PUNCH to launch with Tele Vue optical lenses

Posted on Saturday, March 1, 2025 by RICHARD HARRIS, Executive Editor

On Sunday, March 2, 2025, the night sky over California’s south-central coast will be illuminated by the launch of a Falcon 9 rocket from Vandenberg Space Force Base. Along with a small near-infrared observatory named SPHEREx, the NASA payload will include the PUNCH mission, which contains three Tele Vue Optical Lens Assemblies. Tele Vue was honored to be chosen for the project by the lead scientist, who, along with several colleagues at Southwest Research Institute (SwRI), is a long-time admirer of Tele Vue eyepieces and telescopes.

Image credit: SwRI and UCAR.

Nagler Type 7 eyepieces at Woodland Hills

The weekend will feature two major events in California, as the PUNCH launch coincides with the debut of the Nagler Type 7 eyepieces at Woodland Hills Camera & Telescope.

March 1, 2025 (11 AM – 4 PM)
Woodland Hills Camera & Telescope
5348 Topanga Canyon Blvd, Woodland Hills, CA

David and Sandy Nagler will be present at Woodland Hills Camera & Telescope on March 1, 2025, offering attendees an exclusive opportunity to explore the new Nagler Type 7 eyepieces. This event will provide astronomy enthusiasts with firsthand experience and insights into the Nagler Type 7 and other Tele Vue products.

PUNCH to launch with Tele Vue optical lenses

PUNCH, or the Polarimeter to UNify the Corona and Heliosphere, consists of four small satellites, each weighing approximately 45 kg (100 lbs). These satellites will be deployed into a 600 km-high, 90-minute polar Sun-synchronous orbit above Earth’s day/night terminator. Once in space, the satellites will gradually precess as Earth orbits the Sun, allowing their instruments to maintain a constant view of the Sun.

Three of the suitcase-sized satellites will be equipped with a Tele Vue-designed and manufactured objective lens for the Wide Field Imager (WFI) cameras. These lenses cover a 53° field of view across a 34.9 mm diagonal and are specially engineered to meet NASA’s launch and space durability standards. The cameras will work in tandem to capture images of the solar wind, spanning from 1.5° (6 R?) to 45° (180 R?) from the Sun. This solar wind not only creates the stunning auroras but also poses risks to power grids, satellites, and astronauts.

The fourth satellite will house the Narrow Field Imager (NFI), a coronagraph operating at f/4, designed to observe the solar corona and the immediate area surrounding the Sun. The fields of view of the three WFI cameras will slightly overlap with one another and with the NFI, ensuring continuous coverage of the entire inner solar system. This marks a significant milestone as the first solar observation mission of its kind.

With PUNCH, scientists aim to gain a deeper understanding of the Sun, the solar wind, and their impact on humanity. The two primary scientific objectives are:

Understanding how coronal structures become the ambient solar wind. Surprisingly little is known about the young solar wind as it departs from the corona. PUNCH seeks to answer key questions:

  • How does the young solar wind flow and evolve?
  • Where and how does the wind become turbulent?
  • What are the physical properties of the transition zone where the outer corona separates to become the ambient solar wind?
     

Understanding transient structures in the young solar wind. The solar wind is not a steady stream, it is disrupted by coronal mass ejections (CMEs), shocks, and other transient effects. PUNCH will capture these structures in 3D as they travel across the inner solar system, providing critical data to help predict space weather. The mission will also investigate:

  • CMEs and their impact on space weather forecasting
  • Corotating interaction regions where solar wind streams collide
  • Interplanetary shocks that accelerate high-energy particle showers
     

The WFI cameras are equipped with 8 GB CCD sensors that will take images of the Sun every 48 seconds using various polarizing filters. Between exposures, a filter wheel will spin, allowing vibrations to settle before the next image is captured. Each satellite is expected to generate 1.41 GB of compressed data per day, which will be stored onboard and transmitted to Earth via an X-band downlink (28.57 Mbit/s) with forward error correction every few days. The onboard computers will flag objects of interest in the images, including comets.

The mission is designed to last two years, with the possibility of an extension to five years. After this period, the CCD cameras will degrade due to exposure to charged particles, rendering them ineffective for further scientific observations. The PUNCH satellites will eventually re-enter Earth’s atmosphere approximately 25 years after launch. Additional details about NASA’s PUNCH mission can be found on the SwRI mission page.

Launch and viewing information

  • What: Launch of PUNCH with SPHEREx
  • Where: Vandenberg Space Force Base, Space Launch Complex 4 East
  • Time: Sunday, March 2, 7:09 PM PST / 10:09 PM EST (3:09 UT, Monday, March 3)
  • Orbit: Polar, Low Earth Orbit
  • Landing: Booster will return to launch site
  • Viewing: The Falcon 9 rocket will launch toward the south, with its plume likely visible across Southern California, including Los Angeles.
     

Streaming coverage

Punch Lens Prototype


Nagler Type 7 eyepiece specifications

  • Optical Design: Ultra-wide-angle, high-performance eyepiece
  • Field of View: 82° apparent field
  • Eye Relief: Comfortable long eye relief for extended viewing
  • Lens Elements: Premium multi-coated optics for maximum contrast and clarity
  • Compatibility: Available in multiple focal lengths, optimized for various telescope types
  • Barrel Size: 1.25" and 2" models available
  • Weight: Varies by focal length; designed for balance and ease of use
     

Woodland Hills event information

  • What: Nagler Type 7 Eyepiece Event with David and Sandy Nagler
  • Where: Woodland Hills Camera & Telescope, 5348 Topanga Canyon Blvd, Woodland Hills, CA
  • When: Saturday, March 1, 2025, from 11 AM - 4 PM
  • Who: Hosted by Tele Vue, featuring David and Sandy Nagler
  • Why Attend?
    • - Get a firsthand look at the new Nagler Type 7 eyepieces
    • - Meet the creators and learn about Tele Vue products
    • - Explore and test various astronomy accessories
    • - Ask questions and get expert advice
       

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