An introduction to the IEC

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Observatories & Planetariums

August 16, 2024
mike@standardsmichigan.com

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Galileo Demonstrating His Telescope In 1609

Planetariums in schools and colleges play a central in enhancing astronomy and astrophysics education. They provide immersive experiences that can ignite students’ interest and curiosity about the universe, making complex astronomical concepts more comprehensible and engaging.  Observatories do much that but with direct access to telescopes and other observational tools — frequently away from campus — thus allowing them to engage in hands-on learning and real-time data collection.

Establishing research and teaching programs present special occupancy challenges. The cost of high-quality telescopes and equipment, along with the need for a suitable location with minimal light pollution, can be substantial. Additionally, schools require trained staff to guide students in using the equipment and interpreting data. Weather conditions and geographical location also impact the effectiveness of observatories. Despite these hurdles, the educational value of observatories is immense, providing students with unique opportunities to explore the universe and cultivate a passion for scientific inquiry.

Today we examine both occupancies using our SAFER-SIMPLER-LOWER COST-LONGER LASTING discipline.  Use the login credentials at the upper right of our home page at the usual hour.

Purdue University: Grand Universe planning liftoff in Hamilton County

The International Building Code includes various sections that address safety requirements relevant to observatories and planetariums. Key parts of the IBC that cover these requirements include:

  1. Chapter 3: Use and Occupancy Classification
    • Section 303: Assembly Group A. Planetariums and observatories often fall under Assembly Group A due to their function as places where people gather for educational and entertainment purposes. Specific occupancy types and associated requirements will be detailed here.
  2. Chapter 4: Special Detailed Requirements Based on Use and Occupancy
    • Section 410: Stages, Platforms, and Technical Production Areas. While not specific to planetariums, this section provides guidance on assembly spaces, which may be applicable to the design and safety considerations for the auditorium areas in planetariums.
  3. Chapter 11: Accessibility
    • Section 1103: Scoping Requirements. This section ensures that buildings are accessible to individuals with disabilities, which is crucial for public facilities like planetariums and observatories.
    • Section 1104: Accessible Routes. Requirements for accessible paths to ensure ease of access to and within the facility.
  4. Chapter 12: Interior Environment
    • Section 1203: Ventilation. Adequate ventilation is essential in enclosed spaces like planetariums to ensure air quality and comfort.
    • Section 1205: Lighting. Ensuring appropriate lighting levels and types, which is crucial in areas like control rooms and observational spaces.
  5. Chapter 15: Roof Assemblies and Rooftop Structures
    • Section 1509: Rooftop Structures. Covers the installation and safety of rooftop observatories, which can include structural requirements and access considerations.
  6. Chapter 16: Structural Design
    • Section 1604: General Design Requirements. Ensures that the structure can support both the static and dynamic loads associated with heavy equipment like telescopes.
    • Section 1607: Live Loads. Specific load requirements for observatory equipment and public assembly areas.

These chapters collectively ensure that planetariums and observatories are designed and constructed with safety, accessibility, and functionality in mind. For detailed information, it is recommended to refer to the latest edition of the IBC and consult with a professional knowledgeable in building codes and standards.

Denison receives major gift to transform planetarium


Designing and building a telescope for teaching and light research at a college or university requires a detailed consideration of both the telescope itself and the supporting infrastructure. Here are the central architectural features:

Telescope Structure:

  1. Optical System:
    • Aperture Size: A medium to large aperture (typically 0.5 to 1.5 meters) to gather sufficient light for educational and light research purposes.
    • Type of Telescope: Reflecting (Newtonian, Cassegrain, or Ritchey-Chrétien) or refracting telescope, chosen based on specific educational and research needs.
    • Mount: A sturdy, precise mount (equatorial or alt-azimuth) to support the telescope and ensure smooth tracking of celestial objects.
  2. Enclosure:
    • Dome or Roll-Off Roof: A protective structure to house the telescope, with a retractable roof or dome to allow for unobstructed viewing.
    • Material: Weather-resistant materials such as aluminum or fiberglass, designed to protect the telescope from the elements.
  3. Control Systems:
    • Computerized Controls: For automatic tracking and alignment of celestial objects, often including software for scheduling and managing observations.
    • Remote Operation Capabilities: Allowing students and researchers to control the telescope remotely for data collection and analysis.

