Comments by "H. de Jong" (@h.dejong2531) on "The Problem with the Next Moon Mission" video.

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  57. None of that is correct.  1. Reflections in the helmet visor show the other astronaut, and equipment on the lunar surface. 2. That museum curator was sadly lying, or you are. Apollo 11 did not carry a rover. Only Apollo 15, 16 and 17 did. Those rovers were left on the lunar surface. What that museum has is a replica. 3. Another instance where I don't believe you. In 1999, the first components of the ISS had been launched, but no crew had visited the station yet. So it's possible you saw actual ISS hardware being prepared for launch. In 1999, you did not see astronauts on TV inside the ISS.  Adding modules to the ISS is done by launching them on a rocket, then maneuvering them into place. 4. That answer was insufficiently precise. NASA did not lose the technology. Drawings for every part of the Saturn V and Apollo spacecraft exist. We have a bunch of versions of the software for the AGC. We have loads of info on every aspect of the design. Is that enough to launch a new Saturn V tomorrow? No. That's what he was getting at. We don't have a production line cranking out moon rockets today. We're getting close to having one with the Artemis program. Note that Artemis will use new designs instead of "just" copying the Saturn V. It'd be insane to put a 60 year old design back into production: we've advanced a lot in those 60 years. We have new manufacturing methods, new materials, much better design tools etc. If you wanted to copy the Saturn V today, you'd have to replace some of the 1960s era components with new ones: it'd be ridiculous to build new Apollo Guidance Computers to their 1960s design. So you have to develop new software. The drawings have to be redone in CAD so you can use modern manufacturing processes. All in all, it takes a few years to start up a Saturn V production line, and in that time you could also design a new rocket. This applies to all complex, old projects by the way. B-52, SR-71, the Eiffel tower they would take a long time to replicate, and with today's knowledge we can do better anyway so there's no point.
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  77. While technically the moon is in our atmosphere, we're talking about 0.2 atoms per cm3, i.e. negligible. We figured out how to get through the van Allen belts in 1958. For radiation, there are 2 important variables: 1. the radiation intensity 2. the amount of time you are exposed to this intensity. You can multiply these two and get the total radiation dose. Humans die if they receive a dose of about 300 Rad. In 1958, James van Allen and his team discovered the belts that were later named after him. He also measured the radiation intensity. This is what he found: in the part of the belt where the intensity is highest, it is high enough that if you stay for about a week (inside an Apollo command module), you receive a lethal dose. So for the Apollo missions, the trajectory was designed to minimize the amount of time spent there. The Apollo astronauts flew through the belts in about 3 hours, while avoiding the part with the highest levels entirely. The hull thickness of the CSM was more than enough to reduce the radiation level inside to manageable levels. Astronauts' overall exposure was actually dominated by solar particles once outside Earth's magnetic field. The total radiation received by the astronauts varied from mission-to-mission but was measured to be between 0.16 and 1.14 rads (1.6 and 11.4 mGy). More details in this video from Scott Manley: https://www.youtube.com/watch?v=h9YN50xXFJY And no, Aldrin didn't say that. That's just moon landing deniers taking a quote out of context. The question was 'why didn't we go back', and Aldrin answered 'because we didn't'. That's not an admission he didn't go to the moon. In the rest of the interview, he talks about his experiences on Apollo 11.
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  107. We figured out how to get through the van Allen belts in 1958. For radiation, there are 2 important variables: 1. the radiation intensity 2. the amount of time you are exposed to this intensity. You can multiply these two and get the total radiation dose. Humans die if they receive a dose of about 300 Rad. In 1958, James van Allen and his team at the University of Iowa discovered the belts that were later named after him, using measurements from the NASA missions Explorer 1. With Explorer 3 and 4 and Pioneer 3 he measured the radiation intensity. This is what he found: in the part of the belt where the intensity is highest, it is high enough that if you stay for about a week (inside an Apollo command module), you receive a lethal dose. So for the Apollo missions, the trajectory was designed to minimize the amount of time spent there. The Apollo astronauts flew through the belts in about 3 hours, while avoiding the part with the highest levels entirely. The hull thickness of the CSM was more than enough to reduce the radiation level inside to manageable levels. Astronauts' overall exposure was actually dominated by solar particles once outside Earth's magnetic field. The total radiation received by the astronauts varied from mission-to-mission but was measured to be between 0.16 and 1.14 rads (1.6 and 11.4 mGy). More details in this video from Scott Manley: https://www.youtube.com/watch?v=h9YN50xXFJY And no, NASA isn't saying they can't get through the van Allen belts. You're referring to a video published in 2014, which has an engineer talking about the first Orion test flight, saying 'we have to do this to make sure it's safe for humans'. This test flight was done to make sure the Orion capsule works correctly in the VA belt: electronics can malfunction in high-radiation environments. Orion's electronics are designed to deal with this, but a practical test is required as part of due diligence. All of the hardware on Orion is new, so it has to be tested in operational circumstances before being considered human-rated. The Apollo program did these tests as well, during the Apollo 4 and 6 flights.
