Why is this Space Telescope so Tiny?

Huygens Optics
15 Oct 202119:41
EducationalLearning
32 Likes 10 Comments

TLDRThe video script introduces Rik ter Horst, an optical engineer at NOVA-Astron, who handcrafts tiny monolithic Schmidt-Cassegrain telescopes from a single piece of glass. These innovative telescopes, known for their compact size and high image quality, are being developed for a student space project at the University of Portland. The process involves meticulous hand-polishing of spherical and aspherical surfaces, showcasing the art of crafting precision optical components in a small home workshop. The script also humorously hints at a 'Very Large Tiny Telescope' project, aiming to connect multiple units for enhanced astronomical observations.

Takeaways
  • 🌌 The script introduces a unique Schmidt-Cassegrain telescope made from a single piece of glass, highlighting its compact size and monolithic design.
  • πŸ‘€ Rik ter Horst, an optical engineer at NOVA-Astron, is the creator of these monolithic telescopes, showcasing his mastery in crafting optical components by hand.
  • πŸ›  The process of making these telescopes is done manually in a small area of Rik's house, using basic tools and traditional polishing techniques.
  • πŸ” The importance of focal length in telescopes is explained, relating it to the size of the projected image and the ability to discern finer details.
  • πŸ¦… A comparison is made between human and eagle eyes, emphasizing the higher photoreceptor density in eagles that allows them to see smaller details.
  • πŸ”¬ The script explains the concept of folding the optical path in telescopes to achieve a higher magnification without increasing the physical size, as seen in modern telescopes.
  • πŸ“š The historical development of the Cassegrain telescope is mentioned, including its mathematical model and the limitations that led to improvements like the addition of a Schmidt plate.
  • πŸ›°οΈ Rik is currently working on a telescope for a space project by the University of Portland, which requires high precision and durability for use in a CubeSat.
  • πŸ”„ The process of creating aspherical surfaces, such as the secondary mirror, is detailed, explaining the challenges and techniques involved in achieving the desired shape.
  • πŸ’‘ The benefits of monolithic telescopes, including thermal stability and the lack of need for collimation, are discussed as advantages for space applications.
  • πŸš€ The script ends with a humorous take on the development of a 'Very Large Tiny Telescope' (VLTT), a concept that plays on the monolithic design's compactness while increasing aperture size.
Q & A
  • What is the unique feature of the telescope being discussed in the script?

    -The unique feature of the telescope is that it is made of a single piece of glass, which replaces the conventional optical and mechanical system of a Schmidt-Cassegrain telescope.

  • Who is Rik ter Horst and what is his profession?

    -Rik ter Horst is an optical engineer at NOVA-Astron, and he is the inventor and maker of the monolithic telescopes discussed in the script.

  • What is the significance of the reflective coating in the telescope's construction?

    -The reflective coating is crucial as it is the only thing missing before the telescope is complete. It allows the telescope to reflect and focus light properly, which is essential for its operation.

  • Why are long focal lengths important in telescopes?

    -Long focal lengths are important because they determine the size of the projected image, allowing for higher magnification and the ability to discern smaller details in objects.

  • How do eagles achieve a higher photoreceptor density compared to humans?

    -Eagles achieve a higher photoreceptor density due to having more photoreceptors per area in their retinas, which is 5-6 times higher than that of humans, allowing them to see smaller details.

  • What is the principle behind folding the optical path in telescopes?

    -Folding the optical path uses a combination of curved mirrors to create a system with the same effective focal length but in a more compact form, which is beneficial for large modern telescopes.

  • Who is credited with the original design of the Cassegrain telescope?

    -Laurent Cassegrain is credited with the original design of the Cassegrain telescope, which was published in 1672.

  • What is the role of the Schmidt plate in the telescope design?

    -The Schmidt plate serves to correct for field curvature and allows for the use of a spherical primary mirror instead of a parabola, simplifying the manufacturing process.

  • What is the advantage of making telescopes from a single piece of glass?

    -Making telescopes from a single piece of glass eliminates the need for separate optical elements and mechanical mounts, resulting in a more thermally stable, rigid, and compact design.

