433 Eros, and does it’s thing. Whatever it’s “thing” is.

MAJestic knows about it. And perhaps it radiated some signals or gave away it’s presence way back in the late 1990’s. Meaning that it was active at that time.

Do you want more?

I have more posts in my MAJestic Index here…

MAJestic

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