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MoonBEAM: A New Era in Gamma-Ray Observation

MoonBEAM satellite aims to improve detection of cosmic gamma-ray bursts.

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The Moon Burst Energetics All-sky Monitor, also known as MoonBEAM, is a small satellite that will orbit the space between the Earth and the Moon. This mission aims to study powerful cosmic events called relativistic jets. These jets can occur in various situations, such as when two stars collide or when a massive star collapses. MoonBEAM will monitor the sky for Gamma-ray Bursts, which are intense flashes of gamma rays that happen as a result of these cosmic events.

Why MoonBEAM is Important

Current gamma-ray observatories are limited because they are situated in low Earth orbit. This position prevents them from observing certain parts of the sky due to the Earth blocking their view. Additionally, these observatories often have to turn off their Detectors when they pass through an area called the South Atlantic Anomaly, where there is a lot of high-energy particle activity. As a result, they miss many important cosmic events.

MoonBEAM will overcome these challenges by being located in Cislunar Space, which means it will not be blocked by the Earth. This position will allow it to see the entire sky at once and will greatly improve the chances of discovering new gamma-ray events. With its unique orbit, MoonBEAM can also work alongside other gamma-ray instruments in low Earth orbit to better pinpoint where these cosmic events are happening.

Scientific Goals of MoonBEAM

The main goals of the MoonBEAM mission include:

  1. Identifying the sources of gamma-ray bursts: MoonBEAM will help determine what causes these powerful bursts of energy in the universe.

  2. Studying the conditions for jet formation: The mission will investigate what conditions need to be present for a relativistic jet to launch.

  3. Understanding high-energy emissions: MoonBEAM will look into where the high-energy emissions from these jets come from.

By achieving these goals, MoonBEAM will contribute significantly to our knowledge of cosmic events and their mechanisms.

How MoonBEAM Works

MoonBEAM will be equipped with six special detectors placed on the spacecraft. These detectors will be designed to look for gamma rays across a broad range of energy levels, from very low to extremely high. The design features two different types of materials to improve sensitivity and effectiveness. This setup allows MoonBEAM to pick up on different signals and helps improve its ability to determine the source of an event.

The unique design of these detectors will also allow them to work together. By comparing signals from different detectors, MoonBEAM will be able to tell where a gamma-ray burst is happening much more accurately. This is critical because knowing the location of these bursts will help astronomers follow up and study them further with other telescopes and instruments.

Observing Cosmic Events

MoonBEAM's main focus will be on detecting gamma-ray bursts arising from different cosmic events. These include:

  • Mergers of compact objects: When two neutron stars or black holes collide, they can create powerful jets.

  • Core collapse supernovae: Massive stars can explode and create jets during their collapse phase.

  • Magnetar giant flares: These are enormous bursts of energy from neutron stars with strong magnetic fields.

By observing these events, MoonBEAM will gather data that can help scientists piece together a clearer picture of how energy and matter behave in extreme situations.

The Need for Gamma-ray Instruments

With the current gamma-ray observatories aging and no new replacements planned, there is a pressing need for more instruments like MoonBEAM. Smaller satellite designs, such as CubeSats and SmallSats, are being proposed as feasible solutions to address this need.

MoonBEAM will provide continuous observations of gamma-ray transients, which are crucial for understanding the universe. The ability to monitor the sky constantly will help capture these fleeting events that other instruments may miss.

Advantages of MoonBEAM

MoonBEAM has several advantages that will enhance its scientific output:

  1. Wide field of view: Its cislunar orbit means there will be no Earth interference, allowing MoonBEAM to observe the entire sky all at once.

  2. High duty cycle: With over 98% uptime, the satellite will be operating most of the time, increasing the chances of capturing gamma-ray bursts.

  3. Stable background readings: Being farther away from Earth means MoonBEAM will experience a more stable background, allowing it to detect faint signals more effectively.

  4. Improved Localization: The ability to pinpoint where bursts happen will greatly enhance follow-up observations by other telescopes, making it easier to study the associated phenomena.

Collaboration in Astronomy

MoonBEAM will work alongside the Interplanetary Gamma-Ray Burst Timing Network, a collaborative effort that combines data from several gamma-ray instruments located both in and outside of low Earth orbit. This teamwork will enable more accurate localization of gamma-ray bursts and allow scientists to share information quickly across the astronomical community.

Preparing for the Mission

Before the satellite is launched, extensive simulations will be conducted to ensure its detectors are working as intended. This includes testing their sensitivity, localization capabilities, and response to different energy levels. These preparations are essential to ensure the mission's success and to maximize the scientific return once MoonBEAM is operational.

The Impact of MoonBEAM on Astronomy

The findings from the MoonBEAM mission will significantly contribute to our understanding of the universe. By identifying the sources of gamma-ray bursts and the conditions needed for jet formation, scientists will be able to make informed conclusions about the life cycles of stars and the complex processes that govern our universe.

Additionally, the data collected will pave the way for further research and collaboration among astronomers. MoonBEAM's results will not only enhance our knowledge of cosmic events but also play a vital role in the broader field of multimessenger astronomy, which focuses on combining signals from various sources, such as electromagnetic radiation and gravitational waves.

Conclusion

The Moon Burst Energetics All-sky Monitor is set to play a crucial role in the future of astronomy by monitoring gamma-ray bursts and studying the conditions that give rise to these extraordinary cosmic phenomena. With its innovative design, high operational capabilities, and collaboration with other missions, MoonBEAM will advance our understanding of the universe and the events that occur within it. As we explore the unknown, MoonBEAM will provide valuable insights that could reshape our perspective on astrophysics and the fundamental processes that drive the cosmos.

Original Source

Title: The Scientific Performance of the MoonBurst Energetics All-sky Monitor(MoonBEAM)

Abstract: MoonBEAM is a SmallSat concept placed in cislunar orbit developed to study the progenitors and multimessenger/multiwavelength signals of transient relativistic jets and outflows and determine the conditions that lead to the launching of a transient relativistic jet. The advantage of MoonBEAM is the instantaneous all-sky coverage due to its orbit, which maximizes the gamma-raytransient observations and provides upperlimits for non-detections. Earth blockage and detector downtime from the high particle activity in the South Atlantic Anomaly region prevent gamma-ray observatories in low Earth orbit from surveying the entire sky at a given time. In addition, the long baseline provided from a cislunar orbit allows MoonBEAM to constrain the localization annulus when combined with a gamma-ray instrument in low Earth orbit utilizing the timing triangulation technique. We present the scientific performance of MoonBEAM including the expected effective area, localization ability and duty cycle. MoonBEAM provides many advantages to the gamma-ray and gravitational-wave follow up community by reducing the search region needed to identify the afterglow and kilanova emission. In addition, the all-sky coverage will provide insight into the conditions that lead to a successful relativistic jet, instead of a shock breakout event, or a completely failed jet in the case of core collapse supernovae.

Authors: C. Fletcher, C. M. Hui, A. Goldstein, The MoonBEAM Team

Last Update: 2023-08-30 00:00:00

Language: English

Source URL: https://arxiv.org/abs/2308.16293

Source PDF: https://arxiv.org/pdf/2308.16293

Licence: https://creativecommons.org/licenses/by-nc-sa/4.0/

Changes: This summary was created with assistance from AI and may have inaccuracies. For accurate information, please refer to the original source documents linked here.

Thank you to arxiv for use of its open access interoperability.

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