Tag: Change 4 Luna Lander

#CNSA #ChinaNationalSpaceAdministration #国家航天局 |#BeltAndRoadinitiative #CLEP #June2022 | #VonKarmanCrater #LunarMission #Change4 #Yutu2 #ChineseAcademyOfSciences Research Reveals the Constraints of the Chang’e-4 Infrared Imaging Spectroscopic Ground Validation Experiment on the Material Composition of the Lunar SPA Surface…

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As of Month of April 2022, The CNSA –China National Space Administration CLEP- China Lunar Exploration Program  Belt and Road Initiative Lunar Mission……Chang’e-4 with Yutu two the Lunar rover still working exploring more than moved more than 1142.39 meters on the other side of the moon on the 103 Kilometers Diameter Von Karman Crater in which is least than two length by length fifty five Kilometers Hong Kong –Macau- Zhuhai Bridges …. Working Exploring the Crater on the other side of the Moon Chang’e Luna….

On 27th June 2022 the Chinese Academy of Sciences Research Reveals the Constraints of the Chang’e-4 Infrared Imaging Spectroscopic Ground Validation Experiment on the Material Composition of the Lunar SPA Surface

The Infrared Imaging Spectrometer (VNIS) on the Yutu No. 2 Lunar Rover has measured infrared imaging spectral data at multiple locations along the rover’s walking route. VNIS is the main method used to study the composition of lunar soil and lunar surface rocks in the landing area and to trace their origin. The research of the Institute of Geology and Earth Sciences, Chinese Academy of Sciences revealed the constraints on the composition of the lunar SPA surface by the Chang’e-4 infrared imaging spectroscopy ground verification experiment.

The Yutu-2 rover has been working on the lunar surface for more than 40 months, and the infrared imaging spectrometer (VNIS) it carried has measured infrared imaging spectral data at multiple locations along the rover’s walking route. VNIS is the main method used to study the composition of lunar soil and lunar surface rocks in the landing area and to trace their origin. However, factors such as space weathering, particle size and multiple scattering, the spectral response of the instrument, and observation conditions all affect the spectral characteristics and lead to large uncertainties in the mineral composition calculated from the lunar surface spectral data.

　　In order to quantitatively evaluate the reliability of different VNIS data processing methods, Chang Rui, a doctoral student in the Key Laboratory of Earth and Planetary Physics, Institute of Geology and Geophysics, Chinese Academy of Sciences, under the guidance of his supervisor researcher Yang Wei and associate researcher Lin Honglei, selected a mineral composition with Spectroscopic ground verification experiments were performed on the Suchang-gabbro with similar lunar highland rocks (Fig. 1). The rock (CR-1) studied by the ground verification experiment has an actual mineral pattern content of 12.9% olivine, 35.0% pyroxene and 52.2% plagioclase, as measured by scanning electron microscopy. In order to more accurately calculate the spectral results of CR-1, the researchers ground and sorted the olivine, low-calcium pyroxene, high-calcium pyroxene and plagioclase from the rock samples in CR-1. -4, ASD) to measure the visible-near-infrared spectral results of each single mineral (Fig. 2a), and each single mineral has its own spectral absorption characteristics. The spectrum of CR-1 measured by the VNIS identifier showed distinct absorption features at the 971 (±1) nm and 1957 (±8) nm bands (Fig. 2b). This absorption feature is similar to the rock absorption feature detected by VNIS on the Yutu-2 rover on the third day of the month. The Hapke model of the VNIS spectrum of CR-1 calculated the mineral pattern content of the sample to be 7.5% olivine, 39.3% pyroxene and 53.2% plagioclase, which were consistent with the true results within the error range.