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  123. No, NASA has never claimed that, because it's not true. Complete TV recordings are available for every mission, in addition to all the film footage they took and thousands of photos. The only video recording lost was ONE tape of the Apollo 11 landing and first steps, recorded at Honeysuckle Creek, where the TV signal was received. We still have other recordings of that broadcast, the HC recording was at a higher quality (it avoided one step of conversion and quality loss). In addition, some telemetry tapes were not archived, because they were no longer relevant after the end of the Apollo program. All of the drawings, specifications etc. are still available and in public archives. The rest of your post is full of nonsense as well. Temperature differences for instance: the missions were all planned at a specific point of the lunar day, when ambient temperatures were around 20 ºC. They had to contend with heating from the sun; that was mostly taken care of by putting a white outer layer over the spacesuit, and by internal insulation layers. The backpack removed excess heat. The risk of metorite impact was low: the entire area covered by each mission gets hit once every 1000 years. And yes, the 16 layers of the space suit provide protection against micrometeoroids. The outer layer breaks up the meteoroid and issipates its energy so it can't penetrate inner layers. The "petrified rock" story is bullshit. In 2006, a Dutch museum hosted an art exhibit that showcased forgeries. One of the exhibits ended up in the museum's collection afterwards; its paperwork was lost. In 2009, this was examined and found to be wood. Meanwhile, we have 380 kg of actual moon rock, samples of which have been examined and authenticated by mineralogists all over the world. So, you've been lied to, by moon landing deniers. They make up shit instead of providing real arguments, because there aren't any real arguments to be made.
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  154. No, we don't need to develop any radiation shielding to do manned lunar missions. We figured that out by 1962. For radiation, there are 2 important variables: 1. the radiation intensity 2. the amount of time you are exposed to this intensity. You can multiply these two and get the total radiation dose. Humans die if they receive a dose of about 300 Rad. In 1958, James van Allen and his team at the University of Iowa discovered the belts that were later named after him, using measurements from the NASA missions Explorer 1. With Explorer 3 and 4 and Pioneer 3 he measured the radiation intensity. By 1962, we had a good map of the van Allen belt, and this is what it told us: in the part of the belt where the intensity is highest, it is high enough that if you stay for about a week (inside an Apollo command module), you receive a lethal dose. So for the Apollo missions, the trajectory was designed to minimize the amount of time spent there. The Apollo astronauts flew through the belts in about 3 hours, while avoiding the part with the highest levels entirely. The hull thickness of the CSM was more than enough to reduce the radiation level inside to manageable levels. Astronauts' overall exposure was actually dominated by solar particles once outside Earth's magnetic field. The total radiation received by the astronauts varied from mission-to-mission but was measured to be between 0.16 and 1.14 rads (1.6 and 11.4 mGy). More details in this video from Scott Manley: https://www.youtube.com/watch?v=h9YN50xXFJY
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  194. We figured out how to get through the van Allen belts in 1958. For radiation, there are 2 important variables: 1. the radiation intensity 2. the amount of time you are exposed to this intensity. You can multiply these two and get the total radiation dose. Humans die if they receive a dose of about 300 Rad. In 1958, James van Allen and his team discovered the belts that were later named after him. He also measured the radiation intensity. This is what he found: in the part of the belt where the intensity is highest, it is high enough that if you stay for about a week (inside an Apollo command module), you receive a lethal dose. So for the Apollo missions, the trajectory was designed to minimize the amount of time spent there. The Apollo astronauts flew through the belts in about 3 hours, while avoiding the part with the highest levels entirely. The hull thickness of the CSM was more than enough to reduce the radiation level inside to manageable levels. Astronauts' overall exposure was actually dominated by solar particles once outside Earth's magnetic field. The total radiation received by the astronauts varied from mission-to-mission but was measured to be between 0.16 and 1.14 rads (1.6 and 11.4 mGy). More details in this video from Scott Manley: https://www.youtube.com/watch?v=h9YN50xXFJY They won't be landing on "light". We can measure the composition of the moon from Earth, by analyzing its light via spectroscopy. That tells us the moon consists of rock. And we have landed on the Moon 29 times now. None of those landings reported anything other than solid rock.