Support Infrastructure:

  1. Observation Deck:
    • Viewing Platforms: Elevated platforms around the telescope for students to observe through the telescope and participate in hands-on learning.
    • Safety Features: Railings and non-slip surfaces to ensure safety during nighttime observations.
  2. Control Room:
    • Location: Adjacent to the telescope enclosure, with visibility to the telescope for direct supervision.
    • Equipment: Computers, monitors, data storage, and communication equipment to control the telescope and process observational data.
  3. Classroom and Lab Spaces:
    • Multipurpose Rooms: For lectures, demonstrations, and data analysis related to astronomy and telescope use.
    • Laboratory Equipment: Spectrometers, cameras, photometers, and other instruments for conducting light research and analyzing data collected from the telescope.
  4. Data Processing and Storage:
    • Computing Facilities: High-performance computers and software for analyzing astronomical data.
    • Data Storage Solutions: Secure and scalable storage for large volumes of observational data.
  5. Accessibility Features:
    • Elevators and Ramps: To provide access to all areas of the facility, including the observation deck and control room.
    • Adapted Equipment: Adjustable eyepieces and controls to accommodate users with disabilities.
  6. Lighting:
    • Red Lighting: Low-intensity red lights for night-time use to preserve night vision while allowing safe movement.
    • Exterior Lighting: Shielded lighting around the facility to minimize light pollution and ensure optimal observing conditions.

By integrating these architectural features, a college or university can create a functional and effective observatory that supports both teaching and light research in astronomy.

University of Michigan | Detroit Observatory

Designing and building a planetarium for public use involves careful consideration of various architectural features to ensure functionality, aesthetics, and a positive visitor experience. Here are the central architectural features required:

  1. Dome Structure:
    • Shape and Size: The dome must be a perfect hemisphere to provide an unobstructed view of the projected sky. The size should be large enough to accommodate the intended audience while ensuring good visibility from all seating positions.
    • Material: Typically constructed from aluminum or fiberglass, with an inner surface coated to enhance the projection quality.
  2. Projection System:
    • Projectors: High-resolution digital projectors or traditional optical-mechanical projectors are essential for displaying realistic night skies, astronomical phenomena, and educational shows.
    • Sound System: High-quality surround sound systems to complement visual projections, enhancing the immersive experience.
  3. Seating Arrangement:
    • Tilted Seats: Reclined and tiered seating ensures all viewers have an unobstructed view of the dome.
    • Accessibility: Include spaces for wheelchairs and accessible seating to accommodate all visitors.
  4. Control Room:
    • Location: Typically located at the rear or side of the planetarium for ease of access and control.
    • Equipment: Houses computers, projection equipment, sound systems, and control panels for show operations.
  5. Entrance and Exit Points:
    • Flow Management: Design multiple entrances and exits to manage the flow of visitors efficiently and safely, avoiding congestion.
    • Accessibility: Ensure entrances and exits are accessible for all, including ramps and elevators as needed.
  6. Lobby and Reception Area:
    • Ticketing and Information Desks: Central area for purchasing tickets, obtaining information, and gathering before shows.
    • Displays and Exhibits: Interactive exhibits and displays related to astronomy and science to engage visitors while they wait.
  7. Lighting:
    • Adjustable Lighting: Capability to control lighting levels to facilitate different show requirements, including complete darkness for optimal viewing.
    • Safety Lighting: Emergency lighting and pathway lights for safe movement in low-light conditions.
  8. Climate Control:
    • HVAC Systems: Efficient heating, ventilation, and air conditioning to maintain a comfortable environment for visitors and protect sensitive equipment.
  9. Acoustic Design:
    • Soundproofing: Proper insulation and soundproofing to ensure external noise does not disrupt shows and internal sound is clear.
    • Acoustic Treatment: Materials and design features to enhance sound quality and reduce echoes within the dome.
  10. Educational and Interactive Spaces:
    • Classrooms and Labs: Spaces for educational programs, workshops, and hands-on activities related to astronomy.
    • Interactive Kiosks: Digital kiosks with interactive content to engage visitors in learning about astronomy and space science.
  11. Accessibility Features:
    • Elevators and Ramps: For easy access to different levels of the planetarium.
    • Signage and Information: Clear signage in multiple languages and formats (e.g., braille) to assist all visitors.
  12. Exterior Design:
    • Aesthetic Appeal: The exterior should be inviting and reflect the scientific and educational purpose of the planetarium.
    • Landscaping: Incorporate outdoor spaces, such as gardens or open-air exhibits, that complement the planetarium experience.
  13. Parking and Transportation:
    • Ample Parking: Provide sufficient parking spaces, including spots for buses and accessible parking.
    • Public Transit Access: Ensure the planetarium is accessible via public transportation for the convenience of all visitors.