  • What is the space project that Rik ter Horst is working on and what is its purpose?

    -Rik ter Horst is working on a student space project from the University of Portland, where they are developing a CubeSat and require a camera with sufficient resolution to see the campus from space.

  • How does the process of making aspherical surfaces differ from making spherical surfaces?

    -Making aspherical surfaces is more complex because it requires non-uniform material removal over the surface area, often starting with a spherical surface and using smaller tools to create the desired aspherical shape.

  • What is the significance of the VLTT mentioned in the script?

    -The VLTT, or Very Large Tiny Telescope, is a concept for connecting four of the new generation 'ter Horst' telescopes using interferometers to create one very large telescope.

Outlines
00:00
🌌 The Art of Crafting a Monolithic Telescope

This paragraph introduces the unique process of creating a Schmidt-Cassegrain telescope from a single piece of glass, a craft mastered by Rik ter Horst, an optical engineer at NOVA-Astron. The telescope's compact size and monolithic design are highlighted, along with the background of optical components and the significance of focal length in magnification. The explanation covers the comparison between human and eagle eyes, the evolution of telescope design, and the concept of folding the optical path to achieve higher magnification without impractical lengths, exemplified by the Yerkes telescope. The paragraph concludes with the introduction of the Cassegrain telescope and its subsequent improvements, including the addition of a Schmidt plate for correcting field curvature and simplifying manufacturing.

05:04
πŸ› οΈ The Innovation of Solid Glass Telescopes

The second paragraph delves into the innovative concept of monolithic telescopes, which eliminate the need for separate optical elements and mechanical systems by integrating everything into a single piece of glass. This design not only simplifies the manufacturing process but also incorporates features like baffles directly into the glass, enhancing the optical performance. The discussion includes an interview with Rik ter Horst, who shares his background in making ophthalmic molds and his transition to crafting telescopes. The paragraph also touches on the time and effort required to handcraft these telescopes, especially for specialized projects like a space mission involving a CubeSat developed by the University of Portland.

10:04
πŸ‘¨β€πŸ”§ The Handcrafted Process of Telescope Making

This paragraph provides an in-depth look at the handcrafting process of monolithic telescopes in Rik's home workshop. Despite the high-tech nature of the telescopes, the process relies on traditional methods and minimal equipment. Rik explains the tools he uses, including a measuring device for parallelism, a thickness measuring tool, and test glasses for curvature checking. The polishing process is highlighted, with a focus on the time-consuming and meticulous work required for spherical and aspherical surfaces. The challenges of creating aspherical surfaces are discussed, emphasizing the need for non-uniform material removal and the iterative process to achieve the desired shape.

15:07
πŸš€ Advancing Telescope Technology for Space Applications

The final paragraph discusses the strategic advantages of monolithic telescopes, particularly their thermal stability and rigidity, which are beneficial for space applications. The interviewee, Dr. Liam, introduces the new generation of 'ter Horst' telescopes developed by Huygens Optics, which increases the aperture and mass-to-aperture ratio. The concept of connecting multiple telescopes using interferometers to create a Very Large Tiny Telescope (VLTT) is presented, showcasing the potential for innovative applications in astronomy.

