Astronomy Report – April 4th

[category  astronomy-report]

Report title: Astronomy Report
Crew #: 333
Position: Crew Astronomer
Report prepared by: Matias Ballivian Ascarrunz
Date:04-04-2026
Sol: 6

MDRS ROBOTIC OBSERVATORY
Robotic Telescope Requested: MDRS-WF & RCOS-16
Objects to be Imaged this Evening: M86, NGC 7000, M104
Images submitted with this report: M51 (Whirlpool Galaxy). The image was processed by stacking exposures taken with the same filter and then combining the layers using RGB + Lum.
Problems Encountered: None

MUSK OBSERVATORY
Solar Features Observed: N/A
Images submitted with this report: N/A
Problems Encountered: N/A

Questions: For image processing, what techniques would you recommend to achieve sharper images with brighter, more balanced colors? I find that the submitted image appears overly blue.

Astronomy Report – April 5th

[category 

astronomy-report]

Report title: Astronomy Report
Crew #: 333
Position: Crew Astronomer
Report prepared by: Matias Ballivian Ascarrunz
Date: 06-04-2026
Sol: 7

MDRS ROBOTIC OBSERVATORY
Robotic Telescope Requested: RCOS-16 & MDRS-WF
Objects to be Imaged this Evening: M64, M82
Images submitted with this report: None
Problems Encountered: None
MUSK OBSERVATORY
Solar Features Observed: N/A
Images submitted with this report: N/A
Problems Encountered: N/A

Astronomy Report – April 5th

[category 

astronomy-report]

Report title: Astronomy Report
Crew #: 333
Position: Crew Astronomer
Report prepared by: Matias Ballivian Ascarrunz
Date: 05-04-2026
Sol: 7

MDRS ROBOTIC OBSERVATORY
Robotic Telescope Requested: RCOS-16 & MDRS-WF
Objects to be Imaged this Evening: M64, M82
Images submitted with this report: None
Problems Encountered: None
MUSK OBSERVATORY
Solar Features Observed: N/A
Images submitted with this report: N/A
Problems Encountered: N/A

Mid-mission Research Report – April 5th

[category science-report]

Mid mission report – Crew 333

Crew 333 – First Days on Mars: Adapting, Exploring, and Connecting

Crew 333 officially landed on the surface of Mars. Upon arrival, we quickly familiarized ourselves with the station and, after a restorative night’s sleep, began working on our respective experiments and preparing for the first EVAs.

The first two sols were particularly intense, filled with a fast-paced sequence of reports, extravehicular activities, experiment setup, station tasks, and the necessary adjustments to the Martian simulation lifestyle. Early on, the crew also had to address a technical issue: a pressurized tunnel damaged by strong winds. The repair required coordination and careful execution, but it was successfully completed, reinforcing both safety and team cohesion. A bit of confusion surrounding reporting procedures during these initial days added to the challenge, but the crew quickly adapted and found its rhythm.

Over the following sols, although the schedule remained demanding, we managed to organize our workload more efficiently. Multiple EVA sites have already been explored, with additional ones planned depending on weather conditions that may restrict access to the field. This improved pace also allowed us to take moments to fully appreciate the experience of living and working on “Mars”: observing the surrounding landscape, and sharing moments of team bonding through cooking, games, and informal discussions.

These first days have laid the foundation for a cohesive, resilient, and motivated crew, ready to make the most of the mission ahead.

Experiments:

This section provides an overview of the current status and recent developments in the various research projects being conducted by the crew. Each experiment continues to evolve in alignment with its objectives.

Matias Ballivian (Crew Astronomer):

As the astronomer for the mission, I am submitting photos every night to take advantage of the less dense Martian atmosphere. So far, I have not yet captured images that meet the standard I aim to achieve, and I am working closely with the Mission Support astronomer to improve my astrophotography skills.

During the first week of the mission, I have also been working on my research concerning radio communication. The goal of my research is to compare passive methods for increasing radio communication range during EVA without increasing transmitter power consumption. The methods being evaluated are a reflective surface and a tuned loop resonator.

I have already gathered some data to better understand how radio communication works in this environment, and I have conducted short-range tests that look promising for the long-range transmission tests I will be carrying out in the coming week.

