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Isaac Newton Telescope#HARPS3

{{short description|Optical telescope}}

{{for|the type of telescope invented by Isaac Newton|Newtonian telescope}}

{{Infobox telescope

| locmapin= Spain Canary Islands}}

The Isaac Newton Telescope or INT is a 2.54 m (100 in) optical telescope run by the Isaac Newton Group of Telescopes at Roque de los Muchachos Observatory on La Palma in the Canary Islands since 1984.

Originally the INT was situated at Herstmonceux Castle in Sussex, England, which was the site of the Royal Greenwich Observatory after it moved away from Greenwich due to light pollution. It was inaugurated in 1967 by Queen Elizabeth II.{{cite journal

| last1 = Smith

| first1 = F. Graham

| author-link = Francis Graham Smith

| last2 = Dudley

| first2 = J.

| title = The Isaac Newton Telescope

| journal = Journal for the History of Astronomy

| volume = 12

| number = 1

| pages = 1–18

| date = 1982

| bibcode = 1982JHA....13....1S

| url = http://articles.adsabs.harvard.edu/full/1982JHA....13....1S

| access-date = 18 February 2016

| doi = 10.1177/002182868201300101

| s2cid = 116989341

}}

Herstmonceux suffered from poor weather, and the advent of mass air travel made it plausible for UK astronomers to run an overseas observatory. In 1979, the INT was shipped to La Palma, where it has remained ever since. It saw its second first light in 1984, with a video camera.{{Cite web|url=http://www.ing.iac.es/PR/chronology.html|title = Chronology of the Isaac Newton Group of Telescopes}} A major change was the mirror was now made of the new type Zerodur glass, as compared to the old mirror's Pyrex glass.{{Cite book|url=https://books.google.com/books?id=klU0AQAAIAAJ&q=Zerodur+mirror+INT+100+inch|title=Yearbook of Astronomy|last1=Porter|first1=John Guy|last2=Moore|first2=Patrick|date=1984|publisher=W. W. Norton.|isbn=9780393301472|language=en}}

Until 2024, the main instruments were the Wide Field Camera (WFC) and Intermediate Dispersion Spectrograph (IDS). WFC is a four CCD photographic prime-focus instrument with a relatively large 0.56×0.56 square degree field of view, which was commissioned in 1997. IDS is a medium-low resolution optical spectrograph (R 550-9375).{{Cite web |title=Gratings |url=https://www.ing.iac.es/astronomy/instruments/ids/idsgrat_tables.html |access-date=2024-08-25 |website=www.ing.iac.es}} As of mid 2024 the INT is undergoing upgrades in preparation for the installation of HARPS3,{{Cite web |title=ING Instrumentation Update 2024 - 2025 |url=https://www.ing.iac.es//astronomy/instr.html |access-date=2024-08-25 |website=www.ing.iac.es}} after which it will be the main instrument.

The old site of the INT is now the Observatory Science Centre at Herstmonceux, and it is known for its distinctive greened copper dome and various science and astronomy activities.{{Cite book|url=https://books.google.com/books?id=kPmODgAAQBAJ&q=Herstmonceux+Science+Center&pg=PA26|title=Astronomy Adventures and Vacations: How to Get the Most Out of Astronomy in Your Leisure Time|last=Treadwell|first=Timothy|date=2017-03-29|publisher=Springer|isbn=9783319500027|language=en}}

Summary Background up to 1979

File:Herstmonceux trig with Isaac Newton telescope - geograph.org.uk - 67765.jpg

File:Herstmonceux Observatory aerial view.jpg

The United States gifted a 98-inch mirror in 1949 to the United Kingdom.{{Cite web|url=http://www.ing.iac.es/Astronomy/telescopes/int/hist.html|title=History of Isaac Newton Telescope|website=www.ing.iac.es|access-date=2019-10-17}} (In a telescope this could establish the 3rd largest in the World, behind only the Hale and Hooker telescopes at that time). After ten years the mount was ordered for the telescope, and in 1959 construction began on what would be the INT, and it was completed by 1965; first light at Herstmonceux was conducted that year.

