Mars Exploration News
MARSDAILY
Effect of geometric porosities on aerodynamic characteristics of supersonic parachutes
File illustration only
Effect of geometric porosities on aerodynamic characteristics of supersonic parachutes
by Staff Writers
Beijing, China (SPX) Sep 08, 2023

The safe landing of the probe is one of the most difficult challenges in Mars exploration, and the Mars supersonic parachute is extremely important for this process. To date, all the successful Mars exploration missions have used disk-gap-band (DGB) parachutes. However, the DGB parachute with the highest diameter of 21.35 m cannot be further used for future Mars exploration missions with higher loads. Next-generation supersonic parachutes conducted by NASA, such as disksail parachutes, are alternatives to DGB parachutes. Disksail parachutes have larger porous gaps and smaller porous seams on the canopy surface than DGB parachutes. However, there are few studies on the aerodynamic characteristics of supersonic parachutes with different geometric porosity structures and locations.

Hence, the influence mechanism of porous seams or gaps and their locations on the performance of supersonic parachute systems in Martian atmospheric conditions remains unclear. In a research paper recently published in Space: Science and Technology, eight scholars from five organizations, including Central South University, Xi'An Jiaotong University, Nanjing University of Aeronautics and Astronautics, Beijing Institute of Space Mechanics and Electricity, and The Hong Kong Polytechnic University, together investigate the aerodynamic characteristics of the new supersonic parachute with different porosities and seam/gap positions and understand the influence mechanism of the porosity and the positions of porous structures on the aerodynamic performances of supersonic parachutes.

First, the authors introduce the parachute model in the study. The original parachute system model used in this study includes the capsule and canopy, as shown in Fig. 1. The canopy model is designed from the SSDS model in NASA's Low-Density Supersonic Decelerator (LDSD) flight tests, and the capsule model is consistent with the Mars Science Laboratory (MSL) probe model. The structure of the canopy model is divided into 4 parts along the X-axis direction from the mouth to the top of the canopy body: the canopy band, the ring 19-ring 16, the ring 15-ring 10, and the canopy disk with a vent. As shown in Fig. 2, the canopy model has 2 types of porosity structures, i.e., gap and seam. The top gap, G1, locates between ring 10 and the canopy disk, and its geometric porosity is 4%.

The middle gap, G2, locates between rings 16 and 15, and its geometric porosity is 3%. The seams locate between the other rings or the ring and canopy band. The order number of the seam is named from the upper ring. The gaps have large geometric porosity, and the seams have tiny geometric porosity. In this study, canopy models with different single-seam positions are designed (the top vent is retained for all the models), in which only one seam is open for a canopy model. Meanwhile, the top gap model, the G1 model, is a model that only retains the top gap of G1 and the top vent, and the middle gap model, the G2 model, only retains the middle gap of G2 and the top vent. Combining the above seams with different gaps, new canopy models with different seams and gaps are also designed. Furthermore, the canopy model is considered a rigid body in this work.

Then, authors set forth the freestream conditions and numerical methods used in the simulation. The freestream conditions used in the simulation are consistent with those of the working altitude of the supersonic parachute in the MSL mission and the working speeds of the parachute in the stable descent stage. As for numerical methods, the unsteady flows over the supersonic parachute system (i.e., different canopy models with the same MSL capsule) are studied by numerically solving the 3-dimensional compressible N-S equations. The finite volume method is adopted for spatial discretization, and the HLLC (Harten-Lax-van Leer-Contact) scheme is employed to calculate the inviscid flux term. Furthermore, the TVD polynomial interpolation scheme is used to avoid numerical oscillations. In addition, an implicit 2-time-step propulsion scheme is adopted to capture the complex unsteady flow field structures around the supersonic parachute with the time step of 1.0+ 10-4 s.

Last, the authors present the results and draw the conclusion. The numerical results are summarized as follows.

(1) The porosity structures of the canopy body have no significant effect on the flow field mode of the supersonic parachute system, and they have little effect on the pressure distribution of the capsule surface and the flow field structure around the capsule body.

(2) For the canopy models with single seams in the present study, the models with lower seams (lower side of canopy) have better drag performance, and the S11 and S17 models show larger drag coefficients and better stability performance. For the canopy models with a single gap, the drag coefficient of the G2 model (0.72) is significantly larger than that of the G1 model (0.64), while the lateral force coefficient fluctuation of G1 (0.072) is smaller than that of the G2 model (0.091).