　　According to the data processing method in this study combined with the photometric correction of the Chang’e-4 lunar surface data by Yang et al. (2020), the more accurate mineral model content of the rocks detected by the Yutu-2 rover on the third day should be 11.7 % olivine, 42.8% pyroxene and 45.5% plagioclase. The rover found another lunar surface rock on the 26th day with spectral absorption characteristics similar to those found on the 3rd day, with mineral pattern contents of 3.2% olivine, 24.6% pyroxene, and 72.2% plagioclase. The two lunar surface rocks belong to the sutraite category in the “Anorthosite-Norite-Troctolite” (ANT) system (Fig. 3) (Heiken G, 1991), which means that the Chang’e-4 landing area lunar The rock formations under the soil are mainly ANT rocks. The rocks detected by the Yutu-2 rover on the 26th day contained more plagioclase and were closer to the mineral composition of the average lunar crust.

　　To sum up, the lunar surface of the Chang’e-4 landing area has su-long and plagio-like rocks, which represent the material formed by the rapid crystallization in the impact melting pool and the composition of the average lunar crust, respectively. On the one hand, an impact event excavated material from the underlying layers of lunar soil to the lunar surface. These excavated materials have the characteristics of crystalline plutonic rocks in the molten pool of the South Pole Aitken Basin (SPA). On the other hand, the initial lunar crustal material formed before the SPA big impact event can also be retained in the SPA.

　　The related research results were published in Remote Sensing . The research work has been funded by the Strategic Pilot Science and Technology Project of the Chinese Academy of Sciences, the Key Deployment Project of the Chinese Academy of Sciences, the Innovation Interdisciplinary Team of the Chinese Academy of Sciences, the Civil Aerospace Pre-research Project of the National Space Administration, and the Key Deployment Project of the Institute of Geology and Geophysics of the Chinese Academy of Sciences.

Figure 1. (a) The image of the lunar surface rock detected by Chang’e-4 on the third month; (b) the spectral detection status of the lunar surface rock (the yellow circle represents the near-infrared spectral detection field); (c) the ground verification of this study The rock used in the experiment (CR-1)

Figure 2. (a) Visible-NIR spectra of single minerals in CR-1; (b) VNIS spectra of rocks and CR-1 measured on the third day of Chang’e-4

Fig. 3. Mineral composition distribution of olivine-pyroxene-plagioclase in lunar surface rocks measured by Chang’e-4 (Heiken G, 1991). The lunar sample sampling points are marked in the figure, for example: A-11 is Apollo 11, L-16 is Luna 16, (H) and (M) represent high ground and lunar soil, respectively

Images and visuals are from their Respectives source Chinese Academy of Sciences .. 52 Sanlihe Rd., Xicheng District, Beijing, China (100864)- People’s Republic of China.

#CNSA #ChinaNationalSpaceAdministration #国家航天局 |#BeltAndRoadinitiative #CLEP #April2022 | #VonKarmanCrater #LunarMission #Change4 #Yutu2 Lunar adventuring the latest research results of Chang’e-4 featured on #ScienceRobotics #ScientificExploration …..

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As of Month of April 2022, The CNSA –China National Space Administration CLEP- China Lunar Exploration Program  Belt and Road Initiative Lunar Mission……Chang’e-4 with Yutu two the Lunar rover still working exploring more than moved 1142.39 meters on the other side of the moon on the 103 Kilometers Diameter Von Karman Crater in which is least than two length by length fifty five Kilometers Hong Kong –Macau- Zhuhai Bridges …. Working Exploring the Crater on the other side of the Moon Chang’e Luna….

Figure 1 The trajectory of the “Yutu” 2 lunar rover (cover of Science Robotics magazine)

​​ The latest research results of Chang’e-4 …..At the beginning of 2022, by the State Key Laboratory of Robotics and Systems of Harbin Institute of Technology, Beijing Aerospace Flight Control Center, State Key Laboratory of Remote Sensing Science, Institute of Aeronautical and Astronautical Information, Chinese Academy of Sciences, China Academy of Space Technology, Ryerson University in Canada, etc. A number of units cooperated and published the title of “A 2-year locomotive exploration and scientific investigation of the lunar farside by the Yutu-2 rover” in the internationally renowned academic journal “Science Robotics”. and Scientific Exploration)” cover paper.