Zahraa Al-bayati (Health and Safety Officer):

Throughout the first half of the mission, significant attention has been given to the health and well-being of each crew member. Medication intake has been carefully tracked, with dosages and administration times systematically logged for each individual. Hydration levels have also been closely monitored to ensure the crew remains in optimal condition during both EVA and habitat activities. Overall, the crew’s health status has been satisfactory, with no major incidents to report.

As for my experience, it investigates the evolution of verbal fluency over the course of the mission. The first round of data collection has been completed, including a language questionnaire and a recorded audio linguistic task administered to all crew members. This initial dataset establishes the baseline for the study.

Data collection is scheduled to be conducted two additional times: at mid-mission and at the end of the mission, in order to track potential changes in verbal fluency and draw meaningful conclusions about the cognitive effects of an isolated and confined environment on language performance.

Matthias De Groote (GreenHab Officer):

The experiment conducted aims to evaluate the impact of different soil compositions, including Martian regolith simulant and Utah desert soil, on tomato seed germination and early plant development. Understanding how plants respond to extraterrestrial or extreme terrestrial substrates is essential for the development of sustainable agriculture systems in future space missions, particularly in Martian environments. Since substrate composition directly influences water retention, nutrient availability, and root development, assessing plant responses under these conditions is crucial.

Tomato seeds were selected as a model due to their rapid germination and sensitivity to environmental conditions. The experiment investigates how varying proportions of potting soil, Martian soil simulant, and Utah desert soil affect germination rate, germination timing, and early plant growth parameters.

The experimental setup consisted of six different substrate conditions, each duplicated in two pots, resulting in a total of twelve pots. Each pot was filled with a substrate mixture prepared based on mass to ensure consistency, while maintaining a similar volume across all pots (approximately 2 cm below the rim) due to differences in bulk density between substrates.

The six conditions were defined as follows:

  • Condition 1 (control): 100% potting soil

  • Condition 2: 25% potting soil, 75% Martian soil

  • Condition 3: 10% potting soil, 90% Martian soil

  • Condition 4: 25% potting soil, 75% Utah desert soil

  • Condition 5: 100% Martian soil

  • Condition 6: 100% Utah desert soil

For each pot, 25 mL of water was added and thoroughly mixed with the substrate to ensure homogeneous moisture distribution and prevent water accumulation at the surface. Ten tomato seeds were then evenly distributed in each pot.

To control environmental conditions and limit excessive evaporation or localized greenhouse effects, each pot was covered with plastic film and placed inside a white bag. The seeds were sprayed with water and monitored daily.

At this stage of the experiment, I am still awaiting seed germination. I am currently encountering minor difficulties in maintaining sufficient humidity within the pots, likely due to the physical properties of the substrates, particularly those containing high proportions of Martian simulant and desert soil. Adjustments in watering frequency and moisture management are therefore being considered to optimize germination conditions.

Once germination occurs, the plastic cover will be removed. The germination rate and the timing of germination will be recorded for each condition, allowing the assessment of both the success and speed of germination under different substrate constraints. These parameters provide insights into the physiological response of seeds to environmental stress.

After germination, five plants per condition will be selected and maintained for further growth analysis. Watering will be performed periodically, with the volume and frequency adjusted according to ambient temperature conditions, in order to maintain adequate soil moisture while minimizing water usage.

At the end of the experiment, several growth parameters will be measured to evaluate plant development. These will include shoot length (hypocotyl and epicotyl), root system length, number of secondary roots, and fresh biomass. These measurements will allow for a comprehensive assessment of how substrate composition influences both aboveground and belowground plant development.

This experiment provides valuable insights into the ability of plants to grow in Martian-like substrates and extreme terrestrial soils, contributing to our understanding of plant adaptation in constrained environments and informing future strategies for extraterrestrial agriculture.

Joanna Galloway (Crew Journalist):

As part of the human–machine interaction experiments conducted during the MDRS mission, I have been analyzing crew gestures using a Tap Strap device. The objective of this study is to record and characterize a set of eight predefined gestures performed by crew members, in order to generate a dataset that can later be used to train a machine learning module currently being developed by a professor at UCL.

During the initial phase of the mission, I focused on collecting baseline data under controlled conditions. Crew members were asked to reproduce each of the eight gestures multiple times in the Science Dome, ensuring consistency in execution and minimizing external variables. This approach allows for the creation of a reliable reference dataset for gesture recognition.