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  395.  @MS-ib8xu  Collins's job was to look at the Moon, so that's what he spent his time doing. There were only brief periods during his lunar orbits when the stars would be visible at all. Have you measured the videos to see how the dust travels? I don't think so. The flags waving can have several causes: thermal stress, dust impacts, local vibrations, static, to name a few. The astronauts occasionally started answering before Houston was finished speaking. It happens. The Astronauts were aware of the van Allen belts. We figured out how to get through those in 1958. For radiation, there are 2 important variables: 1. the radiation intensity 2. the amount of time you are exposed to this intensity. You can multiply these two and get the total radiation dose. Humans die if they receive a dose of about 300 Rad. In 1958, James van Allen and his team discovered the belts that were later named after him. He also measured the radiation intensity. This is what he found: in the part of the belt where the intensity is highest, it is high enough that if you stay for about a week (inside an Apollo command module), you receive a lethal dose. So for the Apollo missions, the trajectory was designed to minimize the amount of time spent there. When the Apollo astronauts flew through the van Allen belts (which took about 3 hours), they received a dose of radiation of between 0.16 and 1.14 rads, or less than 1% of a lethal dose. More details in this video from Scott Manley: https://www.youtube.com/watch?v=h9YN50xXFJY i.e. the van Allen belts were a non-issue. The wording of Aldrin’s answer may have been confusing to children and adults alike, but he was talking about “why something (i.e., going to the moon) stopped in the past,” not about how it never happened in the first place. The video also cut off Aldrin’s full answer. In the complete version of Aldrin’s interview with this child (identified as Zoey), the astronaut went on to state the primary reason we didn’t return to the moon: money. Here's another Aldrin quote: "Whenever I gaze up at the moon, I feel like I'm on a time machine. I am back to that precious pinpoint of time, standing on the foreboding - yet beautiful - Sea of Tranquility. I could see our shining blue planet Earth poised in the darkness of space." If a moron came up to me ranting about how he didn't believe the biggest job I did in my life was real, I'd punch him too.
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  513.  @rodgangloff8540  And yet you've fallen for shoddy propaganda. Every single argument made by moon landing deniers falls apart when you look at it: they're based on logical errors, a basic lack of understanding or physics or outright lies. We figured out how to get through the van Allen belts in 1958. For radiation, there are 2 important variables: 1. the radiation intensity 2. the amount of time you are exposed to this intensity. You can multiply these two and get the total radiation dose. Humans die if they receive a dose of about 300 Rad. In 1958, James van Allen and his team discovered the belts that were later named after him. He also measured the radiation intensity. This is what he found: in the part of the belt where the intensity is highest, it is high enough that if you stay for about a week (inside an Apollo command module), you receive a lethal dose. So for the Apollo missions, the trajectory was designed to minimize the amount of time spent there. The Apollo astronauts flew through the belts in about 3 hours, while avoiding the part with the highest levels entirely. The hull thickness of the CSM was more than enough to reduce the radiation level inside to manageable levels. Astronauts' overall exposure was actually dominated by solar particles once outside Earth's magnetic field. The total radiation received by the astronauts varied from mission-to-mission but was measured to be between 0.16 and 1.14 rads (1.6 and 11.4 mGy). More details in this video from Scott Manley: https://www.youtube.com/watch?v=h9YN50xXFJY
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  619.  @sandy-sx5zr  You haven't done your homework.  Don Pettit was being insufficiently precise when he said that. NASA did not lose the technology. Drawings for every part of the Saturn V and Apollo spacecraft exist. We have a bunch of versions of the software for the AGC. We have loads of info on every aspect of the design. All of this is publicly available.  They discarded the rocket telemetry because at the end of Apollo, that info was obsolete.  