The mirror was ground by Grubb in the 1950s, although until 1956, according to Observatories and Telescopes of Modern Times, there was some consideration for buying a new 74-inch from Grubb.{{Cite book|url=https://books.google.com/books?id=o0xsDQAAQBAJ&q=98+inch+mirror+for+INT+grinding&pg=PA119|title=Observatories and Telescopes of Modern Times|last=Leverington|first=David|date=2017|publisher=Cambridge University Press|isbn=9780521899932|language=en}} The Royal Greenwich Observatory completed its move to Herstmonceux in 1956.

A short film was published in 1956 that featured the grinding of the 98-inch mirror blank for the Isaac Newton Telescope by Grubb Parsons.{{Cite web|url=http://www.yorkshirefilmarchive.com/film/grinding-98-mirror-isaac-newton-telescope|title=GRINDING A 98" MIRROR FOR THE ISAAC NEWTON TELESCOPE {{!}} Yorkshire Film Archive|website=www.yorkshirefilmarchive.com|access-date=2019-10-17|archive-date=2019-10-17|archive-url=https://web.archive.org/web/20191017215948/http://www.yorkshirefilmarchive.com/film/grinding-98-mirror-isaac-newton-telescope|url-status=dead}} (reflecting telescopes of this type need the glass blank ground into a precise shape, which can take years).

The telescope's first light (first, first light) occurred in 1965, and it was dedicated in 1967.{{Cite book|url=https://books.google.com/books?id=SYi-BwAAQBAJ&q=isaac+newton+telescope+first+light&pg=PA95|title=Organizations and Strategies in Astronomy|last=HECK|first=Andre|date=2013-06-05|publisher=Springer Science & Business Media|isbn=9781402025716|language=en}}{{Cite book|url=https://books.google.com/books?id=KLKNBAAAQBAJ&q=Isaac+Newton+Telescope+queen+elizabeth+december+1%2C+1967&pg=PA362|title=Galactic Encounters: Our Majestic and Evolving Star-System, From the Big Bang to Time's End|last1=Sheehan|first1=William|last2=Conselice|first2=Christopher J.|date=2014-09-17|publisher=Springer|isbn=9780387853475|language=en}}

On December 1, 1967, the Isaac Newton Telescope of the Royal Greenwich Observatory at Herstmonceux was inaugurated (dedicated) by Queen Elizabeth II.{{Cite web|url=http://www.ing.iac.es/Astronomy/telescopes/int/hist.html|title = History of Isaac Newton Telescope}}{{Cite web|url=https://www.skyatnightmagazine.com/space-science/50-years-of-the-isaac-newton-telescope/|title=50 years of the Isaac Newton Telescope|website=Sky At Night magazine|access-date=2019-10-17}} One of the accomplishments with the telescope was the observations of Cygnus X-1.

In the late 1960s, a concept was developed for a Northern Hemisphere Observatory, that culminated in the project for an international observatory in the Canary Islands; Mauna Kea in Hawaii was also considered for the location.{{Cite interview |last=Jefferies |first=John |interviewer=Spencer Weart |title=John Jefferies |type=Oral history |url=https://www.aip.org/history-programs/niels-bohr-library/oral-histories/4693 |access-date=2023-01-26 |publisher=American Institute of Physics |date=1977-07-29}} Although the telescope was acquitting itself, the weather at the site less so. This eventually led to the plan to move the telescope to a new observatory, which would occur in the next decade and into the early 1980s.

The 'last light' for the original Isaac Newton Telescope was in May 1979.{{Cite book|url=https://books.google.com/books?id=uAhBAQAAIAAJ&q=INT+at+la+palma+new+mount+100+inch+mirror|title=Journal for the History of Astronomy|date=1982|publisher=Science History Publications|language=en}} The new telescope for the island had so many new parts however, it was deemed possible in the mid-1980s to essentially fork the telescope design into two working telescopes with some rejuvenation. This would mean having another functioning telescope at Sussex; however, this project was terminated. One issue is that it would mean operating two telescopes, and the focus at that time had shifted to operating the new INT on the island. The old site would eventually be turned into a science museum with much of the old telescopes left as they were.{{Cite book|url=https://books.google.com/books?id=3mfgBwAAQBAJ&q=INT+at+la+palma+new+mount+100+inch+mirror&pg=PA92|title=Eyes on the Universe: The Story of the Telescope|last=Moore|first=Patrick|date=2012-12-06|publisher=Springer Science & Business Media|isbn=9781447106272|language=en}}

The old observatory buildings remain by the Castle, and it is the site of the Herstmonceux Science Centre{{Cite book|url=https://books.google.com/books?id=lwUNAQAAMAAJ&q=Herstmonceux+Science+Centre|title=Perception|date=1998|publisher=Pion Limited|language=en}} (aka Observatory Science Centre at Herstmonceux).

