Roman Coronagraph: A New Tool for Planetary Observation
The Roman Coronagraph aims to enhance our view of distant planets.
Schuyler G. Wolff, Jason Wang, Karl Stapelfeldt, Vanessa P. Bailey, Dmitry Savransky, Justin Hom, Beth Biller, Wolfgang Brandner, Ramye Anche, Sarah Blunt, Marah Brinjikji, Julien H. Girard, Oliver Krause, Zhexing Li, John Livingston, Maxwell A. Millar-Blanchaer, Malachi Noel, Laurent Pueyo, Robert J. De Rosa, Matthias Samland, Nicholas Schragal
― 6 min read
Table of Contents
The Roman Coronagraph is a cool tool that will be part of the Nancy Grace Roman Space Telescope. It is expected to launch in late 2026 or early 2027 and will help us look at distant planets outside our solar system, specifically those that might be rocky and have conditions similar to Earth.
The main goal here is to take pictures of these planets without too much pesky star light getting in the way. Just think of it like trying to take a selfie at a party where the sun is shining right in your eyes. We want to see those planets clearly, and the Roman Coronagraph is designed to help do just that!
What’s Happening with Observations?
In its first 18 months of operation, the Roman Coronagraph will have special observation sessions. During these times, it will attempt to capture images of planets that are similar to Jupiter, but that are quite far away. The people working on this project are currently focused on planning these observations carefully.
There’s a group dedicated to this Planning which is called the Observation Planning Working Group (OPWG). This team is a mix of about 50 enthusiastic folks from different stages in their careers from all over the world. They’ve been gathering since November 2023 to discuss which planets to observe and how best to do it.
Precursor Observations
Before the big Roman Coronagraph kicks off its major observations, the team is doing some prep work. They’re taking preliminary images of potential target stars that might hide planets. This is like checking out a restaurant’s menu before making a reservation—gotta know what you’re getting into!
While these plans are solid, the team knows that things can get a bit tricky. Some stars they want to observe may have other faint stars lurking around them, making it harder to see the planets. They’ve already gathered data from Keck Observatory to get a head start in figuring out which stars could make good targets.
Cleaning Up the Mess
As the team starts collecting data, they need to clean it up too. They’ve created a system to process the images they gather from Keck. Think of it as washing vegetables before cooking. The data has all sorts of bits and pieces that need to be sorted out.
These images get even more attention from the software they’re using, which helps them line everything up properly. The team is making sure they can find any background stars that might interfere with their focus. They’re not just winging it; they want to be well-prepared!
The Reference Star Catalog
Now, before we dive back into the juicy bits about planets, let’s talk about reference stars. These stars are like trusty sidekicks in superhero movies, always there to help out. The Roman Coronagraph needs these bright reference stars to create a perfect dark space around the star it’s trying to study.
They need to be bright and single—no star couples allowed! This is to ensure the Coronagraph can keep a steady eye on things and not get distracted. The team has been busy hunting for these stars, collecting information from various catalogs and ensuring they meet the criteria.
The Campaign for Companions
Starting in 2024, the OPWG plans to kick off a campaign to find companions for these reference stars. This involves taking close-up images of the stars to check for any hidden partners that might hurt their plans. They’ll use different methods to spot these companions, making sure they’re not blindsided.
This is crucial because the presence of nearby stars could mess up the observations they want to make. It’s a bit like having a noisy roommate while you’re trying to study—very distracting!
Building a Better Database
As they work through these stars, the OPWG is building a comprehensive database. The Imaging Mission Database collects all relevant information about stars and planets. This makes it easier to track which stars are good for observations and helps in planning everything more efficiently.
There are plans to expand this database to include even more information about other science targets. It’s like upgrading your phone—better features and more options help you do things faster!
Exposure Time Calculator
Next, we have the Exposure Time Calculator (ETC). This handy tool will help scientists determine how long they need to observe each target star. It’s like setting an alarm clock for the right time to get out of bed.
With the ETC, users will have access to various scenarios based on the predicted performance of the Roman Coronagraph. This will allow them to plan effectively and know when to hit that “record” button.
