NASA plans to submit the first manned missions to Mars by its Moon to Mars program by the end of the next decade.
According to RCO News AgencyNASA is examining advanced technologies through numerous programs to realize this bold vision. These technologies include advanced propulsion systems that reduce the time to travel to Mars and reduce astronauts exposed to its micro -radiation and radiation.
Other technologies studied include methods for removing waste, water reproduction, health and safety crew and self -sufficiency.
NASA is also trying to develop key technologies. These technologies allow low -cost exploration missions to Mars and across the solar system.
The most importa technology considered is the electrical propulsion systems less than 5 kg for small spacecraft.
In an article preseed at the 56th Lunar and Planetary Science Conference, a team of NASA researchers proposed a new initiative. The initiative was the “Hall’s propulsion work for freight services to the planet Mars.”
This study was conducted by NASA researchers. Researchers in the team include NASA engineers in the common areas that examine the unified carrier systems.
Technology Gap
As researchers poi out, their study is based on previous studies. These studies proved the importance of “HET Effects” with low power and high efficiency and magnetic protection optimization.
These propulsion systems rely on solar energy or another source of energy. These systems are also used to produce drift force by magnetic fields.
“Hall’s Blinders” are a type of ion that accelerates the rocket fuel by an electric field.
According to the Artemis Space Program, these systems direct the two primary modules of the Lunar Gateway, the PPE and the Halo (Halo) module (PPE) and the Halo (Halo) module.
The mission is scheduled for year 2, and both elemes will be thrown from Earth to the moon by Falcon Heavy. Upon arrival, the “PPE” and “Halo” modules will rely on their powerful “solar electrical propulsion” (SEP) systems to create a “nrho).
Unfortunately, this field has a technology gap, meaning that technology has not yet been able to do it. So NASA launched a “SMSEP) project in year 2. The project aims to develop small versions of the most advanced SEP systems.
The curre “H3M” system is a high -performance small version of “SEP”. NASA began cooperation and licensing for “H3M” with business partners. This led the researchers to develop the idea of a Champs mission to Mars.
This study seeks to build a spacecraft using the commercial version of “H3M”. These missions will rely on freque and less expensive throwing opportunities.
The concept of mission
One of the biggest challenges for lower -cost scieific missions and smaller spacecraft is to ideify and adhere to a specific time to launch the carrier on Mars. Usually the carrier launch as the main cargo is costly, and the carrier launch as a secondary cargo can have consequences, as the main cargo requires the date and path of the launch. In addition, the date of launch cannot always be changed.
The Champs architecture resolves the problem by launching a carrier as a secondary cargo on the “CLP” mission.
Scieists expect these missions to carry cargo regularly to the moon in the coming years. The launch route is well determined and there are many alternatives. This mission can do tools by observing the moh.
The mission also provides a gravitational help to increase acceleration. This maneuver or practice allows the mission to temporarily place itself in a “NHRO” around the moon uil a favorable synergy between the Earth and Mars occurs.
The first maneuver with the drift force will take about three mohs. Upon arriving at Mars, the spacecraft will be located at a height of 2 kilometers above Mars. In this maneuver, many scieific goals can be achieved by studying Deimos. After two years, the spacecraft will reach an orbits of 2 kilometers above Mars.
Tools and goals
The “Champs” mission will conduct numerous scieific studies using various tools. These tools include a visible/ultraviolet illustrator, “Mars Ideification Orbiter” (MRO), “Heat Frame Radio” (TIR) and NIR Spoketer (NIR).
Using these tools, the “Champs” mission can measure the 3D structure of the atmosphere. The behavior and changes of dust and ice clouds can also be observed. These observations can give scieists more about the climate patterns of the planet and seasonal dust storms.
These tools can also measure the plasma conditions and the magnetic field structure around Mars and how it ieracts with the “EUV” radiation (EUV).
These studies allow scieists to examine key scieific questions about Mars’ climate, how to connect the various atmospheric surfaces on the planet, and how the space weather affects the atmosphere of the planet.
The team also pois out that their proposal is in line with NASA’s “Mars Exploration Program” (MEP).
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