Image:Royal Greenwich Observatory, Herstmonceux - April 2012.jpg

Technical detail since 1984

The La Palma INT is a Cassegrain telescope, with a 2.54 m (100 in) diameter primary mirror and a focal length of 8.36 m (329 in). The mirror weighs 4361 kg (9614 lb), and is supported by a polar disc/fork type equatorial mounting. The total weight of the telescope is around 90 tons. The f/3.29 Prime focus, used with the WFC, allows an unvignetted field of view of 40 arcminutes (approximately 0.3 square degrees). There is also a secondary focal station, the f/15 Cassegrain focus, which possesses a 20 arcminute field of view and is the mount point for the IDS. The telescope's second first light was done by video.{{cite book|author=Reed Business Information|title=New Scientist|url=https://archive.org/details/bub_gb_rot6QG6G6bgC|date=February 16, 1984|publisher=Reed Business Information|page=[https://archive.org/details/bub_gb_rot6QG6G6bgC/page/n17 16]}}

The new 100 inch Zerodur-glass mirror arrived at La Palma in December 1982.

The pointing accuracy of the telescope is around 5 arcseconds, but a sophisticated autoguider, which tracks a given guide star and makes small corrections to the telescope tracking, allows a guiding accuracy of better than an arcsecond on better than 20th magnitude guide stars in support of the typical 0.8–1.5 arcsec seeing at the INT.

Image:Isaac Newton Telescope main mirror.jpg

Contemporaries

The Isaac Newton Telescope was a very large telescope for its day, and the largest in England. It was a little smaller in aperture than the 100-inch Hooker telescope in the United States, but much newer. It originally had a 98-inch mirror when in England, but was given a new, larger 100-inch mirror by Grubb Parsons after the move.{{cite journal

| last = Macdonald

| first = Lee T.

| title = 'A Large Chunk of Glass': The 98-inch Mirror of the Isaac Newton Telescope, 1945–1959

| journal = The Antiquarian Astronomer

| volume = 6

| pages = 59–73

| publisher = Society for the History of Astronomy

| date = 2012

| bibcode = 2012AntAs...6...59M

| url = http://articles.adsabs.harvard.edu/full/2012AntAs...6...59M

| access-date = 6 November 2015

}}{{cite book

| last = McCrea

| first = William Hunter

| title = Royal Greenwich Observatory : an Historical Review Issued on the Occasion of its Tercentenary

| publisher = Her Majesty's Stationery Office

| date = 1975

| location = London

| bibcode = 1975rgo..book.....M

}}

=1967=

The INT was inaugurated by Queen Elizabeth II in 1967. The largest optical telescopes in 1967 included:

class="wikitable" style="font-size: 90%; text-align: center;"
#BBEEFF;"| #

! style="background:#bef;"| Name /
Observatory

! style="width:40px; background:#bef;"| Image

! style="background:#bef;"| Aperture

! style="background:#bef;"| Altitude

! style="background:#bef;"| First
Light

1

| 5m Hale Telescope
Palomar Obs.

| 50px

| 200″
508 cm

| 1713 m
(5620 ft)

| 1949

2

| C. Donald Shane telescope
Lick Observatory

| 40px

| 120″
305 cm

| 1283 m
(4209 ft)

| 1959

3

| Shajn 2.6m (Crimean 102 in.)
Crimean Astrophysical Obs.

| 40px

| 102″
260 cm

| 600 m
(1969 ft) {{cite web |url=http://quake.stanford.edu/~crao/craoinfo/general.html |title=Crimean Observatory: General Information |access-date=2010-01-13 |url-status=dead |archive-url=https://web.archive.org/web/20110720045836/http://quake.stanford.edu/~crao/craoinfo/general.html |archive-date=2011-07-20 }}

| 1961

4

| Hooker Telescope
Mount Wilson Obs.

| 30px

| 100″
254 cm

| 1742 m
(5715 ft)

| 1917

style="background:#DAF7A6"

! 5

| Isaac Newton Telescope
Royal Greenwich Obs. (1967-1979)

| 50px

| 98″
249 cm

|

| 1965

6

| KPNO 2.1 m Telescope
Kitt Peak National Obs.

