AI Analysis
The package shows some obfuscation techniques but lacks clear indicators of malicious intent. It's safe to assume it is not a supply-chain attack.
- Obfuscation risk due to use of eval and encoded strings.
- No network or shell execution risks detected.
Per-check LLM notes
- Network: No network calls detected, which is normal unless the package requires external services.
- Shell: No shell execution patterns detected, indicating no immediate signs of malicious activity.
- Obfuscation: The use of eval and encoded strings may indicate an attempt to hide code logic, but it could also be used for legitimate purposes like handling encrypted data.
- Credentials: No clear patterns indicative of credential harvesting were found.
- Metadata: The package has some non-HTTPS links and an author with limited information, but no clear signs of malicious intent.
Package Quality Overall: Medium (6.2/10)
Test suite present — 3 test file(s) found
Test runner config found: pyproject.toml3 test file(s) detected (e.g. test_annulus.py)
Well-documented package
Documentation URL: "Documentation" -> https://eddy.readthedocs.io1 documentation file(s) (e.g. conf.py)Detailed PyPI description (3546 chars)
No contributing guide or governance files found
Development Status classifier >= Beta
No type annotations detected
No type annotations, py.typed marker, or stub files detected
Active multi-contributor project
4 unique contributor(s) across 100 commits in PlanetFormationLab/eddySmall but multi-author team (3–4 contributors)
Heuristic Checks
No suspicious network call patterns found
Found 1 obfuscation pattern(s)
.extent ax.imshow(eval(fill), **kw) # Draw the contours. The azimuthal ang
No shell execution patterns detected
No credential harvesting patterns detected
No typosquatting candidates detected
Email domain looks legitimate: mit.edu>
Found 4 suspicious link(s) on the package page
Non-HTTPS external link: http://joss.theoj.org/papers/2868c5ad4b6405eba1aaf1cd8ea53274Non-HTTPS external link: http://joss.theoj.org/papers/2868c5ad4b6405eba1aaf1cd8ea53274/status.svgNon-HTTPS external link: http://ascl.net/1901.010Non-HTTPS external link: http://joss.theoj.org/papers/10.21105/joss.01220
Repository PlanetFormationLab/eddy appears legitimate
2 maintainer concern(s) found
Author name is missing or very shortAuthor "" appears to have only 1 package on PyPI (new or inactive account)
No known vulnerabilities found in OSV database.
AI App Starter Prompt
Create a mini-application called 'DiskDynamicsExplorer' using the Python package 'astro-eddy'. This application will allow users to simulate and visualize the dynamics of protoplanetary disks under various conditions. Here are the key steps and features to implement: 1. **Setup Environment**: Begin by setting up a virtual environment for your Python project. Install necessary packages including 'astro-eddy', 'matplotlib' for plotting, and 'numpy' for numerical operations. 2. **User Interface**: Design a simple command-line interface (CLI) that allows users to input parameters such as disk size, mass distribution, and external forces like stellar radiation pressure or gravitational perturbations from nearby stars. 3. **Simulation Engine**: Use 'astro-eddy' to create a simulation engine that takes user inputs and simulates the evolution of the protoplanetary disk over time. Ensure the simulation accounts for the physical laws governing these systems, such as conservation of angular momentum and hydrodynamics. 4. **Visualization Module**: Implement a visualization module that uses 'matplotlib' to plot the results of the simulations. Users should be able to see how the disk structure changes over time, including any gaps or spiral arms that might form due to gravitational instabilities. 5. **Save & Load Functionality**: Include functionality to save the simulation parameters and results to a file, and to load previously saved simulations for further analysis or modification. 6. **Documentation**: Write comprehensive documentation for your application, explaining each feature and how to use it effectively. Provide examples of different scenarios that users can explore, such as the effect of varying the disk's mass or the influence of a passing star. The 'astro-eddy' package is utilized primarily in Step 3 for running the simulations. It provides tools and models that accurately represent the physics involved in protoplanetary disk dynamics, which are essential for generating realistic simulations. Your goal is to make 'DiskDynamicsExplorer' an educational tool for students and researchers interested in planetary science.
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