Interstellar Probe (spacecraft)

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Interstellar Probe
Interstellar Probe (2020s).png
Artist's rendering of the Interstellar Probe (plasma wave antennas extend far beyond portion shown)
Mission typeOuter planetary, heliosphere, and interstellar medium exploration
Operator NASA / Johns Hopkins Applied Physics Laboratory
Website interstellarprobe.jhuapl.edu
Spacecraft properties
Launch mass860 kg (1,900 lb)
Power470 watts (at launch)
Start of mission
Launch date2036
Rocket Space Launch System Block 2
Flyby of Jupiter
Closest approach2037
Distance~4 000 km
 

Interstellar Probe (ISP) is a proposed NASA space probe designed to explore and characterize the heliosphere and interstellar space. The study was originally proposed in 2018 by NASA for the Applied Physics Laboratory. It would have a baseline launch between 2036 and 2041. [1] The probe would launch on a direct hyperbolic trajectory to encounter Jupiter after six to seven months, after which the probe would travel at a speed of about 6–7 astronomical units (900,000,000–1.05×109 kilometres) per year, leaving the heliosphere after only 16 years. [2]

Contents

The probe may have the opportunity to encounter minor planets on the way out, including Orcus and Quaoar, though such flybys would require specific launch dates. With next-generation radioisotope thermoelectric generators (RTGs), the mission would be designed to last for over 50 years after its launch, a similar feat reached by the Voyager 1 and 2 probes despite their intended 5-year lifetime. The mission has been called "Voyager on steroids". [2]

Mission background

Interstellar probes such as the Voyager program were made only with the intent to visit the outer planets, with the added interstellar mission as a mere bonus. Their lifetime had never been expected to be much longer than 12 years at the most, but the probes have lasted for upwards of four decades thus far. Both Voyagers left the heliosphere in the 2010s; Voyager 1 in 2012, [3] and 2 in 2018. [4]

While their readings have been valuable, many of their instruments have been shut off due to a lack of power in their RTGs. In addition, neither of them are headed toward the IBEX ribbon, a region discovered by the Interstellar Boundary Explorer where energetic neutral atoms (ENAs) seem to highly affect the heliosphere and are able to breach it at unprecedented rates. [5]

A graph displaying the IBEX ribbon juxtaposed with flyby speed and secondary targets Interstellar IBEX ribbon and dwarf planets.png
A graph displaying the IBEX ribbon juxtaposed with flyby speed and secondary targets

Primary science goals

The main goals of the Interstellar mission include characterizing the heliosphere as a habitable astrosphere by its global nature, its interactions with the Sun and the interstellar medium, and the nature of said interstellar medium. Similar goals may include viewing the Sun as a habitable exoplanetary system from beyond, with potential outbound giant or dwarf planet flybys along the way depending on chosen launch date, and understanding the universe from beyond the heliosphere. [1]

Scientific instruments

The probe would contain two differing scientific payloads, both weighing about 85–90 kg (187–198 lb). One would prioritize Lyman-alpha science, whereas the other would prioritize visible and infrared imaging of flyby targets. [1] Payloads highlighted in red are exclusive to the baseline payload. Instruments in green are intended for the augmented flyby payload.