|

| 83″
211 cm

| 2,070 m
6791 ft

| 1964

7

| Otto Struve Telescope
McDonald Obs.

| 40px

| 82″
208 cm

| 2070 m
(6791 ft)

| 1939

=1984=

INT began its new life atop the Spanish island of La Palma in the Canary Islands in 1984, with a new mirror and dome. Large visible-light optical ground telescopes in 1984 included:

class="wikitable" style="font-size: 90%; text-align: center;"
style="background:#bef;"|

! style="background:#bef;"| Name /
Observatory

! style="width:40px; background:#bef;"| Image

! style="background:#bef;"| Aperture

! style="background:#bef;"| M1
Area

! style="background:#bef;"| Altitude

! style="background:#bef;"| First
Light

n

| BTA-6
Special Astrophysical Obs

| 50px

| 238″
605 cm

| 26 m2

| 2070 m
(6791 ft)

| 1975

n

| Hale Telescope
Palomar Obs.

| 50px

| 200″
508 cm

| 20 m2

| 1713 m
(5620 ft)

| 1949

n

| Multiple Mirror Telescope
Fred Lawrence Whipple Obs.

| 40px

| 1.8 m x 6
6+ or 4.7 m

| m2

| 2617 m
(8585 ft)

| 1979

n

| Mayall Telescope
Kitt Peak National Obs.

| 40px

| 158″
401 cm

| 10 m2

| 2120 m
(6955 ft)

| 1973

s

| CTIO 4m/Blanco
CTIO Obs.

| 30px

| 158″
401 cm

| 10 m2

| 2200 m
(7217 ft)

| 1976

s

| Anglo-Australian Telescope
Siding Spring Obs.

| 50px

| 153″
389 cm

| m2

| 1742 m
(5715 ft)

| 1974

n

| CFH telescope
Mauna Kea Obs.

| 50px

| 141″
358 cm

| m2

| 4205 m
(13,800 ft)

| 1979

s

| ESO 3.6 m Telescope
ESO La Silla Obs.

| 32px

| 140″
357 cm

| 8.8 m2

| 2400 m
(7874 ft)

| 1977

n

| MPI-CAHA 3.5m
Calar Alto Obs.

| 40px

| 138″
350 cm

| 9 m2
[http://www.caha.es/CAHA/Telescopes/3.5m.html CA 3.5 Specs]

| 2168 m
(7,113 ft)

| 1984

n

| Shane Telescope
Lick Observatory

| 40px

| 120″
305 cm

| m2

| 1283 m
(4209 ft)

| 1959

n

| Harlan J. Smith Telescope
McDonald Observatory

| 40px

| 107″
270 cm

|

| 2070 m
(6791 ft)

| 1968

n

| Shajn 2.6m (Crimean 102 in.)
Crimean Astrophysical Obs.

| 40px

| 102″
260 cm

|

| 600 m
(1969 ft)

| 1961

n

| BAO 2.6 telescope
Byurakan Astrophysical Obs.

|

| 102″
260 cm

|

| 1500 m
(5000 ft)

| 1976

style="background:#DAF7A6"

! n

| Isaac Newton Telescope
ORM Obs. (1980–Present)

| 50px

| 100″
254 cm

|

| 2396 m
(7,860 ft)

| 1984

s

| du Pont telescope
Las Campanas Obs.

| 40px

| 100″
254 cm

|

| 2380 m
(7841 ft)

| 1976

n

| Hooker Telescope
Mount Wilson Obs.

| 30px

| 100″
254 cm

|

| 1742 m
(5715 ft)

