// Copyright 2019-present, the HuggingFace Inc. team, The Google AI Language Team and Facebook, Inc. // Copyright 2019 Guillaume Becquin // Licensed under the Apache License, Version 2.0 (the "License"); // you may not use this file except in compliance with the License. // You may obtain a copy of the License at // http://www.apache.org/licenses/LICENSE-2.0 // Unless required by applicable law or agreed to in writing, software // distributed under the License is distributed on an "AS IS" BASIS, // WITHOUT WARRANTIES OR CONDITIONS OF ANY KIND, either express or implied. // See the License for the specific language governing permissions and // limitations under the License. extern crate anyhow; use std::sync::{Arc, RwLock}; use rust_bert::bart::{ BartConfigResources, BartMergesResources, BartModelResources, BartVocabResources, }; use rust_bert::pipelines::common::ModelResource; use rust_bert::pipelines::summarization::{SummarizationConfig, SummarizationModel}; use rust_bert::resources::{BufferResource, RemoteResource, ResourceProvider}; use tch::Device; fn main() -> anyhow::Result<()> { let input = ["In findings published Tuesday in Cornell University's arXiv by a team of scientists \ from the University of Montreal and a separate report published Wednesday in Nature Astronomy by a team \ from University College London (UCL), the presence of water vapour was confirmed in the atmosphere of K2-18b, \ a planet circling a star in the constellation Leo. This is the first such discovery in a planet in its star's \ habitable zone — not too hot and not too cold for liquid water to exist. The Montreal team, led by Björn Benneke, \ used data from the NASA's Hubble telescope to assess changes in the light coming from K2-18b's star as the planet \ passed between it and Earth. They found that certain wavelengths of light, which are usually absorbed by water, \ weakened when the planet was in the way, indicating not only does K2-18b have an atmosphere, but the atmosphere \ contains water in vapour form. The team from UCL then analyzed the Montreal team's data using their own software \ and confirmed their conclusion. This was not the first time scientists have found signs of water on an exoplanet, \ but previous discoveries were made on planets with high temperatures or other pronounced differences from Earth. \ \"This is the first potentially habitable planet where the temperature is right and where we now know there is water,\" \ said UCL astronomer Angelos Tsiaras. \"It's the best candidate for habitability right now.\" \"It's a good sign\", \ said Ryan Cloutier of the Harvard–Smithsonian Center for Astrophysics, who was not one of either study's authors. \ \"Overall,\" he continued, \"the presence of water in its atmosphere certainly improves the prospect of K2-18b being \ a potentially habitable planet, but further observations will be required to say for sure. \" \ K2-18b was first identified in 2015 by the Kepler space telescope. It is about 110 light-years from Earth and larger \ but less dense. Its star, a red dwarf, is cooler than the Sun, but the planet's orbit is much closer, such that a year \ on K2-18b lasts 33 Earth days. According to The Guardian, astronomers were optimistic that NASA's James Webb space \ telescope — scheduled for launch in 2021 — and the European Space Agency's 2028 ARIEL program, could reveal more \ about exoplanets like K2-18b."]; let weights = Arc::new(RwLock::new(get_weights()?)); let summarization_model = SummarizationModel::new(config(Device::Cpu, weights.clone()))?; // Credits: WikiNews, CC BY 2.5 license (https://en.wikinews.org/wiki/Astronomers_find_water_vapour_in_atmosphere_of_exoplanet_K2-18b) let output = summarization_model.summarize(&input)?; for sentence in output { println!("{sentence}"); } let summarization_model = SummarizationModel::new(config(Device::cuda_if_available(), weights))?; // Credits: WikiNews, CC BY 2.5 license (https://en.wikinews.org/wiki/Astronomers_find_water_vapour_in_atmosphere_of_exoplanet_K2-18b) let output = summarization_model.summarize(&input)?; for sentence in output { println!("{sentence}"); } Ok(()) } fn get_weights() -> anyhow::Result, anyhow::Error> { let model_resource = RemoteResource::from_pretrained(BartModelResources::DISTILBART_CNN_6_6); Ok(std::fs::read(model_resource.get_local_path()?)?) } fn config(device: Device, model_data: Arc>>) -> SummarizationConfig { let config_resource = Box::new(RemoteResource::from_pretrained( BartConfigResources::DISTILBART_CNN_6_6, )); let vocab_resource = Box::new(RemoteResource::from_pretrained( BartVocabResources::DISTILBART_CNN_6_6, )); let merges_resource = Box::new(RemoteResource::from_pretrained( BartMergesResources::DISTILBART_CNN_6_6, )); let model_resource = ModelResource::Torch(Box::new(BufferResource { data: model_data })); SummarizationConfig { model_resource, config_resource, vocab_resource, merges_resource: Some(merges_resource), num_beams: 1, length_penalty: 1.0, min_length: 56, max_length: Some(142), device, ..Default::default() } }