(3) With the addition of different seams, the drag coefficient of G1S models is larger than that of the G1 model with a single G1. Compared with the original G1 model, the stability performance of the combined G1S models has no significant change. The drag performance of the combined G2S models with the seams decreases compared with the original G2 model; how- ever, the stability performance of the combined G2S models is improved compared with the original G2. Furthermore, when the combination of seam and gap farther apart is designed for a canopy, the pressure inside the canopy basically decreases compared with the original single model, while the combination of seam and gap with a short distance is designed for a canopy and the pressure change inside the canopy is minor.

The numerical results of this study show that the new supersonic parachutes with different porosity structures of seams, gaps, and their combinations exhibit significantly different aerodynamic performances. The next generation of parachutes with more complex combinations of seams and gaps should be designed to investigate their aerodynamic characteristics and influence mechanisms.

Research Report:Effect of Different Geometric Porosities on Aerodynamic Characteristics of Supersonic Parachutes

Related Links
Beijing Institute of Technology
Mars News and Information at MarsDaily.com
Lunar Dreams and more

Subscribe Free To Our Daily Newsletters
Tweet

RELATED CONTENT
The following news reports may link to other Space Media Network websites.
MARSDAILY
Can we see Mars' Breath in the Winter Cold: Sols 3907-3908
Pasadena CA (JPL) Aug 04, 2023
Earth planning date: Wednesday, August 2, 2023: We don't have a lot of power to play with today, so we have to be careful about how much time we give the different activities. As Arm Rover Planner, I got to sequence the contact science activities today. We start this two-sol plan with a nap to save up power. After waking up in the afternoon, we do a short block of imaging. Mastcam is taking three stereo mosaics. The first is a 4-frame mosaic of the Mt. Sharp foothills, specifically looking at an e ... read more

MARSDAILY
NASA's LRO observes crater likely from Luna 25 impact

Indian rover confirms sulphur on Moon's south pole

Renderings offer images of China's next-generation spacecraft

Korean lunar space environment payload ships to US for 2024 launch

MARSDAILY
China solicits names for manned lunar exploration vehicles

From rice to quantum gas: China's targets pioneering space research

China to launch "Innovation X Scientific Flight" program, applications open worldwide

Scientists reveal blueprint of China's lunar water-ice probe mission

MARSDAILY
NASA completes last OSIRIS-REx test before asteroid sample delivery

Psyche on track for liftoff next month

Newly discovered comet visible in night sky this weekend

Hera asteroid spacecraft assembled

MARSDAILY
SwRI will lead Hubble, Webb observations of Io, Jupiter's volcanic moon

In the service of planetary science, astrophysics and heliophysics

Mysterious Neptune dark spot detected from Earth for the first time

Neptune's Disappearing Clouds Linked to the Solar Cycle

MARSDAILY
Studying rivers from worlds away

Saturn's Rings shine in Webb's observations of Gas Giant

Key building block for life found at Saturn's moon Enceladus

MARSDAILY
Space Dynamics Lab-Built AWE Instrument Prepares for Launch at Space Center

Spire Global awarded $4.6M NASA contract to develop NOAA sounder

Remote-sensing satellite launched from Gobi Desert

China launches three remote-sensing satellites

MARSDAILY
China continues to make strides in space breeding technique

Artificial star

Station Hosts 11 Crewmates from Five Countries

A multinational crew blasts off from Florida, heading for the International Space Station

MARSDAILY
Newly discovered planet has longest orbit yet detected by the TESS mission

Thermometer molecule confirmed on exoplanet WASP-31b

New giant planet evidence of possible planetary collisions

Hot Jupiter blows its top

Subscribe Free To Our Daily Newsletters




The content herein, unless otherwise known to be public domain, are Copyright 1995-2024 - Space Media Network. All websites are published in Australia and are solely subject to Australian law and governed by Fair Use principals for news reporting and research purposes. AFP, UPI and IANS news wire stories are copyright Agence France-Presse, United Press International and Indo-Asia News Service. ESA news reports are copyright European Space Agency. All NASA sourced material is public domain. Additional copyrights may apply in whole or part to other bona fide parties. All articles labeled "by Staff Writers" include reports supplied to Space Media Network by industry news wires, PR agencies, corporate press officers and the like. Such articles are individually curated and edited by Space Media Network staff on the basis of the report's information value to our industry and professional readership. Advertising does not imply endorsement, agreement or approval of any opinions, statements or information provided by Space Media Network on any Web page published or hosted by Space Media Network. General Data Protection Regulation (GDPR) Statement Our advertisers use various cookies and the like to deliver the best ad banner available at one time. All network advertising suppliers have GDPR policies (Legitimate Interest) that conform with EU regulations for data collection. By using our websites you consent to cookie based advertising. If you do not agree with this then you must stop using the websites from May 25, 2018. Privacy Statement. Additional information can be found here at About Us.