China is preparing to send a new spacecraft to its orbital station

China is preparing to send a new spacecraft to its orbital station Chinese Central Television announced that his country is preparing to launch a new cargo vehicle towards its national orbital station.  According to the available information, "China is preparing to send the Tianzhou-6 cargo vehicle to its orbital station in the first half of this May, so that this trip will be the first flight of a space cargo vehicle to the station since its official operation in December 2022."  The aforementioned vehicle will carry to the station 70 kg of fresh fruits, food, water, scientific test equipment, and many materials and items necessary for the astronauts to be there. It will also transport a quantity of xenon, which is used as a backup fuel for the electric propulsion systems at the station.  Tianzhou-6 is about 10.6 meters long, weighs 13.5 tons, and can transport 7.4 tons of cargo and payloads to Earth orbits.  The Chinese orbital station currently revolves around the Earth at an altitude of approximately 400 km, and China had indicated earlier that this station is supposed to operate for 10 years in space, on orbits between 340 and 450 km from Earth, and it was designed to have 3 people on board. Pioneers (or 6 Pioneers for a short period in the phase of replacing Pioneer crews), and this station will also be used for international space projects.       A Chinese rover discovers evidence of recent water activity on the Red Planet  The Chinese rover Zhurong has found evidence of liquid water at the low latitudes of Mars.  Scientists have long believed that Mars harbored abundant liquid water some three billion years ago. But dramatic weather changes have frozen much of it, as the ice is now trapped in plumes and has left much of the planet parched.  Now, the Zuurong rover has found evidence of water on sand dune surfaces on modern Mars by providing key observational evidence for liquid water at the low latitudes of Mars, according to a study led by Professor Chen Xiaoguang of the Institute of Geology and Geophysics (IGG) of the Chinese Academy of Sciences (CAS). CAS).  Researchers from the National Astronomical Observatories of the Chinese Academy of Sciences and the Academy's Institute of Atmospheric Physics participated in the study.  The latest findings, published in the journal Science Advances on April 28, from analysis of images and data sent home by Zurong and its orbital companion Tianwen 1 show that notable amounts of water from the planet's icy polar regions flowed into lower latitudes a few million years ago, and settled Over the dunes of Utopia Planitia.  Since landing in the northern hemisphere of Mars in May 2021, the rover has moved near four nearby crescent-shaped dunes in the "Utopia Planitia" region to verify the composition of their surface. All four of the wind-formed miniature geological features are covered with crusts and thin, rift grooves all around formed by the melting of small pockets of "modern water" sometime between 1.4 million years ago to 400,000 years ago, according to the new paper.  Previous studies provided evidence of a large amount of liquid water in early Mars, but as the early Martian atmosphere escaped during the later period, the climate changed dramatically.  The extremely low pressure and water vapor content make it difficult for liquid water to exist sustainably on Mars today. Hence, it was widely believed that water can only exist in solid or gaseous forms.  However, the droplets observed on the Phoenix robotic arm's camera prove that salty liquid water can appear in summer at present-day high latitudes on Mars.  Numerical simulations have also shown that suitable climatic conditions for liquid water can occur briefly in certain regions of Mars today.  So far, though, no evidence of liquid water has been shown at low latitudes on Mars. However, the results obtained from the Zuurong spacecraft fill in this gap.  The researchers used the data obtained by the Navigation and Terrain Camera (NaTeCam), the Multispectral Camera (MSCam) and the Mars Surface Composition Detector (MarSCoDe) on the Zuurong rover to study the various scale surface characteristics and physical compositions of the sand dunes in the landing area. On the southern edge of the plain "Utopia Planitia" (109.925 E, 25.066 N).  They found some important morphological features on the dune surfaces, such as ground crusts, grooves, granules, polygonal ridges and a ribbon-like effect.  Analysis of the spectral data revealed that the surface dune layer is rich in hydrated sulfates, hydrated silica (especially opal-CT), trivalent iron oxide minerals (especially ferrihydrate) and possibly chlorides.  Professor Xiaoguang said: “According to the meteorological data measured by the Zurong rover and other Mars astronauts, we concluded that these dune surface properties are related to the involvement of liquid brine formed from the subsequent melting of frost/snow falling on the salt-containing dune surfaces when the occurrence of cooling".  Specifically, salts in sand dunes cause frost/snow to melt at lower temperatures to form liquid, salty water. When the brine dries, hydrated sulfates, hydrated silica, iron oxide and other hydrated minerals precipitate sand particles to form sand aggregates and even crust. Then the shell cracks as a result of shrinkage.  Subsequent thaw/frost forms further polygonal ridges and streak-like traces on the surface of the crust.  The estimated age of the dunes (about 0.4-1.4 million years) and the relationship between the three phases of water indicate that the movement of water vapor from the polar ice sheet towards the equator during the large deflection phases in the late Martian Amazonian period led to the recurrence of moist environments at low latitudes. Therefore, a scenario for water activity was proposed, that is, cooling at low latitudes during the large tilt phases of Mars leads to frost / snow precipitation, and thus results in the formation of earth crusts and accumulations on the surface of salty sand dunes, thus solidifying the dunes and leaving traces of liquid brine activity.  This discovery provides key observational evidence for liquid water at the lower latitudes of Mars, where surface temperatures are relatively warmer and more suitable for life than at higher latitudes.  "This is important for understanding the evolutionary history of the Martian climate, searching for a habitable environment, and providing key clues for the future search for life," said Professor Chen.

