What could be NASA’s next big space telescope mission?

Of course, after the James Webb Space Telescope is launched

A three-day symposium, facilitated by the Universities Space Research Association (USRA) entitled The Space Astrophysics Landscape for the 2020s and Beyond started on Monday at the William F. Bolger Center in Maryland, USA. 

Three Day Symposium on The Space Astrophysics Landscape for the 2020s and Beyond (Credits: @CastorMission)

Three Day Symposium on The Space Astrophysics Landscape for the 2020s and Beyond (Credits: @CastorMission)

On the inaugural day, a bulk of the symposium’s talks was about NASA's prospective future space telescope missions - HabEX, LUVOIR, Lynx, and the Origins Space Telescope. Already, there is stiff competition among the four projects to become NASA’s next flagship mission — the next Hubble or James Webb. 

Of course, the James Webb Space Telescope (JWST) is yet to be launched. Last month, an independent review board raised concerns about the project’s ability to stay on track for a launch within the next two years. Also in line is the Wide Field Infrared Survey Telescope (WFIRST) that was the top-ranked flagship mission in NASA's last decadal survey, and is currently facing a major funding crunch

Having said that, it has become all the more important now to plan better for upcoming space telescope missions - keeping in mind the hurdles faced by JWST and WFIRST.

James Webb Space Telescope Full Size Model (Credits: NASA)

Here's a look at each of NASA’s four space telescope concept missions that were discussed during the symposium. 

OST: The Origins Space Telescope

The Origins Space Telescope is the concept for an infrared telescope with a 5.9-meter diameter mirror, and would be two to four orders of magnitude more sensitive than the European Space Agency’s former Herschel Observatory

As the name suggests, OST will be designed to search for the origins of galaxies and planets. This will help us look for exoplanets spinning around smaller and colder stars, and in gazing deeper into parts of the universe from where very weak electromagnetic signals reach Earth. OST’s infrared detection capabilities will also allow us to track how water is transported and formed in young planets, asteroids, meteorites, and comets. This could potentially improve our understanding of how planets like Earth form. 

In February, Johannes Staguhn, principal scientist at Johns Hopkins University and on the Origins Space Telescope team told Science Friday that in about two finger snaps, OST would have obtained as much mapping potential on the sky as the Herschel Observatory had done during its entire mission.

But we may not see OST launched into operation for another 20-30 years as some instruments that will be part of its conceptualized mission need a few more years of rigorous innovation to meet operational standards. This is particularly so with the far-infrared spectroscopy systems proposed for the telescope which according to an interim report submitted last year “requires an increase in sensitivity.”

Origins Space Telescope (Credits: NASA/GSFC)

Origins Space Telescope (Credits: NASA/GSFC)

Diagram of the conceptualized lens diameter of OST (Credits: Wikimedia Commons)

Diagram of the conceptualized lens diameter of OST (Credits: Wikimedia Commons)

Concept Image of OST (Credits: NASA)

Concept Image of OST (Credits: NASA)

Lynx

To understand space-telescopes better, it helps to know the distribution of different kinds of radiation across the electromagnetic spectrum. We have low-frequency radio waves towards one end, the visible portion of light in the middle, and X-rays and Gamma rays towards the high-frequency end. 

The spectrum of electromagnetic waves and their common sources (Credits: Wikimedia Commons)

The spectrum of electromagnetic waves and their common sources (Credits: Wikimedia Commons)

As you can see from the chart above, high energy waves have more frequency. So naturally, the radiation from the biggest booms and bangs from the farthest ends of the universe that reach Earth are shifted towards the spectrum’s high frequency end. This is one of the main reasons why X-ray telescopes are used in the discovery of blackholes and neutron stars. And since the earth’s atmosphere absorbs X-rays, making none available for observers on the ground, we have no option but to launch these telescopes into space.

Lynx, if and when launched, would give astrophysicists the power to view the depths of the cosmos with X-ray vision. 

Concept image of Lynx Space Telescope (Credits: NASA)

Concept image of Lynx Space Telescope (Credits: NASA)

What makes Lynx special is how it compares to the currently most powerful X-ray telescope - Chandra. An interim document produced last year noted that Lynx is bounds ahead of both Chandra, and another X-ray telescope currently in development - Athena.  The report added:

Across the board, Lynx will be capable of making generational advances enabled by leaps in capability over NASA’s existing flagship Chandra and the European Space Agency’s planned Athena mission: 100-fold increase in sensitivity via coupling superb angular resolution with high throughput; 16 times larger field of view (FOV) for sub-arcsecond imaging; and 10–20 times higher spectral resolution for both point-like and extended sources.

The report also mentions that the telescope when built according to its concept plan will be powerful enough to detect X-rays from far away black holes, and can also throw light on some of the first galaxies to have formed in the early universe. Lynx can also help us look at cosmic environments ranging from young stars and their planets, to high energy bursts coming from supermassive black holes and neutron stars. With these inputs we can better understand what forces drive the formation of galaxies, and more about how stars evolve.

Once Athena is operational, a later Lynx launch may also see the two telescopes working together, as was discussed during the symposium by astrophysicist Alexey Vikhlinin.

Earlier this year, Grant Tremblay, a team member of the Lynx study told Katie Feather of Science Friday that the telescope could be the most powerful X-ray observatory ever flown to space by several orders of magnitude, and across multiple dimensions. “It would do science from the poles of Jupiter to black holes at the edge of time and everything in between,” he told Feather.