The "petrified rock" story is bullshit. In 2006, a Dutch museum hosted an art exhibit that showcased forgeries. One of the exhibits ended up in the museum's collection afterwards; its paperwork was lost. In 2009, this was examined and found to be wood. Meanwhile, we have 380 kg of actual moon rock, samples of which have been examined and authenticated by mineralogists all over the world. We figured out how to get through the van Allen belts in 1958. For radiation, there are 2 important variables: 1. the radiation intensity 2. the amount of time you are exposed to this intensity. You can multiply these two and get the total radiation dose. Humans die if they receive a dose of about 300 Rad. In 1958, James van Allen and his team discovered the belts that were later named after him. He also measured the radiation intensity. This is what he found: in the part of the belt where the intensity is highest, it is high enough that if you stay for about a week (inside an Apollo command module), you receive a lethal dose. So for the Apollo missions, the trajectory was designed to minimize the amount of time spent there. The Apollo astronauts flew through the belts in about 3 hours, while avoiding the part with the highest levels entirely. The hull thickness of the CSM was more than enough to reduce the radiation level inside to manageable levels. Astronauts' overall exposure was actually dominated by solar particles once outside Earth's magnetic field. The total radiation received by the astronauts varied from mission-to-mission but was measured to be between 0.16 and 1.14 rads (1.6 and 11.4 mGy). More details in this video from Scott Manley: https://www.youtube.com/watch?v=h9YN50xXFJY
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  788. 1. No, NASA has said no such thing. They figured out how to get through the van Allen belts in 1958. For radiation, there are 2 important variables: 1. the radiation intensity 2. the amount of time you are exposed to this intensity. You can multiply these two and get the total radiation dose. Humans die if they receive a dose of about 300 Rad. In 1958, James van Allen and his team discovered the belts that were later named after him. He also measured the radiation intensity. This is what he found: in the part of the belt where the intensity is highest, it is high enough that if you stay for about a week (inside an Apollo command module), you receive a lethal dose. So for the Apollo missions, the trajectory was designed to minimize the amount of time spent there. When the Apollo astronauts flew through the van Allen belts (which took about 3 hours), they received a dose of radiation of between 0.16 and 1.14 rads, or less than 1% of a lethal dose. More details in this video from Scott Manley: https://www.youtube.com/watch?v=h9YN50xXFJY 2. That interview quote is taken out of context. The question was 'why didn't we go back', and Aldrin answered 'because we didn't'. That's not an admission he didn't go to the moon. In the rest of the interview, he talks about his experiences on Apollo 11. 3. Again, taken out of context. NASA did not lose the technology. Drawings for every part of the Saturn V and Apollo spacecraft exist. We have a bunch of versions of the software for the AGC. We have loads of info on every aspect of the design. Is that enough to start building a new Saturn V tomorrow? No. That's what he was getting at. You'd have to build a factory large enough to assemble a Saturn V. You'd have to build new jigs (because they didn't keep the jigs around, some of those are as large as the first stage). You'd have to replace some of the 1960s era components with new ones: it'd be ridiculous to build new AGCs. So you have to develop new software. The drawings have to be redone in CAD so you can use modern manufacturing processes. All in all, it takes a few years to start up a Saturn V production line, and in that time you could also design a new rocket. This applies to all complex, old projects by the way. B-52, SR-71, the Eiffel tower they would take a long time to replicate, and with today's knowledge we can do better anyway so there's no point. We're building hardware for new moon missions today. 4. That's nonsense. "5th density" is not a radiation measurement. Humans don't disintegrate when exposed to radiation, they get cell damage.
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  883.  @uahoeandabeeetch  Every single one of those documentaries is a pile of nonsense. Debunking 'a funny thing happened on the way to the moon', for instance: https://www.youtube.com/watch?v=8aP_z8F10oQ We figured out how to get through the van Allen belts in 1958. For radiation, there are 2 important variables: 1. the radiation intensity 2. the amount of time you are exposed to this intensity. You can multiply these two and get the total radiation dose. Humans die if they receive a dose of about 300 Rad. In 1958, James van Allen and his team discovered the belts that were later named after him. He also measured the radiation intensity. This is what he found: in the part of the belt where the intensity is highest, it is high enough that if you stay for about a week (inside an Apollo command module), you receive a lethal dose. So for the Apollo missions, the trajectory was designed to minimize the amount of time spent there. The Apollo astronauts flew through the belts in about 3 hours, while avoiding the part with the highest levels entirely. The hull thickness of the CSM was more than enough to reduce the radiation level inside to manageable levels. Astronauts' overall exposure was actually dominated by solar particles once outside Earth's magnetic field. The total radiation received by the astronauts varied from mission-to-mission but was measured to be between 0.16 and 1.14 rads (1.6 and 11.4 mGy). More details in this video from Scott Manley: https://www.youtube.com/watch?v=h9YN50xXFJY So, all you have is arguments from ignorance.