Observing Programs
There will be multiple observing programs lined up to help the Coronagraph fulfill its mission. These programs will work to ensure the Coronagraph meets its requirements for observing time and image quality. It’s like training for a marathon, with different runs designed to improve various aspects of performance.
The OPWG is collecting ideas for these observing programs as they want to explore a wide range of topics. They’re looking at everything from the stability of the instruments to the performance of the imaging capabilities, making sure they leave no stone unturned.
Community Involvement
One exciting part of this whole project is that the OPWG wants to involve the community. They’re putting together a survey asking for input from scientists and researchers who are interested in what the Coronagraph can do. It’s a way to make sure everyone can share their thoughts and ideas.
Participants will be asked to rank their preferences for different science cases. This way, the team can focus on what people are most excited about and make sure they’re aligned with community interests.
The Bigger Picture
Getting down to the nitty-gritty of space observations is all well and good, but the ultimate goal is to make discoveries that shed light on the universe. The Roman Coronagraph aims to provide a better view of the cosmos, uncovering insights that could teach us more about the formation of planets and even our own place in the universe.
With the right technology and careful planning, we may finally be able to directly observe planets that could potentially host life, and that’s truly exciting!
Wrapping Up
As we wait for the Nancy Grace Roman Space Telescope to launch, it’s great knowing there’s a dedicated group of people working hard to make these observations happen. They’re taking their time to carefully choose targets, collect data, and clear the way for what’s to come.
With community involvement and a strong support system, we’re all set for some breathtaking discoveries that could change what we know about our universe. Who knows? One day, we might just find that there’s more out there than we ever dreamed of!
So, fasten your seatbelts and get ready for a cosmic roller coaster ride that could take us to new heights. The stars are just the beginning!
Title: The Roman coronagraph community participation program: observation planning
Abstract: The Coronagraphic Instrument onboard the Nancy Grace Roman Space Telescope is an important stepping stone towards the characterization of habitable, rocky exoplanets. In a technology demonstration phase conducted during the first 18 months of the mission (expected to launch in late 2026), novel starlight suppression technology may enable direct imaging of a Jupiter analog in reflected light. Here we summarize the current activities of the Observation Planning working group formed as part of the Community Participation Program. This working group is responsible for target selection and observation planning of both science and calibration targets in the technology demonstration phase of the Roman Coronagraph. We will discuss the ongoing efforts to expand target and reference catalogs, and to model astrophysical targets (exoplanets and circumstellar disks) within the Coronagraph's expected sensitivity. We will also present preparatory observations of high priority targets.
Authors: Schuyler G. Wolff, Jason Wang, Karl Stapelfeldt, Vanessa P. Bailey, Dmitry Savransky, Justin Hom, Beth Biller, Wolfgang Brandner, Ramye Anche, Sarah Blunt, Marah Brinjikji, Julien H. Girard, Oliver Krause, Zhexing Li, John Livingston, Maxwell A. Millar-Blanchaer, Malachi Noel, Laurent Pueyo, Robert J. De Rosa, Matthias Samland, Nicholas Schragal
Last Update: 2024-11-26 00:00:00
Language: English
Source URL: https://arxiv.org/abs/2411.17868
Source PDF: https://arxiv.org/pdf/2411.17868
Licence: https://creativecommons.org/licenses/by/4.0/
Changes: This summary was created with assistance from AI and may have inaccuracies. For accurate information, please refer to the original source documents linked here.
Thank you to arxiv for use of its open access interoperability.
Reference Links
- https://github.com/MalachiNoel3/kecknirc2pipeline
- https://docs.google.com/spreadsheets/d/1p5r0VmjBCjXU25daJl5oJOPoPh1V79nuESbnwmca0s0/edit?usp=sharing
- https://romancgi.sioslab.com
- https://www.exoplanetdatachallenge.com/SIT
- https://plandb.sioslab.com/
- https://plandb.sioslab.com/docs/html/index.html
- https://github.com/hsergi/Roman_Coronagraph_ETC