LUVOIR: Large UV/Optical/IR Surveyor

LUVOIR is probably the most ambitious among the four telescopes. While Hubble’s primary mirror is 2.4 meters in diameter, the LUVOIR team is planning for two different sizes for its mirrors - One is 8 meters in diameter, and another is 12-15 meters

Comparison of mirror sizes across Hubble, James Webb, and LUVOIR space telescopes (Credits: @Shamrocketeer)

Comparison of mirror sizes across Hubble, James Webb, and LUVOIR space telescopes (Credits: @Shamrocketeer)

LUVOIR would help us get more answers for critical questions in astronomy like how galaxies assemble; how stars form; and if life exists beyond our planet. It will scope in on rocky Earth-like exoplanets orbiting the habitable zones around stars similar to our Sun.

By functioning in the UV/Optical/IR parts of the spectrum, the large and powerful telescope would be able to directly image such exoplanets, and identify whether they have key signals of life such as water, oxygen, carbon dioxide, methane, or other such signs.

LUVOIR can image galaxies hundreds of times quicker than the Hubble Space Telescope. To put that in perspective, the following image was taken by the Hubble Space Telescope's Ultra-Deep Field image, and it took the telescope more than a week, and over 100 hours of exposure to capture. 

Hubble Space Telescope's Ultra Deep-Field View: This image containing over 10,000 galaxies was formed from the data accumulated by the Hubble Space Telescope from September 2003 to January 2004. (Credits: NASA)

Hubble Space Telescope's Ultra Deep-Field View: This image containing over 10,000 galaxies was formed from the data accumulated by the Hubble Space Telescope from September 2003 to January 2004. (Credits: NASA)

John O’Meara, the cosmic origins science lead for LUVOIR told Science Friday that the same image will be done in 47 minutes with LUVOIR. 

LUVOIR Concept art (Credits: NASA)
LUVOIR Concept art (Credits: NASA)

HabEx

HabEx - short for the Habitable Exoplanet Observatory - is the concept for a four-meter long, stable telescope operating in the UV, optical, and very near-IR ranges of the electromagnetic spectrum. Its operation is similar to that of the Hubble Space Telescope, but is planned to be 10 times as large in area

By operating in the UV/Visible/IR wavelengths, HabEx will be able to look for the best chemical signatures for life in exoplanets. (Credits: NASA)

By operating in the UV/Visible/IR wavelengths, HabEx will be able to look for the best chemical signatures for life in exoplanets. (Credits: NASA)

As the name suggests, HabEx will mainly try to directly image habitable Earth-like exoplanets, and throw some light on the contents of their atmosphere. It will also be looking at all other types of planets. 

Astrophysicist Scott Gaudi updated in the symposium that the concept architecture design for HabEx was nearly complete.

The habitable zone in a solar system is like the porridge Goldilocks finds “just right” in the story of Goldilocks and the Three Bears. It is a region around a star that is neither too close (and hot) nor far way from it (and cold), making the region conducive for life to flourish. When trying to look for planets in the Goldilocks zone, the light and radiation from the sun-like star itself could glare out any prospect of looking at the planets. So, one of HabEx’s proposed instruments is a starshade, which when deployed from the telescope, physically blocks out the light from the Sun-like stars and helps focus only on the planets.

The trickiest thing about the starshade is that it will be carried in a folded state by the telescope and will expand to its operational form when deployed.

Concept video of a starshade deploying from a telescope (Credits: TED)

Concept video of a starshade deploying from a telescope (Credits: TED)

By doing this, HabEx will look for life sustainability signatures in these planets. HabEx will also help us understand more about the earliest epochs of the universe, and the life cycle and deaths of some of the largest stars. Studying these would in turn tell us about the source of some of the elements in the periodic table, and how they end up assembling into life forms in habitable zones of the cosmos. 

NASA HabEx with screenshade deployed (Credit: NASA)

NASA HabEx with screenshade deployed (Credit: NASA)

HabEx with a deployed starshade to look at Habitable Exoplanets (Credits: NASA)

HabEx with a deployed starshade to look at Habitable Exoplanets (Credits: NASA)

What lies ahead for these mission concepts?

These are ambitious projects that will try to answer some of the most fundamental questions in astrophysics. But only one of them may get pushed to become NASA's next flagship telescope project- even if the launch and operation of any of these in space is definitely more than a decade away.

Later in the year, these projects will be assessed by a decadal survey conducted jointly by the Board of Physics and Astronomy, and the Space Studies Board of the National Academies. In June last year, A NASA press release noted that the cost caps of missions working towards the 2020 Decadal Survey would be narrowed down to $3-5 billion. This reflected a need for the agency to balance its astrophysics program within anticipated budget constraints.

NASA Astrophysicist Ira Thorpe's tweet following the symposium reflected what kind of budget constraint exists.

Discussions at the symposium also reflected on doubts among astrophysicists if in the current trajectory of American astrophysics, space explorers and probes would be prioritized more compared to strategic flagship missions.

In 2016, when NASA initiated these telescope studies, it aimed for them to be prioritized by the Decadal Survey for launch in the 2030s right after JWST and WFIRST. This survey matters because it is a useful resource for agencies supporting astronomy and astrophysics, the Congressional committees that have jurisdiction over those agencies, the scientific community, and the public. 

The agency’s aim in 2016 was to design a mission that could deliver the best results for the spent capital. However, with recent delays and budget constraints surrounding JWST and WFIRST, there could be a change in direction among these contenders for NASA's next flagship mission. Since the last flagship missions became operational, inflation has also made it difficult to budget for new missions, as Christopher Stark -Associate Scientist at Space Telescope Science Institute - noted in his tweet:

Hence, there's more pressure on the contendors for the next space telescope mission to submit a concept note that better ensures delivery within a quoted time and budget.

The final report on the four space telescopes is expected to be submitted to the decadal committee for review by September. According to the American Astronomical Society’s website, the survey results for the next decade is expected to be released by mid-2020.

So it will be interesting to see if there's any change in trajectory these projects may undergo after the symposium to better meet the requirements and expectations of the decadal committee.