In the next phase of the experiment, I plan to investigate the impact of extravehicular constraints on gesture performance. To achieve this, crew members will perform the same set of gestures during two separate outdoor sessions while wearing different types of spacesuits. These trials are designed to simulate operational conditions on Mars and to assess how mobility restrictions, glove thickness, and environmental factors affect both gesture execution and sensor detection.

The data collected will subsequently be analyzed to identify variations in gesture accuracy and consistency across conditions. This work aims to contribute to the development of robust gesture-based control systems adapted to space environments, with potential applications in future planetary exploration missions.

Antoine Dubois (Crew Executive Officer / Crew Engineer):

As part of my experiment, I aim to compare terrain perception in a Martian analogue environment between human observation during EVA and drone-based imagery. On Mars, understanding the terrain relies on a dual perspective: that of astronauts on the ground, constrained by their field of view, and that of robotic systems such as drones. This perception can be affected by dust, potentially altering the recognition of landforms, obstacles, and geomorphological structures.

In the field, selected sites are explored both by EVA crew members and through aerial imaging using a drone when conditions allow. Crew members assess the terrain based on predefined criteria such as readability, visibility, and surface characteristics, while the drone captures complementary visual data from above. This approach enables a direct comparison between ground-based and aerial perceptions of the same environment.

At the midpoint of the mission, two sites have already been successfully studied. The initial observations highlight noticeable differences in terrain interpretation depending on the observation method, particularly in areas with uneven surfaces or dust cover. Additional EVA sessions are planned to investigate two or three more sites, depending on weather conditions, which may limit access to the field or drone operations.

By the end of the mission, this experiment is expected to provide valuable insights into how observational biases may influence terrain assessment on Mars, and how combining human and robotic perspectives could improve navigation, safety, and scientific analysis during future exploration missions.

Marie Jansen (Crew Commander):

In their study on conflict management styles before and after a long-duration spaceflight simulation, Kass et al. (2010) draw on the Thomas-Kilmann Conflict Mode Instrument, which identifies five modes of response to disagreement. Their findings show a predominant use of the accommodating mode (over 75%) compared to the collaborating mode (under 25%). These observations highlight a tendency to prioritize harmony over collaborative conflict resolution. This theoretical framework served as the foundation for the present research.

The aim of this study is to examine the extent to which conflict management strategies influence conflict resolution over time. It also seeks to analyze how these strategies evolve, and to compare their use between a standard terrestrial environment and a confined, isolated setting, as well as the impact all of this may have on stress levels. This study will contribute to a better understanding of how individuals adapt to conflict in contexts of isolation and confinement.

Prior to departure, participants completed an initial Dutch questionnaire designed to assess their typical conflict management styles in everyday life. During the simulation, data were collected using two tools. The first is an anonymized online logbook, filled out daily at the end of each day (estimated time: 5 to 10 minutes). Participants briefly described any disagreements experienced during the day, identified the conflict management strategies they used based on the Thomas-Kilmann model through Likert-type scales, and rated both their own conflict management and that of the other parties involved. A follow-up question assessed whether the disagreement was still emotionally or cognitively present at the time of completion. At the end of the questionnaire, participants were asked to rate their stress level during the conflict.

At this stage, I am unable to access the results of my experiment. As one of the participants in my own mission, reviewing my crewmates’ responses would risk biasing the data, so I have chosen to set that aside until we return.

That said, here are my personal observations. I believe that starting the simulation earlier than originally planned likely had a meaningful impact on the results. The most significant conflicts emerged and were resolved right at the beginning, we took the time to openly share our ways of living, our boundaries, and our frustrations, which meant that by Sol 1, we had already reached a solid understanding on many fronts.

I have also noticed that the crew makes a genuine effort to express their reservations, whether through me as a channel, during shared meals, or even through lighthearted but pointed humor. Overall, conflict tends to be managed fairly well, and people do try to adapt to one another. However, I do sense that at times, some crew members hold back and absorb tension rather than actively seeking a collaborative solution.

I very much look forward to discovering the full results once we are back in Belgium.