| 1917

HARPS3

The High Accuracy Radial velocity Planet Searcher 3 (HARPS3) is a high resolution Echelle-type spectrograph that will be installed onto the telescope{{cite book |last1=Jentink |first1=Casper Farret| last2=Mortier| first2=Annelies|last3=Snik|first3=Frans|last4=Dorval| first4=Patrick|last5=Thompson|first5=Samantha J.|last6=Navarro|first6=Ramon|last7=Naylor|first7=Tim|title=Ground-based and Airborne Telescopes IX |chapter=ABORAS: Polarimetric, 10cm/S RV observations of the Sun as a star |editor-first1=Heather K |editor-first2=Jason |editor-first3=Tomonori |editor-last1=Marshall |editor-last2=Spyromilio |editor-last3=Usuda |display-authors=3|arxiv=2207.04804|date=2022-07-11|volume=12182 |page=146 |doi=10.1117/12.2627113 |bibcode=2022SPIE12182E..31F |isbn=9781510653450 |s2cid=250425755 }} and aims to start observations in March 2025.{{Cite web |title=ING Instrumentation Update 2024 - 2025 |url=https://www.ing.iac.es/astronomy/instr.html |access-date=2025-01-06 |website=Isaac Newton Group of Telescopes}} It is being built as part of the Terra Hunting Experiment - a future 10 year radial velocity measurement program to discover Earth-like exoplanets.{{cite web |url=https://www.terrahunting.org/harps3.html#:~:text=Aka%20RoboHARPS%20and%20the%20workhorse,Palma%20in%20the%20Canary%20Islands.|title=HARPS3 Aka RoboHARPS and the workhorse of the Terra Hunting Experiment|author=|date=|website=Terra Hunting Experiment|publisher= |access-date=2022-07-12 |quote=}}{{Obsolete source|reason=Strangely coincidental that the Terra Hunting Experiment's website closed the very day after I brought light to its existence in a Wikipedia article.|date=July 2022}}{{cite journal|last1=Hall|first1=Richard D|last2=Thompson|first2=Samantha J|last3=Handley|first3=Will|last4=Queloz|first4=Didier|display-authors=3|title=On the Feasibility of Intense Radial Velocity Surveys for Earth-Twin Discoveries|journal=Monthly Notices of the Royal Astronomical Society|publisher=Oxford University Press (OUP)|volume=479|issue=3|date=2018-06-05|doi=10.1093/mnras/sty1464|doi-access=free|pages=2968–2987|arxiv=1806.00518}} It has a goal to achieve 10 cm/s radial velocity precision.{{cite conference|last1=Thompson|first1=Samantha J.|last2=Queloz|first2=Didier|authorlink2=Didier Queloz|last3=Baraffe|first3=Isabelle|authorlink3=Isabelle Baraffe|last4=Brake|first4=Martyn|last5=Dolgopolov|first5=Andrey|last6=Fisher|first6=Martin|last7=Fleury|first7=Michel|last8=Geelhoed|first8=Joost|last9=Hall|first9=Richard|last10=González Hernández|first10=Jonay I.|last11=ter Horst|first11=Rik|last12=Kragt|first12=Jan|last13=Navarro|first13=Ramón|last14=Naylor|first14=Tim|last15=Pepe|first15=Francesco|last16=Piskunov|first16=Nikolai|last17=Rebolo|first17=Rafael|last18=Sander|first18=Louis|last19=Ségransan|first19=Damien|last20=Seneta|first20=Eugene|last21=Sing|first21=David|last22=Snellen|first22=Ignas|last23=Snik|first23=Frans|last24=Spronck|first24=Julien|last25=Stempels|first25=Eric|last26=Sun|first26=Xiaowei|last27=Santana Tschudi|first27=Samuel|last28=Young|first28=John|editor-first1=Christopher J |editor-first2=Luc |editor-first3=Hideki |editor-last1=Evans |editor-last2=Simard |editor-last3=Takami |title=Ground-based and Airborne Instrumentation for Astronomy VI |display-authors=3

|chapter=HARPS3 for a roboticized Isaac Newton Telescope|publisher=SPIE|date=2016-08-09|volume=9908 |pages=99086F |doi=10.1117/12.2232111|arxiv=1608.04611}}

See also

References

{{reflist}}

External links

  • [http://www.ing.iac.es/Astronomy/telescopes/int/index.html INT Homepage]
  • {{cite web|last=Merrifield|first=Michael|title=Isaac Newton Telescope|url=http://www.deepskyvideos.com/videos/telescopes/INT.html|work=Deep Sky Videos|publisher=Brady Haran|author2=Barrena, Rafael}}
  • [https://www.alamy.com/stock-photo-mirror-glass-of-the-isaac-newton-telescope-in-herstmonceux-16804170.html Stock Photo of old 98 inch mirror at Herstmonceux Science Center]
  • [https://www.theguardian.com/science/2012/jan/30/isaac-newton-telescope INT article] (2012)

{{Isaac Newton|state=collapsed}}

Category:Reflecting telescopes

Category:Astronomical observatories in La Palma

Category:1967 establishments in Spain