Fig. 2 Analysis of physical and mechanical properties of lunar soil based on “Yutu” 2 wheel-earth interaction

The team estimated the mechanical properties of the lunar soil based on the information on the interaction between the lunar rover wheel and the lunar surface and the ground mechanical model. The results show that the pressure-bearing properties of the lunar soil regolith are similar to the dry sand and sandy loam on the earth, and are similar to those in the American Apollo program. Compared with typical lunar soil, it has stronger pressure bearing characteristics. Large lumps of soil were observed adhering to the wheels of “Yutu 2” in images from different locations, while the wheels of “Yutu 2” basically had no clay phenomenon, indicating that the lunar soil cohesion near the landing area of ​​Chang’e 4 is relatively large , the reason may be that it contains a higher proportion of aggregates, which makes soil particles more likely to agglomerate after being rolled by wheels.

Figure 3 The impact craters and rocks discovered by the “Yutu-2” observation

The research is based on my country’s lunar exploration missions and faces engineering scientific issues. The relevant results can provide theoretical and technical support for future lunar exploration missions. This research was supported by the National Natural Science Foundation of China (51822502, 91948202, 41771488), the National Key Research and Development Program (2019YFB1309500), and the “111” Innovation and Talent Introducing Program (BP0719002). The link to the original publication of the results: https://www.science.org/doi/10.1126/scirobotics.abj6660
At present, Chang’e-4 is on the 41st night of the moon. The rover has moved 1142.39 meters, and the two devices and one satellite are in good condition.

Images and visuals are from Chinese lunar exploration project  CNSA- China National Space Administration also from their respectives…!

#CNSA #ChinaNationalSpaceAdministration #国家航天局 |#BeltAndRoadinitiative #CLEP #February2022 | #VonKarmanCrater #LunarMission #Change4 #Yutu2 Lunar adventuring #LunaExploration recently discovered explorationally of macroscopic translucent glass globules Stalagmite detected..

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As of Month of January  2022, The CNSA –China National Space Administration CLEP- China Lunar Exploration Program  Belt and Road Initiative Lunar Mission……Chang’e-4 with Yutu two the Lunar rover still working exploring more than 1003.9 meters on the other side of the moon on the 103 Kilometers Diameter Von Karman Crater in which is least than two length by length fifty five Kilometers Hong Kong –Macau- Zhuhai Bridges …. Working Exploring the Crater on the other side of the Moon Chang’e Luna….

On the 19th February 2022 week Hong Kong SAR – Beijing Time CNSA CLEP – China National Space Administration –China Lunar Space Program has released the 23rd batch of scientific data released by Chang’e-4 this month’s data came relatively late, but the content is very rich. More than 240 photos include more than 30 color photos. The data collection time announced this time is during the day of the 27th month (2021.02.04~2021.02.19).

is in the last month day In , experts analysed a “milestone” shaped stone, which, in fact, wasn’t the only similarly shaped stone nearby. Just south of the “milestone”, there is another similar stone, which the driving team calls a “stalagmite”, the relationship between the two is marked in Figure 1 (map from Chapter 27 of the Driving Diary). The focus of this moon and day detection is on this “stalagmite”, and the specific process is full of twists and turns. It is recommended that you read the original text of “Driving Diary”. Data source: Lunar and Planetary Data Release System

At 4:32 on February 6 2022 Hong Kong SAR- Beijing Time, Yutu-2 successfully woke up and entered the 27th lunar day, during which it spent its third Spring Festival on the moon.