Astronomy Report – April 6th

[category 

astronomy-report]

Report title: Astronomy Report
Crew #: 333
Position: Crew Astronomer
Report prepared by: Matias Ballivian Ascarrunz
Date: 06-04-2026
Sol: 8

MDRS ROBOTIC OBSERVATORY
Robotic Telescope Requested:RCOS-16
Objects to be Imaged this Evening: M51 Green, Blue and Lum filters
Images submitted with this report: None
Problems Encountered: None
MUSK OBSERVATORY
Solar Features Observed: N/A
Images submitted with this report: N/A
Problems Encountered: N/A

Astronomy Report – April 8th

[category 

astronomy-report]

Report title: Astronomy Report
Crew #: 333
Position: Crew Astronomer
Report prepared by: Matias Ballivian Ascarrunz
Date: 08-04-2026
Sol: 10

MDRS ROBOTIC OBSERVATORY
Robotic Telescope Requested: MDRS-WF & MLC RCOS-16
Objects to be Imaged this Evening: Resubmission of M51& M81 (The previous images were corrupted), and M99
Images submitted with this report: ngc7000 colored using ASIStudio to stack and to combine the RGB+Lum
Problems Encountered:None
MUSK OBSERVATORY
Solar Features Observed: N/A
Images submitted with this report: N/A
Problems Encountered: N/A
Question: Would you recommend doing the coloring in Photoshop? If so, after stacking I have three images; PNG, TIFF, and FITS. Which one should I use for coloring?
Thanks again for all the help!

Astronomy Report – April 9th

[category 

astronomy-report]

Report title: Astronomy Report
Crew #: 333
Position: Crew Astronomer
Report prepared by: Matias Ballivian Ascarrunz
Date: 09-04-2026
Sol: 11

MDRS ROBOTIC OBSERVATORY
Robotic Telescope Requested: MDRS-WF & RCOS-16
Objects to be Imaged this Evening:NGC 2237, M66, M81, M51
Images submitted with this report: NGC7000 colored
Problems Encountered:Mount error in the MDRSWF
MUSK OBSERVATORY
Solar Features Observed: N/A
Images submitted with this report: N/A
Problems Encountered: N/A

Astronomy Report – April 10th

[category 

astronomy-report]

Report title: Astronomy Report
Crew #: 333
Position: Crew Astronomer
Report prepared by: Matias Ballivian Ascarrunz
Date: 10-04-2026
Sol: 12

MDRS ROBOTIC OBSERVATORY
Robotic Telescope Requested: MDRS-WF & RCOS-16
Objects to be Imaged this Evening: NGC 2237 resubmission
Images submitted with this report: None
Problems Encountered: All of the images taken last night with the RCOS-16 are corrupted.
MUSK OBSERVATORY
Solar Features Observed: N/A
Images submitted with this report: N/A
Problems Encountered: N/A

End-Mission Research Report – April 10th

[category science-report]

Crew 333 – The Final Chapter: Farewell, Red Planet

This experience has taught us a great deal. First and foremost, we learned the discipline that comes with rigorous reporting, carefully observing our environment, discussing challenges as a team, resolving issues together, and taking the time each day to truly understand one another’s work.
Beyond that, we learned a tremendous amount about ourselves. Being isolated as a group of six in a confined space with limited resources brings you back to something very fundamental, the core needs of human beings. Each of us had the opportunity to grow, to understand one another more deeply, and to discover our own limits.
We also gained a genuine appreciation for what life in space truly entails. Living in a reduced environment gave us a much closer perspective on the reality astronauts face every day. But above all, what we take away from this experience are the bonds we built with one another. We laughed, we cried, we shared stories and moments of pure joy.
In short, this is an experience that will stay with us forever.

Experiments:
This section outlines the progress of the research projects conducted by the crew during our mission.

Zahraa Al-bayati (Health and Safety Officer):
During this MDRS mission, I conducted a speech and language pathology experiment entitled:
“Verbal Communication and Adaptive Strategies in Extreme Confinement: Contribution of Speech and Language Pathology in a Simulated Martian Mission.”
The objective of this study was to investigate how verbal communication evolves during extreme confinement and isolation conditions similar to a simulated Mars mission. Five crew members participated in the study. Data were collected at multiple time points during the mission using:
phonemic verbal fluency tasks
semantic verbal fluency tasks
open-ended communication questions