Chinese Central Television announced that his country is preparing to launch a new cargo vehicle towards its national orbital station.

According to the available information, "China is preparing to send the Tianzhou-6 cargo vehicle to its orbital station in the first half of this May, so that this trip will be the first flight of a space cargo vehicle to the station since its official operation in December 2022."

The aforementioned vehicle will carry to the station 70 kg of fresh fruits, food, water, scientific test equipment, and many materials and items necessary for the astronauts to be there. It will also transport a quantity of xenon, which is used as a backup fuel for the electric propulsion systems at the station.

Tianzhou-6 is about 10.6 meters long, weighs 13.5 tons, and can transport 7.4 tons of cargo and payloads to Earth orbits.

The Chinese orbital station currently revolves around the Earth at an altitude of approximately 400 km, and China had indicated earlier that this station is supposed to operate for 10 years in space, on orbits between 340 and 450 km from Earth, and it was designed to have 3 people on board. Pioneers (or 6 Pioneers for a short period in the phase of replacing Pioneer crews), and this station will also be used for international space projects.


Pedrosa got a new experience when he "comeback" to MotoGP in Spain  Jakarta (ANTARA) - Motorcycle racer Daniel "Dani" Pedrosa revealed that he gained new experiences and learned many things when he returned to the MotoGP event in Spain last weekend with the KTM racing team, with wildcard status .  Pedrosa, who finished seventh in the main race and sixth in the Sprint race, said the performance of the motorbike he was riding was quite good, especially as two other KTM riders, Brad Binder and Jack Miller, also got podiums in the two race sessions.  “I can take two things from this weekend's race. One is the technical side and all the things that I can pass on to the testing team and we can keep in mind for the next stage of our work. There are also amazing results from friends!” Pedrosa said, quoted from KTM's official statement, Tuesday.  “The second thing is how the people (fans) are still together and cheering me on. It's hard to believe. I'm just trying to give my best and I hope the fans like it. I think we are getting stronger as a project and the bike is improving step by step."  Meanwhile, Red Bull KTM Team Manager Francesco Guidotti added that the positive achievements of the team and the three riders made him more confident to wade through MotoGP this season.  “What a weekend. We started the Grand Prix in a great way with Dani and then qualifying went perfect too, we won the Sprint race and the main race was great. We did something special: both riders fought for victory, led most of the way and took two places on the podium," said Guidotti.  Furthermore, he thanked everyone involved in this project. Guidotti said all those who support are very committed even though they are under pressure to continue to improve the performance of the motorbike and engine.  “Time is running so fast so I'm happy we started to show something important. We had red flags and it even rained at one stage so it's been an intense weekend here. Technicians, designers, mechanics, riders, test team; thank you all for this great result. We are looking ahead and we are confident," said Guidotti.            Federal Oil hopes that its two racers will again win points at the Le Mans GP  Jakarta (ANTARA) - PT ExxonMobil Lubricants Indonesia (PT EMLI) through Federal Oil hopes that its two racers from the Gresini Racing team, namely Alex Marquez and Fabio Di Giannantonio, can again secure points when racing at the Le Mans Circuit, France, in two weeks.  This hope was given after the two drivers won eight points and four points respectively, the results of the sprint race and main race at the Jerez Circuit, Spain, last Sunday (30/4).  These points were obtained after Alex finished in eighth position (8 points) Di Giannantonio finished in 12th position (4 points).  In the sprint race itself, the two of them did not get any points because Alex fell, while Di Giannantonio, or Diggia as he is familiarly called, was only able to finish in 11th position.  "Overall Alex Marquez and Fabio Di Giannantonio tried hard to get the best results at the Jerez Circuit, Spain," said Rommy Averdy as Consumer Brand General Manager of PT EMLI in an official statement.  “Federal Oil hopes that the two drivers can perform even more optimally in the next series at the Le Mans Circuit, France. Hopefully we can get a double podium for the first time for the team and also for the fans in Indonesia."  This additional race point in Spain made Alex sit in 10th position in the MotoGP standings with 41 points, while his Italian teammate is in 16th position with 17 points.  On the same occasion, Alex was in the sprint raceexperienced a crash , said that now he is focused on gaining a lot of points, considering that the 10th position to the fourth position is only eight points apart, in which position is occupied by a racer from Australia Jack Miller.  "We should be happy, I never felt comfortable on the bike after yesterday's crash and today's hot weather, but today's aim was to stay upright and get more points," said rider number 73.  "Between fourth and tenth in the standings are very close in points," he continued.  The younger brother of Marc Marquez added that he would learn more about the motorbike he was riding in order to get the best results in the next MotoGP race series at Le Mans later.  "Continuing the test will be useful to learn more about the motorbike and be better prepared to face the Le Mans Circuit," he added.  Rider number 49, Diggia admits that he also wants to learn more about his motorbike in order to get a comfortable ride and of course the best results for navigating the next series of MotoGP.  "The test will be very important because we will try many things such as the settings of the motorbike, ergonomics and try to take advantage of time by adjusting many components while still feeling more comfortable on the motorbike according to the recommendations of experts from the mechanics team," said Diggia.  The fifth MotoGP 2023 series will take place at the Le Mans Circuit, France, next week on May 14.  Meanwhile, from the previous four MotoGP series Francesco Bagnaia won twice (Algarve Circuit and Jerez Circuit), Marco Bezzecchi won once (Termas de Rio Hondo Circuit), and Alex Rins won once (The America Circuit).          Kemenpora will collaborate in organizing Formula E Jakarta  Jakarta (ANTARA) - Minister of Youth and Sports of the Republic of Indonesia (Menpora RI) Dito Ariotedjo said he would collaborate in holding the 2023 Jakarta Formula E World Championship.  He conveyed this when receiving an audience with the Chairperson of the Jakarta Formula E 2023 Committee Ananda Mikola with Race Leader Bagoes Hermanto, and Managing Director of Jakarta Propertindo (Jakpro) Iwan Takwin in the Meeting Room Floor 10 of the Ministry of Youth and Sports Office, Senayan, Jakarta, Tuesday.  "Later we will support Insha Allah, and later we will try to collaborate," said Menpora Dito, responding to an explanation regarding the readiness of the entire event starting from tickets, side events, volunteers and so on, as published on the official website of the Indonesian Ministry of Youth and Sports, Tuesday.  During the visit, Ananda Mikola reported on the progress of Indonesia's preparations to host the 2023 Formula E which will be held at the Jakarta International E-Prix Circuit (JIEC), Ancol, North Jakarta.  "The 2023 Formula E world championship will be held on 3-4 June 2023. Indonesia has also been entrusted with hosting two series (series 10 and series 11), last year we only had one series," said Ananda.  According to him, besides being quite good at organizing Formula E the previous year, the FIA ​​sees Indonesia as the best organizer of all the series that have been held since 2015.  "For this year, we hope to be able to repeat the success like last year. In terms of spectators and the course of the event. Last year there were 400 children of the nation who worked as RC (Racing Community), that was the heart of the event. Their job was to supervise the running of the race as marshals and everything else," said Ananda.  "The hope is that the government can continue to support this event, this is Indonesia's face in the eyes of the world, this is a world championship equivalent to Formula 1. In the future this automotive sport will use go green or electricity and this will also be a campaign for the G-20 countries. We invite the Minister to attend to check the readiness," he added.  As is well known, FIA Formula E has released the ninth season racing calendar for 2023. In this calendar, Formula E 2023 in Jakarta will be held for two days, namely on the 3-4 June 2023. The implementation was after the event in Monaco on May 6.