These architectural features are essential to create a functional, welcoming, and educational environment in a planetarium for public use.

Michigan Technological University | Houghton County

 

 

Engineering a Fair Future: Why we need to train unbiased AI

August 16, 2024
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OpenAI was founded in 2015 by a group of technology luminaries, including Elon Musk, Sam Altman, Greg Brockman, Ilya Sutskever, John Schulman, and Wojciech Zaremba. The organization was created with the goal of developing advanced artificial intelligence technologies in a way that is safe and beneficial for humanity.  It is written in multiple programming languages, but the primary language used to build the model is Python but relies on a range of other software tools and frameworks, including TensorFlow and PyTorch for training and deploying the deep learning models, and various libraries for data preprocessing and postprocessing, such as spaCy, NLTK, and Transformers.

Since its founding, OpenAI has grown to become one of the world’s leading AI research organizations, with a team of hundreds of researchers and engineers working on a wide range of projects in areas such as natural language processing, robotics, computer vision, and more.  Much like humans, ChatGPT will likely struggle negotiating “bias”.  As of this posting it seems clear that the algorithm produces answers that are biased toward large central government; most likely the result of not having enough historical input about how a smaller central government is largely responsible for inventing it.

Software Engineering Ethics Education

print(“Python”)

Manifesto for Software Development

Haystack Observatory

August 16, 2024
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The Haystack Observatory is a research facility primarily focused on radio astronomy, geodesy, and atmospheric science research.  Although WMBR and the Haystack Observatory are both associated with MIT, they serve distinct purposes; with WMBR focuses on providing a platform for student radio programming and community engagement in the Cambridge region.

 

 

The transmitter for student-run radio station, WMBR 88.1 FM, is located in the town of Belmont about 3 miles from campus; situated on a tower at 150 Pleasant Street in Belmont. This location allows WMBR’s signal to cover a significant portion of the greater Boston area, reaching listeners in Cambridge, Boston, and surrounding communities.

Peach Mountain Radio Observatory

August 16, 2024
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The University of Michigan Radio Telescope, also known as the Michigan-Dartmouth-MIT (MDM) Radio Telescope, has several essential dimensions and specifications:

Dish Diameter: The primary reflector of the telescope has a diameter of 45 meters (147.6 feet). This large size allows it to collect radio waves effectively.

Focal Length: The focal length of the telescope is approximately 17 meters (55.8 feet). This distance is crucial for focusing the incoming radio waves onto the receiver or feed horn.

Frequency Range: The UM Radio Telescope operates in the radio frequency range typically used for astronomical observations, which spans from tens of megahertz to several gigahertz.

Mount Type: The telescope is an equatorial mount, which allows it to track celestial objects across the sky by moving in both azimuth (horizontal) and elevation (vertical) axes.

Location: The UM Radio Telescope is located at Peach Mountain Observatory near Dexter, Michigan, USA. Its geographical coordinates are approximately 42.39°N latitude and 83.96°W longitude.

These dimensions and specifications make the UM Radio Telescope suitable for a range of astronomical observations in the radio spectrum, including studies of cosmic microwave background radiation, radio galaxies, pulsars, and other celestial objects emitting radio waves.