Instrument (abbr.)Dimension, range, resolutionHeritage
Magnetometer (MAG) Electromagnetic radiation:
0.01–100 nT
Magnetospheric Multiscale: DFG
Plasma Waves (PWS)Plasma wave observations:
~1 Hz – 5 MHz, ≤0.7 µV/m at 3 kHz, ∆f/f ≤ 4%, ≤60 s full spectrum
Van Allen: EFW
Plasma Subsystem (PLS)Ion spectrometer:
< 3 eV/e to 20 keV/e
Parker Solar Probe: SWEAP, Span-A
Pick-Up Ions (PUI)Ion counter: 0.5–78 keV/e Ulysses : SWICS
Energetic Particles (EPS)Ionization analysis: 20 keV – 20 MeVParker Solar Probe: IS☉IS, EPI-Lo
Cosmic Rays (CRS)Cosmic ray analysis: H to Sn; 10 MeV/nuc – 1 GeV/nucParker Solar Probe: IS☉IS, EPI-Hi
Interstellar Dust Analyzer (IDA)Dust analysis: 10−19 to 10−14 g Interstellar Mapping and Acceleration Probe: IDEX
Neutral Mass Spectrometer (NMS)H, 3
He
, 4
He
, 14
N
, 16
O
, 20
Ne
, 22
Ne
, 36
Ar
, 38
Ar
, m/Δm ≥ 100
Jupiter Icy Moons Explorer: NMS
Energetic Neutral Atom Imager (ENA)Images emission of energetic neutral atoms; ~1–100 keV HInterstellar Mapping and Acceleration Probe: IMAP-Ultra
Lyman-Alpha Spectrograph (LYA)Mapping solar wind interactions with interstellar medium:
±100 km/s Doppler range, <10 km/s resolution
MAVEN: IUVS
Visible-Near-IR (VIR)Flyby imaging:
0.4–4 µm; ≥ 5 ch. ≤0.975 µm
>240 ch. >0.975 µm
New Horizons : Ralph
Visible-IR Mapper (IRM)Infrared mapping:
0.5–15 µm
30–100 µm
New Horizons : LEISA, CIBER-2

Mission operations

The baseline trajectory, using a passive gravity assist at Jupiter Interstellar (2020) baseline trajectory.png
The baseline trajectory, using a passive gravity assist at Jupiter
The Solar Oberth trajectory, using a brake at Jupiter for a burn at perihelion Interstellar Solar Oberth.png
The Solar Oberth trajectory, using a brake at Jupiter for a burn at perihelion

Launch and trajectories

The baseline launch would be in 2036 using a Space Launch System in its Block 2 configuration, featuring an additional Centaur and Star 48BV booster. This launch would put the probe on a direct trajectory to Jupiter, and after a mere seven months the probe would make a gravity assist to speed out at about 95 km/s (about 216000 mph). [1] Alternative trajectories include bringing the Star 48 booster for a burn upon closest approach; one trajectory involving that burn at Jupiter with a slightly longer transit time, and another with about the same transit time, but passing ahead of Jupiter for a dive down near the Sun for an even faster escape trajectory. [1]

Further trajectory options have been considered, including performing flybys of Saturn, Uranus, or Neptune depending on launch date to help characterize planetary formation and complement missing data sets, and dwarf planets to help characterize them as New Horizons did in 2015 with its flyby of Pluto. [1]

See also

Related Research Articles

<i>Voyager 1</i> NASA space probe launched in 1977

Voyager 1 is a space probe launched by NASA on September 5, 1977, as part of the Voyager program to study the outer Solar System and interstellar space beyond the Sun's heliosphere. Launched 16 days after its twin Voyager 2, Voyager 1 has been operating for 46 years and 20 days as of September 25, 2023 UTC [refresh]. It communicates through the NASA Deep Space Network to receive routine commands and to transmit data to Earth. Real-time distance and velocity data is provided by NASA and JPL. At a distance of 161 AU from Earth as of August 2023, it is the most distant human-made object from Earth.

<i>Voyager 2</i> NASA "grand tour" planetary probe

Voyager 2 is a space probe launched by NASA on August 20, 1977, to study the outer planets and interstellar space beyond the Sun's heliosphere. As a part of the Voyager program, it was launched 16 days before its twin, Voyager 1, on a trajectory that took longer to reach gas giants Jupiter and Saturn but enabled further encounters with ice giants Uranus and Neptune. Voyager 2 remains the only spacecraft to have visited either of the ice giant planets. Voyager 2 was the third of five spacecraft to achieve Solar escape velocity, which allowed it to leave the Solar System.