Mindmap
Keywords
πŸ’‘Telescope
A telescope is an optical instrument that makes distant objects appear closer by using an arrangement of lenses or curved mirrors to gather and focus light. In the video's context, the focus is on a unique type of telescope, the Schmidt-Cassegrain, which is being crafted from a single piece of glass, showcasing the innovation in optical engineering.
πŸ’‘Schmidt-Cassegrain Telescope
The Schmidt-Cassegrain Telescope is a specific type of optical telescope that combines a spherical primary mirror with a corrective Schmidt plate and a secondary hyperbolic mirror to correct for spherical aberration. It is highlighted in the video for its compact design and high image quality, which is achieved without the need for a long linear construction.
πŸ’‘Reflective Coating
A reflective coating in the context of telescopes refers to a thin layer applied to the mirror surfaces to enhance their reflectivity and improve the quality of the image formed. The script mentions that the only thing missing from the telescope under construction is this reflective coating, which is crucial for its functionality.
πŸ’‘Optical Engineer
An optical engineer is a professional who specializes in the design and testing of optical components and systems. Rik ter Horst, the subject of the video, is an optical engineer at NOVA-Astron and is recognized for his expertise in crafting monolithic telescopes by hand, reflecting the artisanal aspect of this field.
πŸ’‘Focal Length
Focal length in optics is the distance from the center of a lens or curved mirror to the point where parallel rays of light converge after being reflected or refracted. The video explains that a longer focal length is necessary for higher magnification in telescopes, which is a key concept in understanding how these instruments function.
πŸ’‘Photoreceptor Density
Photoreceptor density refers to the number of photoreceptor cells per unit area in the retina, which affects the ability to discern fine details. The video uses the example of an eagle's eye to illustrate how higher photoreceptor density allows for better visual acuity, drawing a parallel to the function of a telescope's optics.
πŸ’‘Aspherical Surfaces
Aspherical surfaces are non-spherical shapes used in optical systems to correct for aberrations that occur with spherical shapes. The script discusses the difficulty in manufacturing aspherical surfaces, such as the convex hyperbolic secondary mirror in a Cassegrain telescope, which requires precise polishing techniques.
πŸ’‘Monolithic Telescope
A monolithic telescope, as introduced in the video, is a unique type of telescope made from a single piece of glass, incorporating all optical elements within the glass itself. This innovative design eliminates the need for separate mechanical components, streamlining the construction and potentially improving optical performance.
πŸ’‘Polishing
Polishing in the context of optical manufacturing is the process of smoothing and shaping the surface of a lens or mirror to achieve the desired optical properties. The video script describes the traditional and meticulous hand-polishing process used by Rik to create the aspherical surfaces of the telescope.
πŸ’‘CubeSat
A CubeSat is a type of miniaturized satellite that is commonly used for space research and technology demonstrations. The video mentions a student space project from the University of Portland that utilizes the monolithic telescope for its CubeSat, highlighting the practical applications of this technology in modern space exploration.
πŸ’‘Interferometers
Interferometers are devices that combine waves, typically light waves, to extract information about the waves' properties. In the video's closing, the concept of connecting multiple monolithic telescopes using interferometers to create a Very Large Tiny Telescope (VLTT) is introduced, showcasing the potential for scaling up this technology.
Highlights

Introduction of a telescope in the making, missing only the reflective coating.

The telescope is a tiny Schmidt-Cassegrain type, made from a single piece of glass.

Meeting with Rik ter Horst, an optical engineer at NOVA-Astron, known for crafting optical components to near perfection.

Rik's unique approach to handcrafting monolithic telescopes in contrast to mass manufacturing.

Basics of telescopes explained, emphasizing the importance of focal length for magnification.

Comparison of human and eagle eyes, highlighting the significance of photoreceptor density for detail discernment.

Historical context of telescope development, including the Yerkes telescope with a 19m focal length.

Explanation of how folding the optical path allows for more compact telescopes with long focal lengths.

The Cassegrain telescope design and its limitations due to aspherical reflective surfaces.

Introduction of the Schmidt plate as an improvement to the Cassegrain design, simplifying manufacture.

Popularity of Schmidt Cassegrain telescopes among amateur and professional astronomers.

The concept of monolithic telescopes, replacing the mechanical system with a single piece of glass.

Rik's background in the ophthalmic industry and the serendipitous start of his telescope-making journey.

The hands-on process of crafting these telescopes, typically taking weeks to months depending on requirements.

A space project involving a CubeSat and the specific requirements for the telescope's design and accuracy.

The simplicity of Rik's workshop, despite the high-tech nature of the telescopes being crafted.

Detailed description of the polishing process for spherical and aspherical surfaces.

The challenge of creating aspherical surfaces and the iterative process involved.

Strategic advantages of monolithic telescopes, particularly in thermal stability and lack of need for collimation.

Huygens Optics' development of a new generation 'ter Horst' telescope, with increased diameter and aperture area.

The concept of the Very Large Tiny Telescope (VLTT), connecting four 'ter Horst' telescopes using interferometers.

Transcripts
Rate This

5.0 / 5 (0 votes)

Thanks for rating: