Tag Archives: orbit

CAN YOU PROVIDE MORE DETAILS ABOUT THE TRAJECTORY THAT CAPSTONE WILL FOLLOW TO REACH ITS INTENDED ORBIT

Capstone’s journey starts with a launch on a Rocket Lab Electron rocket from the company’s Launch Complex 1 on Mahia Peninsula in New Zealand. The Electron rocket will place Capstone into an elliptical transfer orbit with a low point, or perigee, of approximately 500 km and a high point, or apogee, of over 35,000 km after separating from the rocket’s second stage.

From this initial transfer orbit, Capstone will use its onboard electric propulsion system to gradually increase its orbit over several months. The spacecraft is equipped with a Hall effect thruster powered by kW-class solar electric propulsion. Hall thrusters accelerate ions using electric and magnetic fields to produce thrust efficiently over long periods of time with minimal propellant requirements. This propulsion method allows Capstone to slowly spiral its orbit outward through low-thrust maneuvers without needing chemical propellant burns common to traditional chemical rockets.

Once separated from the rocket, Capstone’s solar panels will deploy and begin recharging its onboard batteries to power the electric thruster. Over the course of several months, the spacecraft will make a series of short thruster burns to raise the low point of its orbit each revolution. During the first few weeks, the thruster will fire as needed to circularize the transfer orbit to approximately 1,000 km altitude. From this vantage point, mission controllers will check out the spacecraft and electric propulsion system in detail.

With the checkouts complete, a series of about 140 thruster burns over the next 3-4 months will systematically raise Capstone’s apogee to match the target lunar orbit altitude. The duration of each individual burn ranges from a few minutes to a couple hours with breaks in between as the spacecraft travels around the Earth. The increasing apogee altitude efficiently increases the overall orbital energy through these low-thrust maneuvers without requiring a high output chemical engine. By late 2022, the final apogee raise maneuvers will achieve the target altitude of over 54,000 km to complete the Earth orbital phase.

At the point when Capstone’s elliptical orbit passes through the location of the Moon’s orbit once per revolution, known as the orbital resonance point, the electric thruster will fire to perform the lunar orbit insertion burn. This multi-hour burn executed near the Moon’s location will change the orbit plane and reduce velocity just enough for lunar gravity to capture the spacecraft. After orbital insertion, Capstone will be in an elliptical lunar orbit approximately 500 km by 80,000 km, similar to the target rectilinear halo orbit but with higher perigee and apogee distances.

Over the following month, frequent but short electric thruster burns will fine tune the orbit, systematically decreasing both perigee and apogee altitudes to precisely match the target near rectilinear halo orbit parameters. The complex 6-dimensional orbital elements of inclination, right ascension of the ascending node, argument of perigee, mean anomaly, semimajor axis, and eccentricity must all be adjusted in tandem through coordinated thruster firings. Telemetry from Capstone will be closely monitored during orbit adjustment to precisely hit the desired orbital parameters.

When complete, Capstone will be in a halo orbit around the Earth-Moon L1 Lagrange point with a nominal altitude of just 10 km from the target orbit. At this point in late 2022, the technology demonstration mission objectives will be considered achieved with the spacecraft positioned in its optimum vantage point to characterize the dynamics and environment of this unique orbit. Capstone will then begin on-orbit operations to gather data for at least 6 months to validate the viability and performance of smallsat operations in cislunar space.

This ambitious but efficient trajectory allows a small spacecraft like Capstone to reach the first stable halo orbit around the Moon’s nearest Lagrange point using nothing but sunlight and low-thrust electric propulsion. The step-by-step process of raising unique transfer and intermediate orbits systematically injects just the right amount of orbital energy to place the probe into its destination six months after launch. The trajectory was optimized through extensive mission design and modeling to fulfill the technology demonstration goals while minimizing propellant mass and launch vehicle capability requirements. If successful, Capstone will pave the way for extended missions in cislunar space using similar propulsion strategies.

WHAT ARE SOME OF THE KEY ADVANTAGES OF THE NEAR RECTILINEAR HALO ORBIT NRHO FOR LUNAR MISSIONS

The near rectilinear halo orbit, or NRHO, is a special type of halo orbit that was selected by NASA for the Gateway – a small space station that will orbit the Moon and serve as a staging point for Artemis missions. There are several advantages of using an NRHO for the Gateway and future lunar missions compared to other possible orbits.

One major benefit of the NRHO is its stability. Halo orbits around the second Lagrangian point (L2) of the Earth-Moon system are dynamically stable, meaning a spacecraft can remain in this orbit without having to perform complex orbital maintenance maneuvers to counteract perturbations. This allows for long-term dwell of orbital assets like the Gateway. In contrast, low lunar orbits require station-keeping to account for orbital decay over time. The intrinsic stability of the NRHO reduces operational costs and Complexity for missions utilizing the Gateway.

A linked advantage is that the Gateway’s NRHO enables continuous line-of-sight communication with Earth without interruptions from the Moon getting in the way. This “stable remote platform” feature provides mission planners assured and uninterrupted command and control of robonaut or manned sorties from the Gateway to the lunar surface, increasing safety. Low lunar orbits by comparison have intermittent communications blackout periods. Reliable comms through Gateway are crucial for surface missions.

Another key benefit of the Gateway’s NRHO is its free return capability. If engines fail on a spacecraft departing the Gateway for the lunar surface, the craft’s trajectory will return it to the Earth-Moon system without the need for correction. This ensuresBuilt insafe mode return for astronautswithout depleting mission resources. Low lunar orbits lack this fail-safe free return capacity, necessitating precise maneuvers and significant propellant usage for any emergencies.

The phasing properties of the NRHO mean that missions departing from the Gateway can access any part of the lunar surface within a single orbit, offering coverage flexibility for surface sorties, landings or cargo deliveries. This facilitates global access unlike low polar or equatorial orbits which see the same side of the Moon on each pass. The Gateway’s NRHO phasing point allows surface missions to utilize minimal propellant for optimal transit to target locations.

The orbital altitude of the NRHO above the lunar surface, averaging around 70,000 km, also provides an ideal vantage point for long-term scientific observation of the Moon without interference from short-term fluctuations. Platforms in the Gateway will be able to conduct persistent solar astronomy studies as well as high-resolution imaging surveys of the entire lunar farside which remains occluded from Earth-based observation. Long duration monitoring supports rigorous analysis impossible through brief fly-bys alone.

The NRHO actually fosters economical trajectories allowing spacecraft to take advantage of gravity assists from both Earth and Moon, reducing propellant demands. Missions can utilize minimum energy ballistic transfers from low Earth orbit to the Gateway then onward surface excursions. This conserves precious onboard fuel compared to direct transfers and lower orbits. Lower propellant needs cuts spacecraft mass and launch vehicle lift requirements, easing deployment logistics and decreasing costs. Recent studies have shown NRHO transit mass savings can reach 30% compared to lunar surface injection.

The Gateway’s Near Rectilinear Halo Orbit provides unmatched accessibility, communications, crew safety assurances, scientific value, and most importantly – cost effectiveness – through its inherent dynamical characteristics. Its advantages over direct low lunar orbits truly establish it as the optimal orbital choice for establishing a sustainable lunar presence and enabling the long term exploration, development and commercialization of the Moon under the Artemis program and beyond. The decision to position the Gateway in NRHO demonstrates the care and thoroughness that has gone into mission architecture design for enabling sustainable and ambitious human exploration of the lunar surface from this unique vantage point.