<span class="mw-page-title-main">Voyager program</span> Ongoing NASA interstellar program

The Voyager program is an American scientific program that employs two robotic interstellar probes, Voyager 1 and Voyager 2. They were launched in 1977 to take advantage of a favorable alignment of the two gas giants Jupiter and Saturn and the ice giants, Uranus and Neptune, to fly near them while collecting data for transmission back to Earth. After launch the decision was made to send Voyager 2 near Uranus and Neptune to collect data for transmission back to Earth.

<i>New Horizons</i> NASA probe that visited Pluto and Kuiper belt object 486958 Arrokoth

New Horizons is an interplanetary space probe that was launched as a part of NASA's New Frontiers program. Engineered by the Johns Hopkins University Applied Physics Laboratory (APL) and the Southwest Research Institute (SwRI), with a team led by Alan Stern, the spacecraft was launched in 2006 with the primary mission to perform a flyby study of the Pluto system in 2015, and a secondary mission to fly by and study one or more other Kuiper belt objects (KBOs) in the decade to follow, which became a mission to 486958 Arrokoth. It is the fifth space probe to achieve the escape velocity needed to leave the Solar System.

<span class="mw-page-title-main">Heliosphere</span> Region of space dominated by the Sun

The heliosphere is the magnetosphere, astrosphere, and outermost atmospheric layer of the Sun. It takes the shape of a vast, bubble-like region of space. In plasma physics terms, it is the cavity formed by the Sun in the surrounding interstellar medium. The "bubble" of the heliosphere is continuously "inflated" by plasma originating from the Sun, known as the solar wind. Outside the heliosphere, this solar plasma gives way to the interstellar plasma permeating the Milky Way. As part of the interplanetary magnetic field, the heliosphere shields the Solar System from significant amounts of cosmic ionizing radiation; uncharged gamma rays are, however, not affected. Its name was likely coined by Alexander J. Dessler, who is credited with the first use of the word in the scientific literature in 1967. The scientific study of the heliosphere is heliophysics, which includes space weather and space climate.

<span class="mw-page-title-main">Grand Tour program</span> NASAs space program intended to explore the outer solar system

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<span class="mw-page-title-main">Interstellar probe</span> Space probe that can travel out of the Solar System

An interstellar probe is a space probe that has left—or is expected to leave—the Solar System and enter interstellar space, which is typically defined as the region beyond the heliopause. It also refers to probes capable of reaching other star systems.

<span class="mw-page-title-main">Exploration of Saturn</span> Overview of the exploration of Saturn

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<span class="mw-page-title-main">Exploration of Neptune</span> Overview of the exploration of Neptune

Neptune has been directly explored by one space probe, Voyager 2, in 1989. As of September 2023, there are no confirmed future missions to visit the Neptunian system, although a tentative Chinese mission has been planned for launch in 2024. NASA, ESA, and independent academic groups have proposed future scientific missions to visit Neptune. Some mission plans are still active, while others have been abandoned or put on hold.

<span class="mw-page-title-main">Innovative Interstellar Explorer</span> NASA proposed space probe to 1000 AU from the Sun

Innovative Interstellar Explorer was a NASA "Vision Mission" study funded by NASA following a proposal under NRA-03-OSS-01 on 11 September 2003. This study focused on measuring the interstellar medium, the region outside the influence of the nearest star, the Sun. It proposes to use a radioisotope thermal generator to power ion thrusters.

<span class="mw-page-title-main">Heliophysics Science Division</span>

The Heliophysics Science Division of the Goddard Space Flight Center (NASA) conducts research on the Sun, its extended Solar System environment, and interactions of Earth, other planets, small bodies, and interstellar gas with the heliosphere. Division research also encompasses geospace—Earth's uppermost atmosphere, the ionosphere, and the magnetosphere—and the changing environmental conditions throughout the coupled heliosphere.