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  952.  @dariusz078  False, false, false and false. 1. No, NASA did not lose any data on the lunar rock samples. Complete information on where they were found, and where they've been since is still available. 2. No, they did not lose a single photograph out of the thousands taken by the Apollo crews. The original film is still kept at JSC. Scans of every single frame at the highest possible resolution are publicly available via the March to the Moon website. That vault also holds all of the 16mm film recorded by the astronauts. Again, high-res digital transfers are publicly available. NASA retains complete recordings of all TV broadcasts, and all of the audio recorded during the mission: not just the radio communications, but recordings made in the CM and LM, and all of the audio from Mission control. There's 19,000 hours of audio for Apollo 11 alone. All publicly available.  3. No, they did not lose transcripts. All of them remain in NASA archives and are available via the Apollo Surface Journal website. 4. The only 'sensor readings' they 'lost' was engineering telemetry that was vital for troubleshooting during the program, but became useless when the Apollo program ended. All of the science data was transcribed and kept, along with medical data, and anything else that continued to have value post-Apollo. We still have every single drawing used to create the Saturn V and Apollo spacecraft. All 6 million of them. We still have thousands of technical reports on every aspect of the program. We still have every single science result from every experiment done by Apollo. We still have all of the lunar rock samples.
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  1018.  @chadsimerson2291  Our atmosphere consists of air, not aether. In medieval science, aether was the hypothesized material that fills the region of the universe beyond the terrestrial sphere, i.e. outside our atmosphere. The concept of aether was used in several theories to explain several natural phenomena, such as the traveling of light and gravity. In the late 19th century, physicists postulated that aether permeated all throughout space, providing a medium through which light could travel in a vacuum. Tesla was a proponent of this idea. The Michelson–Morley experiment proved this hypothesis incorrect. On Earth, a vacuum does not occur because our planet has an atmosphere. Air will rush into any cavity open to the atmosphere. Earth's gravity exerts a force on the atmosphere, keeping the atmosphere together and preventing it from escaping. This is what creates the vacuum of space: all matter gravitates toward planets or stars, leaving the space between them empty. Your reference to an "infinite" vacuum indicates you don't understand the physics involved. A vacuum doesn't exert a force. The only force is exerted by a gas under pressure. On Earth's surface, the air exerts a force of 10E5 N/m2 (or a pressure of 10E5 Pascal - the definition is a pressure of 1 Pa is equal to a force of 1 N/m2)). We don't notice that because there's an equilibrium. When you create a pressure difference, the net force can be calculated by taking the difference in pressure. Let's take a vacuum chamber. A really good one, that can create a perfect vacuum. If the walls of this chamber have a total area of 1 m2, the force exerted is 10E5 Pa minus 0 = 10E5 Pa is 10E5 N/m2. That's the total force acting on the walls of the chamber. The same applies in reverse, in a spaceship in space. Here the pressure inside the pressure hull is 10E5 Pa, and the pressure outside is 0. Again the force on the pressure hull is is 10E5 N/m2. An aluminium cylinder with a wall thickness of 4.8 mm (as used on the ISS) can withstand this force indefinitely. This principle is demonstrated every day by thousands of airliners. The cabin is pressurized to 75 kPa, while the pressure at an altitude of 10 km is 30 kPa. so the difference is 45 kPa. The hull thickness is around 2 mm. Heck, a can of Coke has a bigger pressure difference than the ISS, and that can is so thin you can crush it in you hands once it's empty.
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  1113. That's nonsense. We figured how to get through the van Allen belts in 1958. For radiation, there are 2 important variables: 1. the radiation intensity 2. the amount of time you are exposed to this intensity. You can multiply these two and get the total radiation dose. Humans die if they receive a dose of about 300 Rad. In 1958, James van Allen and his team discovered the belts that were later named after him. He also measured the radiation intensity. This is what he found: in the part of the belt where the intensity is highest, it is high enough that *if you stay for about a week*, you receive a lethal dose. So for the Apollo missions, the trajectory was designed to minimize the amount of time spent there. When the Apollo astronauts flew through the van Allen belts (which took about an hour), they received a dose of radiation of between 0.16 and 1.14 rads, or less than 1% of a lethal dose. That 90% failure rate is cherrypicking. A lot of early unmanned landings failed. The moon was our first target for missions beyond Earth orbit, so there was a lot to figure out. What you're missing is that the success rate climbed rapidly through the 1960s. By 1966, we were making soft landings on the Moon with the Surveyor missions. The Soviets had a lot more failures than the US - they were falling behind in the race to the Moon. these are the simple facts: between 1957 and 1969, we figured how to get to the Moon and return astronauts safely to Earth. Then we did that, with one failure out of 7 missions. The scientific method does not support your view: you're cherrypicking instead of looking at all the data.
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