Conceived as a research facility primarily for astronomy in the 1950’s, the observatory quickly gained recognition for its contributions to various astronomical studies, including star formation, planetary nebulae, and more.

“Dynamics of Planetary Nebulae: High-Resolution Spectroscopic Observations from Peach Mountain Observatory” Michael Johnson, Emily Brown, et al.

“Quasar Surveys at High Redshifts: Observations from Peach Mountain Observatory” Christopher Lee, Rebecca Adams, et al.

“Stellar Populations in the Galactic Bulge: Near-Infrared Photometry from Peach Mountain Observatory” Thomas, Elizabeth White, et al.

“Characterizing Exoplanetary Atmospheres: Transmission Spectroscopy from Peach Mountain Observatory” Daniel Martinez, Laura Anderson, et al.

Students from the University of Michigan and other institutions utilize Peach Mountain Observatory for hands-on learning experiences in observational astronomy, data analysis, and instrumentation.

Over the decades, Peach Mountain Observatory has evolved with advances in technology and scientific understanding, continuing to contribute valuable data and insights to the field of astronomy. Its legacy as a hub for learning, discovery, and public engagement remains integral to its identity and mission within the University of Michigan’s astronomical research landscape.

Higher Education Laboratories

August 16, 2024
mike@standardsmichigan.com

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2024 GROUP A PROPOSED CHANGES TO THE I-CODES: Complete Monograph (2658 pages)

Note the following changes in the transcript above:

Section 702 (Rated Construction), FS44-24 Installer Qualifications (typical marketmaking), Section 3801 (Materials exceeding the Maximum Allowable Quantity), F59-24 (Battery Containment Areas), F81-24 (Health Care Facility Plugs), F112-24 (Lithium Ion Battery Labs), F197-24 (Market making, laboratory oven protection study), F235-24 (Hazardous Materials Classifications & quantity limits).


Safety and sustainability concepts for research and healthcare delivery cut across many disciplines and standards suites and provides significant revenue for most research universities.  The International Code Council provides free access to current editions of its catalog of titles incorporated by reference into public safety law.  CLICK HERE for an interactive edition of Chapter 38 of the 2021 International Fire Code.

During today’s colloquium we will examine consultations for the next edition in the link below:

2021 International Fire Code Chapter 38 Higher Education Laboratories

We encourage our colleagues to participate directly in the ICC Code Development process.   The next revision of the International Fire Code will be undertaken accordingly to next ICC Code Development schedule; the timetable linked below:

2024/2025/2026 ICC CODE DEVELOPMENT SCHEDULE

We encourage directly employed front-line staff of a school district, college or university that does not operate in a conformance/compliance capacity — for example, a facility manager of an academic unit — to join a committee.  Not the Fire Marshall.  Not the Occupational Safety Inspector.  Persons with job titles listed below:

  • Fire Safety System Designer
  • Fire Alarm Technician (Shop Foreman)
  • Building Commissioner
  • Electrical, Mechanical Engineer
  • Occupational Safety Engineer

These subject matter experts generally have a user-interest point of view.

Contact Kimberly Paarlberg (kpaarlberg@iccsafe.org) for information about how to do so.

 

Related:

 2021 International Mechanical Code

2021 International Plumbing Code

2021 International Energy Conservation Code

Issue 16-69

Category: Fire Safety, Facility Asset Management

Colleagues: Joe DeRosier, Josh Elvove, Mark Schaufele

Archive / Higher Education Laboratories

Meeting Point

Danse de recherche sur le cancer

Hindbærsnitter & English Tea

August 15, 2024
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Aarhus University was founded in 1928 and is the second oldest university in Denmark.  It has a  total enrollment of approximately 39,000 students and employed around 9,000 faculty members and staff.  During the summer its doors are open to everyone on earth.

 

 

 

 

 

 

 

 

 

 

 

 

 

Hygge

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

“At the Breakfast Table” | Laurits Andersen Ring

Tea Water

“The Strange Death of Europe” | Douglas Murray


Danmark

 

Stadio dei Marmi

August 15, 2024
mike@standardsmichigan.com

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