<i>Argo</i> (NASA spacecraft) 2009 NASA spacecraft mission concept

Argo was a 2009 spacecraft mission concept by NASA to the outer planets and beyond. The concept included flybys of Jupiter, Saturn, Neptune, and a Kuiper belt object. A focus on Neptune and its largest moon Triton would have helped answer some of the questions generated by Voyager 2's flyby in 1989, and would have provided clues to ice giant formation and evolution.

<span class="mw-page-title-main">Interstellar Mapping and Acceleration Probe</span> Planned NASA heliophysics mission

The Interstellar Mapping and Acceleration Probe(IMAP) is a heliophysics mission that will simultaneously investigate two important and coupled science topics in the heliosphere: the acceleration of energetic particles and interaction of the solar wind with the local interstellar medium. These science topics are coupled because particles accelerated in the inner heliosphere play crucial roles in the outer heliospheric interaction. In 2018, NASA selected a team led by David J. McComas of Princeton University to implement the mission, which is currently planned to launch in February 2025. IMAP will be a Sun-tracking spin-stabilized satellite in orbit about the Sun–Earth L1 Lagrange point with a science payload of ten instruments. IMAP will also continuously broadcast real-time in-situ data that can be used for space weather prediction.

Trident is a space mission concept to the outer planets proposed in 2019 to NASA's Discovery Program. The concept includes flybys of Jupiter and Neptune with a focus on Neptune's largest moon Triton.

<span class="mw-page-title-main">Neptune Odyssey</span> NASA orbiter mission concept to study the Neptune system

Neptune Odyssey is an orbiter mission concept to study Neptune and its moons, particularly Triton. The orbiter would enter into a retrograde orbit of Neptune to facilitate simultaneous study of Triton and would launch an atmospheric probe to characterize Neptune's atmosphere. The concept is being developed as a potential large strategic science mission for NASA by a team led by the Applied Physics Laboratory at Johns Hopkins University. The current proposal targets a launch in 2033 using the Space Launch System with arrival at Neptune in 2049, although trajectories using gravity assists at Jupiter have also been considered with launch dates in 2031.

Interstellar Express or Interstellar Heliosphere Probe, is the current name for a proposed Chinese National Space Administration program designed to explore the heliosphere and interstellar space. The program will feature two space probes that will purportedly be launched in 2024 and follow differing trajectories to encounter Jupiter to assist them out of the Solar System. The first probe, IHP-1, will travel toward the nose of the heliosphere, while the second probe, IHP-2, will fly near to the tail, skimming by Neptune and Triton in January 2038. There may be another probe—tentatively IHP-3—which would launch in 2030 to explore to the northern half of the heliosphere. IHP-1 and IHP-2 would be the sixth and seventh spacecraft to leave the Solar System, as well as first non-NASA probes to achieve this status.

References

  1. 1 2 3 4 5 6 McNutt, Ralph; Paul, Michael; Brandt, Pontus; Kinnison, Jim. "Interstellar Probe: Humanity's Journey to Interstellar Space" (PDF). Interstellar Probe. Johns Hopkins Applied Physics Laboratory. Retrieved 23 December 2021.
  2. 1 2 Stone, Richard (28 July 2022). "'Voyager on steroids.' Mission would probe mysterious region beyond our Solar System". Science. doi:10.1126/science.ade1070 . Retrieved 15 August 2022.
  3. "Interstellar Mission". NASA Jet Propulsion Laboratory . Retrieved August 24, 2020.
  4. University of Iowa (November 4, 2019). "Voyager 2 reaches interstellar space – Iowa-led instrument detects plasma density jump, confirming spacecraft has entered the realm of the stars". EurekAlert! . Retrieved November 4, 2019.
  5. Baldwin, Emily (October 15, 2009). "IBEX maps edge of Solar System". Astronomy Now. Archived from the original on September 21, 2016. Retrieved August 14, 2016.

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