Last month, we detected the “milestone” rock. Once the news came out, it attracted the attention of scientists all over the world. Dan Moriarty, a researcher at NASA, said: “This rock sample has Similar to the shape of a shark fin, it’s definitely unusual. ” He said that both the shape of the shark fin, and the apparent bulge near the edge of the rock, indicate a very young geological age and a relatively short existence at the site where it was found. Clive Neal, a famous lunar expert at the University of Notre Dame in the United States, also expressed his views on the rocks. While the “milestone” has attracted the attention of the international aerospace science community, Chinese scientists are gradually unravelling the mystery of its identity.

Strange discoveries always come in pairs. Last month, the pilots found a “stalagmite” shaped stone standing in the south direction, similar to the “milestone” shape. The two echoed each other. Everyone decided to act immediately and explore again. “Stalagmite”.

The rhythm of the whole moon, day and morning was tight and orderly. After three moves, Yutu No. 2 arrived near the “stalagmite” before noon on the moon. At this time, the shadow of the car body blocked the target, and it seemed to persuade Yutu to take a nap and explore the “stalagmite” again. , we had to wait for the Yutu to wake up from the lunch break to continue the probe.

Under the scorching sun, Jade Rabbit spent its Spring Festival, and before the fifth day of the first lunar month, it started work early in the day and afternoon. The pilots controlled Yutu-2 to turn to the intended detection heading. According to the previous ground planning path deduction, the road detected at this time is flat, and the bright surface of the “stalagmite” should be able to enter the infrared field of view. However, the obstacle-avoidance images downloaded to the ground are full of artistic “alternation of light and dark”, which is different from the “simple and straightforward” that scientists hoped to be completely illuminated by sunlight.

There are so many exciting moments in lunar exploration. It is within reach, but it seems to be so far away. However, the pilots have been very patient in the long-term detection, and proposed three detection plans for the current situation: go straight ahead, detour to the southwest side of the “stalagmite”, and detour to the southeast to wait for next month’s detection.

Here are a few photos synthesized from the original images:
Figure 2: Color photos of the “Milestone” taken from a distance
Figures 3 and 4: The lunar image taken by Yutu-2 to the “Stalagmite” (you find the Chang’e-4’s photo) Is the lander yet?)
Figure 5: A close-up photo of the “stalagmite”

After repeated deductions and demonstrations, the last plan was not very feasible and was first excluded, and the remaining two plans entered the final PK. Drivers detour from the west side and the southeast side to verify the feasibility of the second option. Detouring from the southeast, there are many potholes along the way. After starting, Yutu No. 2 will step into the pit, which is more dangerous; while the west side seems to be flat along the way, but there is a large impact crater near the end position. Yutu No. 2 The No. 1 can only move around in a small area between the impact crater and the “stalagmite”. Not only is its range of activity severely limited, which may cause the solar wings to be blocked, but it must also return to the original path after detection, which is laborious and dangerous. After several rounds of calculation and demonstration, direct detection wins.

The pilots controlled the Yutu for the first attempt. The preliminary results show that the actual infrared field of view is about 4 cm away from the ideal field of view. The second time, everyone adjusted according to the suggestions of the scientists and tried again, but the results were still biased. The two failed attempts, and the time was approaching zero, and the station resources were almost exhausted. Facing the temptation of the mystery behind the moon, the pilots were still reluctant to give up and decided to try again. They urgently extended the measurement and control arc for an hour, adjusted the posture of the jade rabbit and probed again. With all the hard work, the images uploaded this time show that the infrared field of view finally accurately covers the narrow light of the “stalagmite” !

Those who travel a hundred miles are half and ninety. When it is unknown whether success or failure will come next time, persevering may be our only chance. This time Yutu No.2 and the pilots did it! Next time, would you like to challenge and persevere for your dreams?