These measures allowed the analysis of several communication variables, including: verbal fluency; speech rate; pauses and hesitations; discourse organization; clarity of explanations; adaptive communication strategies.
Overall, the results suggest that communication patterns evolved over the course of the mission. Changes were observed in verbal fluency, speech organization, and the use of adaptive strategies. Several crew members demonstrated increased efficiency in communication, including more concise explanations and improved task-oriented discourse. In some cases, mild reductions in lexical fluency were observed, possibly related to cognitive load, fatigue, or confinement effects. Additionally, participants appeared to develop adaptive communication behaviors, such as simplifying explanations, using more direct language, and improving shared understanding during mission-related interactions.
This experiment highlights the relevance of speech and language pathology in extreme environments. Monitoring communication changes during confinement may help optimize crew performance, reduce misunderstandings, and support psychological and operational functioning in future analog and space missions.

Matthias De Groote (GreenHab Officer):
The experiment conducted aimed to evaluate the impact of different soil compositions, including Martian regolith simulant and Utah desert soil, on tomato seed germination. Understanding how plants respond to extraterrestrial or extreme terrestrial substrates is essential for the development of sustainable agriculture systems in future space missions, particularly in Martian environments. Since substrate composition directly influences water retention and nutrient availability, assessing plant responses under these conditions is crucial.
Tomato seeds were selected as a model due to their rapid germination and sensitivity to environmental conditions. The experiment investigated how varying proportions of potting soil, Martian soil simulant, and Utah desert soil affected germination rate and timing.
The experimental setup consisted of six different substrate conditions, each duplicated in two pots, resulting in a total of twelve pots. Each pot was filled with a substrate mixture prepared based on mass to ensure consistency, while maintaining a similar volume across all pots (approximately 2 cm below the rim) due to differences in bulk density between substrates.
The six conditions were defined as follows:
Condition 1 (control): 100% potting soil
Condition 2: 25% potting soil, 75% Martian soil
Condition 3: 10% potting soil, 90% Martian soil
Condition 4: 25% potting soil, 75% Utah desert soil
Condition 5: 100% Martian soil
Condition 6: 100% Utah desert soil

For each pot, 25 mL of water was added and thoroughly mixed with the substrate to ensure homogeneous moisture distribution and prevent water accumulation at the surface. Ten tomato seeds were then evenly distributed in each pot.
To control environmental conditions and limit excessive evaporation, each pot was covered with plastic film and placed inside a white bag. The seeds were sprayed with water regularly and monitored daily until germination occurred. Water was supplied by daily spraying throughout the experiment, and an additional watering of 100 mL per pot was performed on day 6 in response to the difficulties encountered in maintaining sufficient humidity within the substrates.
Germination began to be observed from day 8. The development of the seedlings was then monitored daily until day 12, at which point the germination rate was determined for each pot. While differences in germination rates appeared between the Martian soil, the Utah desert soil, and the potting soil, it remains difficult at this stage to establish clear trends.
Further statistical analyses will be required to assess the significance of these differences and to better understand the impact of substrate composition on seed germination.
Due to the relatively late onset of germination, the experiment could not be extended to the plant growth phase. As a result, no measurements of shoot or root development were performed.
This experiment nevertheless provides preliminary insights into the ability of tomato seeds to germinate in Martian-like and extreme terrestrial substrates, contributing to our understanding of plant establishment under constrained environmental conditions and informing future research on extraterrestrial agriculture.

Joanna Galloway (Crew Journalist):
This experiment investigated the precision of astronauts’ hand gestures in simulated space conditions. Prior to the simulation phase, each participant was asked to sit and replicate eight predefined gestures presented in a video. Their hand movements were recorded using a Tap Strap device, which captures motion and spatial positioning data. This baseline measurement established a reference for comparison with subsequent trials conducted under varying environmental constraints.
During the simulation, participants repeated the same set of gestures under three distinct conditions. The first trial took place inside the science dome on Sol 3. The second was conducted outdoors on Sol 8 using light equipment, and the third on Sol 9 with heavier equipment. These conditions were designed to evaluate the effects of fatigue and glove bulk on gesture precision, with particular attention to how increased physical strain and reduced dexterity might alter movement accuracy.
With the simulation phase now complete, all participants will be asked to perform the gesture sequence once more after returning to baseline conditions. The full dataset, including pre-simulation, in-simulation, and post-simulation measurements, will then be analyzed to assess changes in movement precision and to better understand the impact of environmental and equipment-related factors on fine motor performance.