A Chinese rover discovers evidence of recent water activity on the Red Planet


The Chinese rover Zhurong has found evidence of liquid water at the low latitudes of Mars.

Scientists have long believed that Mars harbored abundant liquid water some three billion years ago. But dramatic weather changes have frozen much of it, as the ice is now trapped in plumes and has left much of the planet parched.

Now, the Zuurong rover has found evidence of water on sand dune surfaces on modern Mars by providing key observational evidence for liquid water at the low latitudes of Mars, according to a study led by Professor Chen Xiaoguang of the Institute of Geology and Geophysics (IGG) of the Chinese Academy of Sciences (CAS). CAS).

Researchers from the National Astronomical Observatories of the Chinese Academy of Sciences and the Academy's Institute of Atmospheric Physics participated in the study.

The latest findings, published in the journal Science Advances on April 28, from analysis of images and data sent home by Zurong and its orbital companion Tianwen 1 show that notable amounts of water from the planet's icy polar regions flowed into lower latitudes a few million years ago, and settled Over the dunes of Utopia Planitia.

Since landing in the northern hemisphere of Mars in May 2021, the rover has moved near four nearby crescent-shaped dunes in the "Utopia Planitia" region to verify the composition of their surface. All four of the wind-formed miniature geological features are covered with crusts and thin, rift grooves all around formed by the melting of small pockets of "modern water" sometime between 1.4 million years ago to 400,000 years ago, according to the new paper.

Previous studies provided evidence of a large amount of liquid water in early Mars, but as the early Martian atmosphere escaped during the later period, the climate changed dramatically.

The extremely low pressure and water vapor content make it difficult for liquid water to exist sustainably on Mars today. Hence, it was widely believed that water can only exist in solid or gaseous forms.

However, the droplets observed on the Phoenix robotic arm's camera prove that salty liquid water can appear in summer at present-day high latitudes on Mars.

Numerical simulations have also shown that suitable climatic conditions for liquid water can occur briefly in certain regions of Mars today.

So far, though, no evidence of liquid water has been shown at low latitudes on Mars. However, the results obtained from the Zuurong spacecraft fill in this gap.

The researchers used the data obtained by the Navigation and Terrain Camera (NaTeCam), the Multispectral Camera (MSCam) and the Mars Surface Composition Detector (MarSCoDe) on the Zuurong rover to study the various scale surface characteristics and physical compositions of the sand dunes in the landing area. On the southern edge of the plain "Utopia Planitia" (109.925 E, 25.066 N).

They found some important morphological features on the dune surfaces, such as ground crusts, grooves, granules, polygonal ridges and a ribbon-like effect.

Analysis of the spectral data revealed that the surface dune layer is rich in hydrated sulfates, hydrated silica (especially opal-CT), trivalent iron oxide minerals (especially ferrihydrate) and possibly chlorides.

Professor Xiaoguang said: “According to the meteorological data measured by the Zurong rover and other Mars astronauts, we concluded that these dune surface properties are related to the involvement of liquid brine formed from the subsequent melting of frost/snow falling on the salt-containing dune surfaces when the occurrence of cooling".

Specifically, salts in sand dunes cause frost/snow to melt at lower temperatures to form liquid, salty water. When the brine dries, hydrated sulfates, hydrated silica, iron oxide and other hydrated minerals precipitate sand particles to form sand aggregates and even crust. Then the shell cracks as a result of shrinkage.

Subsequent thaw/frost forms further polygonal ridges and streak-like traces on the surface of the crust.

The estimated age of the dunes (about 0.4-1.4 million years) and the relationship between the three phases of water indicate that the movement of water vapor from the polar ice sheet towards the equator during the large deflection phases in the late Martian Amazonian period led to the recurrence of moist environments at low latitudes. Therefore, a scenario for water activity was proposed, that is, cooling at low latitudes during the large tilt phases of Mars leads to frost / snow precipitation, and thus results in the formation of earth crusts and accumulations on the surface of salty sand dunes, thus solidifying the dunes and leaving traces of liquid brine activity.

This discovery provides key observational evidence for liquid water at the lower latitudes of Mars, where surface temperatures are relatively warmer and more suitable for life than at higher latitudes.

"This is important for understanding the evolutionary history of the Martian climate, searching for a habitable environment, and providing key clues for the future search for life," said Professor Chen.

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