Images and visuals are from CNSA- China National Space Administration also from their respectives…

#CNSA #ChinaNationalSpaceAdministration #国家航天局 |#BeltAndRoadinitiative #CLEP #August2021 | #VonKarmanCrater #LunarMission #Change4 #Yutu2 Lunar adventuring #LunaExploration still Exploring working with newly recently release Lunar Photography images.. #AGallery

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As of 7th August 2021, The CNSA –China National Space Administration CLEP- China Lunar Exploration Program  Belt and Road Initiative Lunar Mission……Chang’e-4 with Yutu two the Lunar rover still working exploring more than 708 meters on the other side of the moon on the 103 Kilometers Diameter Von Karman Crater in which is least than two length by length fifty five Kilometers Hong Kong –Macau- Zhuhai Bridges ….

Today The team of the Lunar Exploration Engineering Ground Application System recently announced a new batch of scientific data on Chang’e-4 on the website. Among them, the panoramic camera part of the patrol has a total of about 400 photos, and some of them are selected and put up here.


Most of this batch of photos was taken between July 16th and August 23rd, 2020, and they were taken in full-color mode, so they were black and white photos after processing, but they also magically “included” two Color photo taken on February 7, 2021 (the last two). The photos can be seen from the surface of the moon is really timeless scientifically wild in exploration with wonder, in that wondering hopefully with the Mars rover photographically images data could be fully disclosure….  

Also worth mentioning is the original “lunar exploration data publishing and information service system” website is now fully Revised and renamed “Moon and Planetary Data Release System”, with two different data release pages for “Moon” and “Mars”. At present, the Mars data part is in the protection period application status. Looking forward to the data and images from Tianwen-1 Full disclosure…..

Images and visuals are from CNSA- China National Space Administration also from there respectives…!

#CNSA #ChinaNationalSpaceAdministration #国家航天局 |#BeltAndRoadinitiative #CLEP #Apirl2021 | #VonKarmanCrater #LunarMission #Change4 #Yutu2 Lunar adventuring #LunaExploration Summary awakened smoothly and entered the 29th month day work period back to work …..!

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As of 7th April 2021, The CNSA –China National Space Administration Belt and Road Initiative Lunar Mission……Chang’e-4 successfully awakened completed the 29th day At the time when China Land Spring and Jingming, on the far side of the moon, sunlight again spread on the Chang’e 4 lander and the “Yutu 2” lunar rover, which were at 21:43 and 3 o’clock on April 6th. 54 minutes to end the moon night dormancy, awakened autonomously by light, and entered the 29th month day work period. Up to now, Chang’e-4 has spent 825 Earth days on the back of the moon.

As shown in Figure 1, the patrol is currently located at LE02805, which is located in the northwest direction of the landing site of Chang’e 4, which is about 455 meters straight from the landing point, and the travel path of the patrol is about 682.8 meters. Based on the LE02805 point panoramic camera stitched image, DOM image and other data, the lunar rover will continue to move towards the basalt distribution area (about 1.2km from the current patrol device, located at 177.5389° east longitude, near 45.4119° south latitude) during the 29th day of the month. The location is located northwest of the current detection point. Related scientific results will be released in time.

Work planned for this month:

(1) The panoramic camera carries out ring shooting detection;

(2) Infrared imaging spectrometer to carry out calibration and scientific detection;

(3) Neutral Atomic Sounder (ASAN) to carry out scientific detection;

(4) The moon-measuring radar conducts simultaneous detection of the path area during driving.

Previously ….As of 22th March 2021 Monday, The CNSA –China National Space Administration Belt and Road Initiative Lunar Mission……Chang’e-4 successfully awakened completed the 28th day of the work period after the Chinese Lunar New Year – year of the OX  got  back to work  Chang’e 4 completed the 28th day of work……. The Chang’e 4 lander and the “Yutu 2” lunar rover finished their 28th day of work at 2 o’clock on March 21 and at 17:09 Hong Kong – Beijing Time  on March 20, and entered the moon night Hibernate. Up to now, the Chang’e 4 lander and the “Yutu-2” lunar rover have survived 808 Earth days on the moon. The lunar rover travelled about 30 meters during the day and the accumulated mileage was 682.77 meters…

Images and visual are from Weibo..