Matias Ballivian (Crew Astronomer):
As the mission concludes, I reflect on the progress made in both astronomical observations and radio communication research.
On the astronomy side, I continued nightly imaging sessions, taking advantage of the reduced atmospheric density and favorable observing conditions. Over the course of the mission, I successfully captured several high-quality images that represent a clear improvement from the beginning of the rotation. These results demonstrate a better understanding of imaging techniques, including exposure control, tracking, and target selection.
However, I recognize that image acquisition is only part of the process. I am particularly motivated to further develop my post-processing skills, as this remains a key area for improvement. Enhancing my ability to process and refine raw data will be essential to reaching the level of quality I aim for in future missions.
Regarding telecommunications research, I focused on evaluating passive methods to enhance radio communication range during EVA without increasing transmitter power consumption. The two methods investigated were the use of a reflective surface and a tuned loop resonator.
Throughout the mission, I conducted a series of short-range tests to better understand signal behavior in this environment, followed by initial longer-range evaluations. While the experimental setups functioned as intended, the results indicate that both methods primarily improve signal clarity when the transmission is already above the intelligibility threshold. In other words, they enhance signal quality rather than extending the effective communication range. No significant increase in maximum transmission distance was observed.
Further analysis of the collected data is still required to quantify these effects more precisely. Nonetheless, the findings provide useful insight into the limitations and potential applications of passive signal enhancement techniques in EVA scenarios.

Antoine Dubois (Executive Officer / Crew Engineer):
At the end of the mission, my experiment on terrain perception in a Martian analogue environment has been successfully completed. Data collection was carried out across five distinct sites: Compass Rock, Sea of Shells, Green Mars View, Kissing Camel Ridge, and Candor Chasma. Each location was analyzed both through human observation during EVA and via drone-based imagery, allowing for a comprehensive comparison of perspectives.
All planned datasets have been acquired. I now have both the drone imagery and the qualitative assessments from EVA crew members for each site. The next step will consist of a detailed analysis of these data to better understand the differences in perception, particularly in terms of terrain readability, obstacle identification, and geomorphological interpretation.
Preliminary observations already highlight the clear value of combining both approaches. The drone provides a broader spatial understanding and reveals large-scale structures that are sometimes difficult to perceive from the ground, while EVA observations offer finer, more detailed insights into surface features and textures.
This dual approach appears to be highly complementary and reinforces the importance of integrating both human and robotic perspectives for future planetary exploration. Further analysis will aim to quantify these differences and assess how they can contribute to improving navigation, safety, and scientific efficiency in Martian environments.

Marie Jansen (Crew Commander):
In line with the theoretical framework established by Kass et al. (2010) and the Thomas-Kilmann Conflict Mode Instrument, this study aimed to explore how conflict management strategies evolve over the course of a long-duration simulation in isolation and confinement.
At this stage, I am still unable to access or analyze the collected data, as doing so during the mission could introduce bias, given my dual role as both researcher and participant. A full analysis will therefore only be conducted after the completion of the simulation.
Nevertheless, some personal observations can be noted regarding the final phase of the mission. Around Sol 8–9, an increase in interpersonal tensions was perceptible within the crew. However, these tensions did not escalate into persistent conflict, as open discussion and communication appeared to play a key role in easing the situation. This suggests that, despite moments of strain, the crew retained the ability to regulate conflict through dialogue.
Overall, while a comprehensive interpretation of the results remains pending, these observations hint at a dynamic process in which tensions may intensify over time but can still be mitigated through collective communication strategies. A deeper analysis will be necessary to confirm these preliminary impressions once access to the full dataset is possible.

Astronomy Report – April 23rd

[category  astronomy-report]

Report title: Astronomy Report

Crew #: 335

Position: Engineer

Report prepared by: Katherine Berry

Date: 23Apr2026

Sol: 4

MDRS ROBOTIC OBSERVATORY

Robotic Telescope Requested: MDRS-WF

Objects to be Imaged this Evening: messier 16

Images submitted with this report: In process, will update when photos are processed.

Problems Encountered: None.

MUSK OBSERVATORY

Solar Features Observed: N/A

Images submitted with this report: N/A

Problems Encountered: N/A

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